Astro arXiv | all categories
By Corentin Cadiou
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Episodes: 1314
Description
Daily Astro papers on the arXiv in all categories.
| Episode | Date |
|---|---|
|
Extreme nature of four blue-excess dust-obscured galaxies revealed by optical spectroscopy
|
Nov 30, 2022 |
|
The binary and the disk: the beauty is found within NGC3132 with JWST
|
Nov 30, 2022 |
|
The radio structure of the γ -ray narrow-line Seyfert 1 galaxy SDSS J211852 96 - 073227 5
|
Nov 30, 2022 |
|
Dynamics in the outskirts of four Milky Way globular clusters: it's the tides that dominate
|
Nov 30, 2022 |
|
The H α and O III λ5007 Luminosity Functions of 1 2
|
Nov 30, 2022 |
|
A Component of the Smith High Velocity Cloud Now Crossing the Galactic Plane
|
Nov 30, 2022 |
|
The Dark Energy Survey Year 3 high redshift sample: Selection, characterization and analysis of galaxy clustering
|
Nov 30, 2022 |
|
Lopsided Galaxies in a cosmological context: a new galaxy-halo connection
|
Nov 30, 2022 |
|
The Second Radio Synchrotron Background Workshop: Conference Summary and Report
|
Nov 30, 2022 |
|
Evidence for supernova feedback sustaining gas turbulence in nearby star-forming galaxies
|
Nov 30, 2022 |
|
The volumetric star formation law in nearby galaxies
|
Nov 30, 2022 |
|
Merger Signatures are Common, but not Universal, In Massive, Recently-Quenched Galaxies at z~0 7
|
Nov 30, 2022 |
|
Reconstructing the extended structure of multiple sources strongly lensed by the ultra-massive elliptical galaxy SDSS J0100+1818
|
Nov 30, 2022 |
|
Morphology & Environment's Role on the Star Formation Rate -- Stellar Mass Relation in COSMOS from 0 < z < 3 5
|
Nov 30, 2022 |
|
VERTICO III: The Kennicutt-Schmidt relation in Virgo cluster galaxies
|
Nov 30, 2022 |
|
Stellar Escape from Globular Clusters I: Escape Mechanisms and Properties at Ejection
|
Nov 30, 2022 |
|
Dissecting the interstellar medium of a z=6 3 galaxy: X-shooter spectroscopy and HST imaging of the afterglow and environment of the Swift GRB 210905A
|
Nov 30, 2022 |
|
MUSE-ALMA Haloes VII: Survey Science Goals & Design, Data Processing and Final Catalogues
|
Nov 30, 2022 |
|
Weak Lensing Tomographic Redshift Distribution Inference for the Hyper Suprime-Cam Subaru Strategic Program three-year shape catalogue
|
Nov 30, 2022 |
|
NICMOS Kernel-Phase Interferometry II: Demographics of Nearby Brown Dwarfs
|
Nov 30, 2022 |
|
Calibrating cosmological simulations with implicit likelihood inference using galaxy growth observables
|
Nov 30, 2022 |
|
Parametrized Asymmetric Neutral hydrogen Disk Integrated Spectrum Characterization PANDISC I: Introduction to A Physically Motivated H I Model
|
Nov 30, 2022 |
|
Gravity in the Local Universe : density and velocity fields using CosmicFlows-4
|
Nov 30, 2022 |
|
On the sociology and hierarchy of voids: a study of seven CAVITY nearby galaxy voids and their dynamical CosmicFlows-3 environment
|
Nov 30, 2022 |
|
Orientations of DM Halos in FIRE-2 Milky Way-mass Galaxies
|
Nov 30, 2022 |
|
Updating constraints on phantom crossing f T gravity
|
Nov 30, 2022 |
|
The AstroSat UV Deep Field North: the far and near ultraviolet photometric catalog
|
Nov 30, 2022 |
|
The Complex Structure of the Bulge of M31
|
Nov 30, 2022 |
|
EIGER III JWST NIRCam observations of the ultra-luminous high-redshift quasar J0100+2802
|
Nov 30, 2022 |
|
Star & planet formation: Upcoming opportunities in the space-based infrared
|
Nov 30, 2022 |
|
The dynamical state of the globular clusters Rup 106 and IC 4499
|
Nov 30, 2022 |
|
Peering into the Milky Way by FAST: IV Identification of two new Galactic supernova remnants G203 1+6 6 and G206 7+5 9
|
Nov 30, 2022 |
|
Peering into the Milky Way by FAST: III Magnetic fields in the Galactic halo and farther spiral arms revealed by the Faraday effect of faint pulsars
|
Nov 30, 2022 |
|
Peering into the Milky Way by FAST: II Ionized gas in the inner Galactic disk revealed by the piggyback line observations of the FAST GPPS survey
|
Nov 30, 2022 |
|
Peering into the Milky Way by FAST: I Exquisite HI structures in the inner Galactic disk from the piggyback line observations of the FAST GPPS survey
|
Nov 30, 2022 |
|
Shattering and growth of cold clouds in galaxy clusters: the role of radiative cooling, magnetic fields and thermal conduction
|
Nov 30, 2022 |
|
Large-scale geometry of the Universe
|
Nov 30, 2022 |
|
BASS XXXIX: Swift-BAT AGN with changing-look optical spectra
|
Nov 30, 2022 |
|
Microlensing of gravitational waves by dark matter structures
|
Nov 30, 2022 |
|
Real-world CMB lensing quadratic estimator power spectrum response
|
Nov 30, 2022 |
|
Scattering variability detected from the circumsource medium of FRB 20190520B
|
Nov 30, 2022 |
|
Panchromatic HST WFC3 Imaging Studies of Young, Rapidly Evolving Planetary Nebulae II NGC 7027
|
Nov 30, 2022 |
|
Shock-induced stripping of satellite ISM CGM in IllustrisTNG clusters at z sim0
|
Nov 30, 2022 |
|
Insights on the origin of ORCs from cosmological simulations
|
Nov 30, 2022 |
|
On the ages of bright galaxies sim 500 Myr after the Big Bang: insights into star formation activity at z gtrsim 15 with JWST
|
Nov 30, 2022 |
|
NGC 7538 IRS2 in NeII : Shell and Cavity Kinematics of a Compact HII Region
|
Nov 30, 2022 |
|
A Ghost in Boötes: The Least Luminous Disrupted Dwarf Galaxy
|
Nov 30, 2022 |
|
Constraints on dark matter annihilation and decay from the large-scale structure of the nearby universe
|
Nov 30, 2022 |
|
Accurate modelling of extragalactic microlensing by compact objects
|
Nov 30, 2022 |
|
The diversity of rotation curves of simulated galaxies with cusps and cores
|
Nov 30, 2022 |
|
New constraints on the dark matter density profiles of dwarf galaxies from proper motions of globular cluster streams
|
Nov 30, 2022 |
|
Accelerating BAO Scale Fitting Using Taylor Series
|
Nov 30, 2022 |
|
Line-of-sight effects in strong gravitational lensing
|
Nov 30, 2022 |
|
Effects of the Central Mass Concentration on Bar Formation in Disk Galaxies
|
Nov 30, 2022 |
|
RSD measurements from BOSS galaxy power spectrum using the halo perturbation theory model
|
Nov 30, 2022 |
|
A non-repeating fast radio burst in a dwarf host galaxy
|
Nov 30, 2022 |
|
High- z Quasar Candidate Archive: A Spectroscopic Catalog of Quasars and Contaminants in Various Quasar Searches
|
Nov 30, 2022 |
|
Improving Performance in Java: TOPCAT and STILTS
|
Nov 30, 2022 |
|
Insights on the origin of ORCs from cosmological simulations
|
Nov 30, 2022 |
|
Large-scale geometry of the Universe
|
Nov 30, 2022 |
|
Laue lenses: Focusing optics for hard X soft Gamma-ray Astronomy
|
Nov 30, 2022 |
|
Nitrogen as a Tracer of Giant Planet Formation II : Comprehensive Study of Nitrogen Photochemistry and Implications for Observing NH3 and HCN in Transmission and Emission Spectra
|
Nov 30, 2022 |
|
Nitrogen as a Tracer of Giant Planet Formation I : A Universal Deep Adiabatic Profile and Semi-analytical Predictions of Disequilibrium Ammonia Abundances in Warm Exoplanetary Atmospheres
|
Nov 30, 2022 |
|
NGC 7538 IRS2 in NeII : Shell and Cavity Kinematics of a Compact HII Region
|
Nov 30, 2022 |
|
The Radial Profile of Dust Grain Size in the Protoplanetary Disk of DS Tau
|
Nov 30, 2022 |
|
Impact of galactic distributions in celestial capture of dark matter
|
Nov 30, 2022 |
|
Effects of the Central Mass Concentration on Bar Formation in Disk Galaxies
|
Nov 30, 2022 |
|
Modeling the Evolution of Silicate Volatile Accretion Discs around White Dwarfs
|
Nov 30, 2022 |
|
The MUSE second-generation VLT instrument
|
Nov 30, 2022 |
|
RSD measurements from BOSS galaxy power spectrum using the halo perturbation theory model
|
Nov 30, 2022 |
|
A non-repeating fast radio burst in a dwarf host galaxy
|
Nov 30, 2022 |
|
Panel Discussion: Practical Problem Solving for Machine Learning
|
Nov 30, 2022 |
|
Extreme nature of four blue-excess dust-obscured galaxies revealed by optical spectroscopy
|
Nov 30, 2022 |
|
The binary and the disk: the beauty is found within NGC3132 with JWST
|
Nov 30, 2022 |
|
Determining Dust Properties in Protoplanetary Disks: SED-derived Masses and Settling With ALMA
|
Nov 30, 2022 |
|
Using simulated Tianqin gravitational wave data and electromagnetic wave data to study the coincidence problem and Hubble tension problem
|
Nov 30, 2022 |
|
JWST NIRCam Defocused Imaging: Photometric Stability Performance and How it Can Sense Mirror Tilts
|
Nov 30, 2022 |
|
Dynamics and Origins of the Near-Resonant Kepler Planets
|
Nov 30, 2022 |
|
The radio structure of the γ -ray narrow-line Seyfert 1 galaxy SDSS J211852 96 - 073227 5
|
Nov 30, 2022 |
|
Trace the Accretion Geometry of H 1743--322 with Type C Quasi-periodic Oscillations in Multiple Outbursts
|
Nov 30, 2022 |
|
Dynamics in the outskirts of four Milky Way globular clusters: it's the tides that dominate
|
Nov 30, 2022 |
|
The H α and O III λ5007 Luminosity Functions of 1 2
|
Nov 30, 2022 |
|
SPICE PSF Correction: General Framework and Capability Demonstration
|
Nov 30, 2022 |
|
A Component of the Smith High Velocity Cloud Now Crossing the Galactic Plane
|
Nov 30, 2022 |
|
The Dark Energy Survey Year 3 high redshift sample: Selection, characterization and analysis of galaxy clustering
|
Nov 30, 2022 |
|
First in-situ observation of surface Alfvén waves in ICME flux rope
|
Nov 30, 2022 |
|
Lopsided Galaxies in a cosmological context: a new galaxy-halo connection
|
Nov 30, 2022 |
|
Geomagnetic storm forecasting from solar coronal holes
|
Nov 30, 2022 |
|
Studying cosmic ray sources using intergalactic electromagnetic cascades
|
Nov 30, 2022 |
|
Optimal frequency-domain analysis for spacecraft time series: Introducing the missing-data multitaper power spectrum estimator
|
Nov 30, 2022 |
|
The Second Radio Synchrotron Background Workshop: Conference Summary and Report
|
Nov 30, 2022 |
|
Evidence for supernova feedback sustaining gas turbulence in nearby star-forming galaxies
|
Nov 30, 2022 |
|
The volumetric star formation law in nearby galaxies
|
Nov 30, 2022 |
|
The Birth of a Relativistic Jet Following the Disruption of a Star by a Cosmological Black Hole
|
Nov 30, 2022 |
|
Merger Signatures are Common, but not Universal, In Massive, Recently-Quenched Galaxies at z~0 7
|
Nov 30, 2022 |
|
A localized kinematic structure detected in atomic carbon emission spatially coincident with a proposed protoplanet in the HD 163296 disk
|
Nov 30, 2022 |
|
Multiplicity of TeV muons in air showers detected with IceTop and IceCube
|
Nov 30, 2022 |
|
A very luminous jet from the disruption of a star by a massive black hole
|
Nov 30, 2022 |
|
Reconstructing the extended structure of multiple sources strongly lensed by the ultra-massive elliptical galaxy SDSS J0100+1818
|
Nov 30, 2022 |
|
Morphology & Environment's Role on the Star Formation Rate -- Stellar Mass Relation in COSMOS from 0 < z < 3 5
|
Nov 30, 2022 |
|
VERTICO III: The Kennicutt-Schmidt relation in Virgo cluster galaxies
|
Nov 30, 2022 |
|
Stellar Escape from Globular Clusters I: Escape Mechanisms and Properties at Ejection
|
Nov 30, 2022 |
|
Dissecting the interstellar medium of a z=6 3 galaxy: X-shooter spectroscopy and HST imaging of the afterglow and environment of the Swift GRB 210905A
|
Nov 30, 2022 |
|
MUSE-ALMA Haloes VII: Survey Science Goals & Design, Data Processing and Final Catalogues
|
Nov 30, 2022 |
|
Weak Lensing Tomographic Redshift Distribution Inference for the Hyper Suprime-Cam Subaru Strategic Program three-year shape catalogue
|
Nov 30, 2022 |
|
The Rapidly Spinning Intermediate-Mass Black Hole 3XMM J150052 0+015452
|
Nov 30, 2022 |
|
NICMOS Kernel-Phase Interferometry II: Demographics of Nearby Brown Dwarfs
|
Nov 30, 2022 |
|
Numerical Simulations of Two-Fluid Magnetoacoustic Waves in the Solar Atmosphere
|
Nov 30, 2022 |
|
Calibrating cosmological simulations with implicit likelihood inference using galaxy growth observables
|
Nov 30, 2022 |
|
Parametrized Asymmetric Neutral hydrogen Disk Integrated Spectrum Characterization PANDISC I: Introduction to A Physically Motivated H I Model
|
Nov 30, 2022 |
|
Identifying the physical origin of gamma-ray bursts with supervised machine learning
|
Nov 30, 2022 |
|
First release of PLATO consortium stellar limb-darkening coefficients
|
Nov 30, 2022 |
|
Estimating effective wind speed from Gemini Planet Imager's adaptive optics data using covariance maps
|
Nov 30, 2022 |
|
Determination of 1929 Asteroid Rotation Periods from WISE Data
|
Nov 30, 2022 |
|
Gravity in the Local Universe : density and velocity fields using CosmicFlows-4
|
Nov 30, 2022 |
|
Flares detected in ALMA single-dish images of the Sun
|
Nov 30, 2022 |
|
On the sociology and hierarchy of voids: a study of seven CAVITY nearby galaxy voids and their dynamical CosmicFlows-3 environment
|
Nov 30, 2022 |
|
Orientations of DM Halos in FIRE-2 Milky Way-mass Galaxies
|
Nov 30, 2022 |
|
Updating constraints on phantom crossing f T gravity
|
Nov 30, 2022 |
|
Direct Statistical Constraints on the Natal Kick velocity of a Black Hole in an X-ray Quiet Binary
|
Nov 30, 2022 |
|
The Complex Structure of the Bulge of M31
|
Nov 30, 2022 |
|
EIGER III JWST NIRCam observations of the ultra-luminous high-redshift quasar J0100+2802
|
Nov 30, 2022 |
|
Observations of planetary winds and outflows
|
Nov 30, 2022 |
|
Simultaneous gas accretion onto a pair of giant planets: Impact on their final mass and on the protoplanetary disk structure
|
Nov 30, 2022 |
|
Star & planet formation: Upcoming opportunities in the space-based infrared
|
Nov 30, 2022 |
|
The AstroSat UV Deep Field North: the far and near ultraviolet photometric catalog
|
Nov 30, 2022 |
|
Electromagnetic draping of merging neutron stars
|
Nov 30, 2022 |
|
The dynamical state of the globular clusters Rup 106 and IC 4499
|
Nov 30, 2022 |
|
The high-albedo, low polarization disk around HD 114082 harbouring a Jupiter-sized transiting planet
|
Nov 30, 2022 |
|
Peering into the Milky Way by FAST: IV Identification of two new Galactic supernova remnants G203 1+6 6 and G206 7+5 9
|
Nov 30, 2022 |
|
Peering into the Milky Way by FAST: III Magnetic fields in the Galactic halo and farther spiral arms revealed by the Faraday effect of faint pulsars
|
Nov 30, 2022 |
|
Peering into the Milky Way by FAST: II Ionized gas in the inner Galactic disk revealed by the piggyback line observations of the FAST GPPS survey
|
Nov 30, 2022 |
|
Peering into the Milky Way by FAST: I Exquisite HI structures in the inner Galactic disk from the piggyback line observations of the FAST GPPS survey
|
Nov 30, 2022 |
|
Shattering and growth of cold clouds in galaxy clusters: the role of radiative cooling, magnetic fields and thermal conduction
|
Nov 30, 2022 |
|
Visual Magnitude of the BlueWalker 3 Satellite
|
Nov 30, 2022 |
|
ASTENA: a mission concept for a deep study of the transient gamma-ray sky and for nuclear astrophysics
|
Nov 30, 2022 |
|
V838 Mon: A slow waking up of Sleeping Beauty?
|
Nov 30, 2022 |
|
BASS XXXIX: Swift-BAT AGN with changing-look optical spectra
|
Nov 30, 2022 |
|
Microlensing of gravitational waves by dark matter structures
|
Nov 30, 2022 |
|
Does the gamma-ray binary LS I +61°303 harbor a magnetar?
|
Nov 30, 2022 |
|
Real-world CMB lensing quadratic estimator power spectrum response
|
Nov 30, 2022 |
|
Machine learning classification of CHIME fast radio bursts -- I Supervised methods
|
Nov 30, 2022 |
|
Scattering variability detected from the circumsource medium of FRB 20190520B
|
Nov 30, 2022 |
|
Panchromatic HST WFC3 Imaging Studies of Young, Rapidly Evolving Planetary Nebulae II NGC 7027
|
Nov 30, 2022 |
|
Shock-induced stripping of satellite ISM CGM in IllustrisTNG clusters at z sim0
|
Nov 30, 2022 |
|
Energy transfer and restructuring in amorphous solid water upon consecutive irradiation
|
Nov 30, 2022 |
|
NICMOS Kernel-Phase Interferometry II: Demographics of Nearby Brown Dwarfs
|
Nov 30, 2022 |
|
On the sociology and hierarchy of voids: a study of seven CAVITY nearby galaxy voids and their dynamical CosmicFlows-3 environment
|
Nov 30, 2022 |
|
Period variation of the classical Cepheid SV Vulpeculae over a century 1913-2022
|
Nov 30, 2022 |
|
The Spectroscopic Classification of Astronomical Transients SCAT Survey: Overview, Pipeline Description, Initial Results, and Future Plans
|
Nov 30, 2022 |
|
A Catalog of the Highest-Energy Cosmic Rays Recorded During Phase I of Operation of the Pierre Auger Observatory
|
Nov 30, 2022 |
|
Orientations of DM Halos in FIRE-2 Milky Way-mass Galaxies
|
Nov 30, 2022 |
|
Making hot Jupiters in stellar clusters: the importance of binary exchange
|
Nov 30, 2022 |
|
Updating constraints on phantom crossing f T gravity
|
Nov 30, 2022 |
|
Direct Statistical Constraints on the Natal Kick velocity of a Black Hole in an X-ray Quiet Binary
|
Nov 30, 2022 |
|
The performance of the MAGIC telescopes using deep convolutional neural networks with CTLearn
|
Nov 30, 2022 |
|
Galaxy And Mass Assembly GAMA : The Dependence of Star Formation on Surface Brightness in Low Redshift Galaxies
|
Nov 30, 2022 |
|
The Complex Structure of the Bulge of M31
|
Nov 30, 2022 |
|
EIGER III JWST NIRCam observations of the ultra-luminous high-redshift quasar J0100+2802
|
Nov 30, 2022 |
|
Observations of planetary winds and outflows
|
Nov 30, 2022 |
|
SN 2018gk Revisited: the Photosphere, the Central Engine, And the Putative Dust
|
Nov 30, 2022 |
|
Evidence for a Massive Andromeda Galaxy Using Satellite Galaxy Proper Motions
|
Nov 30, 2022 |
|
Simultaneous gas accretion onto a pair of giant planets: Impact on their final mass and on the protoplanetary disk structure
|
Nov 30, 2022 |
|
Investigating pre-eruptive magnetic properties at the footprints of erupting magnetic flux ropes
|
Nov 30, 2022 |
|
Electromagnetic draping of merging neutron stars
|
Nov 30, 2022 |
|
Satellite Constellation Avoidance with the Rubin Observatory Legacy Survey of Space and Time
|
Nov 30, 2022 |
|
Numerical Simulations of Two-Fluid Magnetoacoustic Waves in the Solar Atmosphere
|
Nov 30, 2022 |
|
The CMB cold spot under the lens: ruling out a supervoid interpretation
|
Nov 30, 2022 |
|
Modeling Reconstructed Images of Jets Launched by SANE Super-Eddington Accretion Flows Around SMBHs with the ngEHT
|
Nov 30, 2022 |
|
The dynamical state of the globular clusters Rup 106 and IC 4499
|
Nov 30, 2022 |
|
Resonant Mode Coupling in δ Scuti Stars
|
Nov 30, 2022 |
|
BASS XXXIX: Swift-BAT AGN with changing-look optical spectra
|
Nov 30, 2022 |
|
Latest data constraint of some parameterized dark energy models
|
Nov 30, 2022 |
|
Real-world CMB lensing quadratic estimator power spectrum response
|
Nov 30, 2022 |
|
Bayesian modelling of scattered light in the LIGO interferometers
|
Nov 30, 2022 |
|
Machine learning classification of CHIME fast radio bursts -- I Supervised methods
|
Nov 30, 2022 |
|
Dust Motion and Possibility of Dust Growth in a Growing Circumstellar Disk
|
Nov 30, 2022 |
|
Scattering variability detected from the circumsource medium of FRB 20190520B
|
Nov 30, 2022 |
|
A Ghost in Boötes: The Least Luminous Disrupted Dwarf Galaxy
|
Nov 30, 2022 |
|
Potential contributions of Pop III and intermediate-mass Pop II stars to cosmic chemical enrichment
|
Nov 30, 2022 |
|
Explosion mechanism of core-collapse supernovae: role of the Si O interface
|
Nov 30, 2022 |
|
The XQR-30 Metal Absorber Catalog: 778 Absorption Systems Spanning 2 < z < 6 5
|
Nov 30, 2022 |
|
What can Gaussian Processes really tell us about supernova lightcurves? Consequences for Type II b morphologies and genealogies
|
Nov 30, 2022 |
|
Prospects for detecting and localizing short-duration transient gravitational waves from glitching neutron stars without electromagnetic counterparts
|
Nov 30, 2022 |
|
Using a Conditional Generative Adversarial Network to Control the Statistical Characteristics of Generated Images for IACT Data Analysis
|
Nov 30, 2022 |
|
Calibrating cosmological simulations with implicit likelihood inference using galaxy growth observables
|
Nov 30, 2022 |
|
Spectroscopic time series performance of the Mid-Infrared Instrument on the JWST
|
Nov 30, 2022 |
|
New constraints on the dark matter density profiles of dwarf galaxies from proper motions of globular cluster streams
|
Nov 30, 2022 |
|
Accelerating BAO Scale Fitting Using Taylor Series
|
Nov 30, 2022 |
|
The role of stellar expansion on the formation of gravitational wave sources
|
Nov 30, 2022 |
|
Adding Workflow Management Flexibility to LSST Pipelines Execution
|
Nov 30, 2022 |
|
The initial spin distribution of B-type stars revealed by the split main sequences of young star clusters
|
Nov 30, 2022 |
|
Oxygen line in fireball spectra and its application to satellite observations
|
Nov 30, 2022 |
|
3UCubed: The IMAP Student Collaboration CubeSat Project
|
Nov 30, 2022 |
|
Hard X-ray Observations of the Hydrogen-poor Superluminous Supernova SN 2018hti with NuSTAR
|
Nov 30, 2022 |
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The statistical properties of stars at redshift, z=5, compared with the present epoch
|
Nov 30, 2022 |
|
Fundamental physics with neutron stars
|
Nov 30, 2022 |
|
Parametrized Asymmetric Neutral hydrogen Disk Integrated Spectrum Characterization PANDISC I: Introduction to A Physically Motivated H I Model
|
Nov 30, 2022 |
|
The complex organic molecular content in the L1517B starless core
|
Nov 30, 2022 |
|
Chemical abundances in the dwarf galaxy NGC 4163 based on the nebular and auroral emission lines
|
Nov 30, 2022 |
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Observing Signals of Spectral Features in the Cosmic-Ray Positrons and Electrons from Milky Way Pulsars
|
Nov 30, 2022 |
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Multi-epoch variability of AT 2000ch SN 2000ch in NGC 3432 -- A radio continuum and optical study
|
Nov 30, 2022 |
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The mid-infrared molecular inventory towards Orion IRc2
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Nov 30, 2022 |
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Formation of star clusters and enrichment by massive stars in simulations of low-metallicity galaxies with a fully sampled initial stellar mass function
|
Nov 30, 2022 |
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Exciting the TTV Phases of Resonant Sub-Neptunes
|
Nov 30, 2022 |
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Inferencing Progenitor and Explosion Properties of Evolving Core-collapse Supernovae from Zwicky Transient Facility Light Curves
|
Nov 30, 2022 |
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Revisiting the space weather environment of Proxima Centauri b
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Nov 30, 2022 |
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Identifying the physical origin of gamma-ray bursts with supervised machine learning
|
Nov 30, 2022 |
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Toward Accurate Modeling of Galaxy Clustering on Small Scales: Halo Model Extensions & Lingering Tension
|
Nov 30, 2022 |
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PHANGS-JWST First Results: Duration of the early phase of massive star formation in NGC628
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Nov 30, 2022 |
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Anisotropic Photon and Electron Scattering without Ultrarelativistic Approximation
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Nov 30, 2022 |
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Evolutionary Origins of Binary Neutron Star Mergers: Effects of Common Envelope Efficiency and Metallicity
|
Nov 30, 2022 |
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Disturbed, diffuse, or just missing? A global study of the HI content of Hickson Compact Groups
|
Nov 30, 2022 |
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Neural networks: solving the chemistry of the interstellar medium
|
Nov 30, 2022 |
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VINTERGATAN-GM: The cosmological imprints of early mergers on Milky-Way-mass galaxies
|
Nov 30, 2022 |
|
Primordial Black Hole Formation during a Strongly Coupled Crossover
|
Nov 30, 2022 |
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X-ray Absorption Lines in the Warm-Hot Intergalactic Medium: Probing Chandra observations with the CAMEL simulations
|
Nov 30, 2022 |
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The Giant Accreting Protoplanet Survey GAPlanetS : Optimization Techniques for Robust Detections of Protoplanets
|
Nov 30, 2022 |
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Estimating effective wind speed from Gemini Planet Imager's adaptive optics data using covariance maps
|
Nov 30, 2022 |
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Forming equal mass planetary binaries by pebble accretion
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Nov 30, 2022 |
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Sensitivity of strong lensing observations to dark matter substructure: a case study with Euclid
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Nov 30, 2022 |
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Statistical Study of the Star Formation Efficiency in Bars: Is Star Formation Suppressed in Gas-Rich Bars?
|
Nov 30, 2022 |
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Separating the blue cloud and the red sequence using Otsu's method for image segmentation
|
Nov 30, 2022 |
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MOJAVE XX Decade-long linear polarization variability in AGN jets at parsec scales
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Nov 30, 2022 |
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Non-ideal magnetohydrodynamics of self-gravitating filaments
|
Nov 30, 2022 |
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Diffuse Emission of Galactic High-Energy Neutrinos from a Global Fit of Cosmic Rays
|
Nov 30, 2022 |
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Bar formation in submaximal disks: a challenge for Λ CDM
|
Nov 30, 2022 |
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Observational studies of high-mass star formation
|
Nov 30, 2022 |
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Palatini formulation for gauge theory: implications for slow-roll inflation
|
Nov 30, 2022 |
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Exoplanet Detection by Machine Learning with Data Augmentation
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Nov 30, 2022 |
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A Bayesian approach for torque modelling of BeXRB pulsars with application to super-Eddington accretors
|
Nov 30, 2022 |
|
Determination of 1929 Asteroid Rotation Periods from WISE Data
|
Nov 30, 2022 |
|
Hubble Space Telescope transmission spectroscopy for the temperate sub-Neptune TOI-270d: a possible hydrogen-rich atmosphere containing water vapour
|
Nov 30, 2022 |
|
GECAM Localization of High Energy Transients and the Systematic Error
|
Nov 30, 2022 |
|
Continuous gravitational wave emission from neutron stars with pinned superfluids in the core
|
Nov 30, 2022 |
|
FIREBall-2: flight preparation of a proven balloon payload to image the intermediate redshift circumgalactic medium
|
Nov 30, 2022 |
|
Assessing the physical reality of Milky Way open cluster candidates
|
Nov 30, 2022 |
|
A Bayesian approach to RFI mitigation
|
Nov 30, 2022 |
|
ISPY-NACO Imaging Survey for Planets around Young stars The demographics of forming planets embedded in protoplanetary disks
|
Nov 30, 2022 |
|
SILCC VII -- Gas kinematics and multiphase outflows of the simulated ISM at high gas surface densities
|
Nov 30, 2022 |
|
How has the solar wind evolved to become what it is today?
|
Nov 30, 2022 |
|
Status and prospects of the CORSIKA 8 air shower simulation framework
|
Nov 30, 2022 |
|
Stellar space weather effects on potentially habitable planets
|
Nov 30, 2022 |
|
Numerical Modeling of Energetic Electron Acceleration, Transport, and Emission in Solar Flares: Connecting Loop-top and Footpoint Hard X-Ray Sources
|
Nov 30, 2022 |
|
MAGIC observations provide compelling evidence of the hadronic multi-TeV emission from the putative PeVatron SNR G106 3+2 7
|
Nov 30, 2022 |
|
Free-form reconstruction of primordial power spectrum using Planck CMB temperature and polarization
|
Nov 30, 2022 |
|
Elements of effective machine learning datasets in astronomy
|
Nov 30, 2022 |
|
The Time-Averaged Mass-Loss Rates of Red Supergiants As Revealed by their Luminosity Functions in M31 and M33
|
Nov 30, 2022 |
|
PHANGS-JWST First Results: Dust embedded star clusters in NGC 7496 selected via 3 3 μ m PAH emission
|
Nov 30, 2022 |
|
Two lensed star candidates at z simeq4 8 behind the galaxy cluster MACS J0647 7+7015
|
Nov 30, 2022 |
|
iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs II the catalogue
|
Nov 30, 2022 |
|
Gravity in the Local Universe : density and velocity fields using CosmicFlows-4
|
Nov 30, 2022 |
|
PERISTOLE: PackagE that geneRates tIme delay plotS caused by graviTatiOnaL lEnsing
|
Nov 30, 2022 |
|
GD 99: Re-investigation of an old ZZ Ceti companion
|
Nov 30, 2022 |
|
A bias-free cosmological analysis with quasars alleviating H 0 tension
|
Nov 30, 2022 |
|
Ultra high energy cosmic rays from past activity of Andromeda galaxy
|
Nov 30, 2022 |
|
Posterior samples of source galaxies in strong gravitational lenses with score-based priors
|
Nov 30, 2022 |
|
Mirror Dark Sector Solution of the Hubble Tension with Time-varying Fine-structure Constant
|
Nov 30, 2022 |
|
Growth of A Massive Black Hole Via Tidal Disruption Accretion
|
Nov 30, 2022 |
|
The Circumgalactic Medium of Milky Way-like Galaxies in the TNG50 Simulation -- I: Halo Gas Properties and the Role of SMBH Feedback
|
Nov 30, 2022 |
|
ALMACAL IX: multi-band ALMA survey for dusty star-forming galaxies and the resolved fractions of the cosmic infrared background
|
Nov 30, 2022 |
|
Energy transfer and restructuring in amorphous solid water upon consecutive irradiation
|
Nov 29, 2022 |
|
Period variation of the classical Cepheid SV Vulpeculae over a century 1913-2022
|
Nov 29, 2022 |
|
The Spectroscopic Classification of Astronomical Transients SCAT Survey: Overview, Pipeline Description, Initial Results, and Future Plans
|
Nov 29, 2022 |
|
A Catalog of the Highest-Energy Cosmic Rays Recorded During Phase I of Operation of the Pierre Auger Observatory
|
Nov 29, 2022 |
|
Making hot Jupiters in stellar clusters: the importance of binary exchange
|
Nov 29, 2022 |
|
The performance of the MAGIC telescopes using deep convolutional neural networks with CTLearn
|
Nov 29, 2022 |
|
Galaxy And Mass Assembly GAMA : The Dependence of Star Formation on Surface Brightness in Low Redshift Galaxies
|
Nov 29, 2022 |
|
SN 2018gk Revisited: the Photosphere, the Central Engine, And the Putative Dust
|
Nov 29, 2022 |
|
Evidence for a Massive Andromeda Galaxy Using Satellite Galaxy Proper Motions
|
Nov 29, 2022 |
|
Investigating pre-eruptive magnetic properties at the footprints of erupting magnetic flux ropes
|
Nov 29, 2022 |
|
Satellite Constellation Avoidance with the Rubin Observatory Legacy Survey of Space and Time
|
Nov 29, 2022 |
|
The CMB cold spot under the lens: ruling out a supervoid interpretation
|
Nov 29, 2022 |
|
Modeling Reconstructed Images of Jets Launched by SANE Super-Eddington Accretion Flows Around SMBHs with the ngEHT
|
Nov 29, 2022 |
|
Resonant Mode Coupling in δ Scuti Stars
|
Nov 29, 2022 |
|
Latest data constraint of some parameterized dark energy models
|
Nov 29, 2022 |
|
Bayesian modelling of scattered light in the LIGO interferometers
|
Nov 29, 2022 |
|
Dust Motion and Possibility of Dust Growth in a Growing Circumstellar Disk
|
Nov 29, 2022 |
|
Potential contributions of Pop III and intermediate-mass Pop II stars to cosmic chemical enrichment
|
Nov 29, 2022 |
|
The XQR-30 Metal Absorber Catalog: 778 Absorption Systems Spanning 2 < z < 6 5
|
Nov 29, 2022 |
|
Using a Conditional Generative Adversarial Network to Control the Statistical Characteristics of Generated Images for IACT Data Analysis
|
Nov 29, 2022 |
|
Spectroscopic time series performance of the Mid-Infrared Instrument on the JWST
|
Nov 29, 2022 |
|
The role of stellar expansion on the formation of gravitational wave sources
|
Nov 29, 2022 |
|
Adding Workflow Management Flexibility to LSST Pipelines Execution
|
Nov 29, 2022 |
|
The initial spin distribution of B-type stars revealed by the split main sequences of young star clusters
|
Nov 29, 2022 |
|
Oxygen line in fireball spectra and its application to satellite observations
|
Nov 29, 2022 |
|
3UCubed: The IMAP Student Collaboration CubeSat Project
|
Nov 29, 2022 |
|
Hard X-ray Observations of the Hydrogen-poor Superluminous Supernova SN 2018hti with NuSTAR
|
Nov 29, 2022 |
|
The statistical properties of stars at redshift, z=5, compared with the present epoch
|
Nov 29, 2022 |
|
Fundamental physics with neutron stars
|
Nov 29, 2022 |
|
The complex organic molecular content in the L1517B starless core
|
Nov 29, 2022 |
|
Chemical abundances in the dwarf galaxy NGC 4163 based on the nebular and auroral emission lines
|
Nov 29, 2022 |
|
Observing Signals of Spectral Features in the Cosmic-Ray Positrons and Electrons from Milky Way Pulsars
|
Nov 29, 2022 |
|
Multi-epoch variability of AT 2000ch SN 2000ch in NGC 3432 -- A radio continuum and optical study
|
Nov 29, 2022 |
|
The mid-infrared molecular inventory towards Orion IRc2
|
Nov 29, 2022 |
|
Formation of star clusters and enrichment by massive stars in simulations of low-metallicity galaxies with a fully sampled initial stellar mass function
|
Nov 29, 2022 |
|
Exciting the TTV Phases of Resonant Sub-Neptunes
|
Nov 29, 2022 |
|
Inferencing Progenitor and Explosion Properties of Evolving Core-collapse Supernovae from Zwicky Transient Facility Light Curves
|
Nov 29, 2022 |
|
Revisiting the space weather environment of Proxima Centauri b
|
Nov 29, 2022 |
|
Toward Accurate Modeling of Galaxy Clustering on Small Scales: Halo Model Extensions & Lingering Tension
|
Nov 29, 2022 |
|
PHANGS-JWST First Results: Duration of the early phase of massive star formation in NGC628
|
Nov 29, 2022 |
|
Anisotropic Photon and Electron Scattering without Ultrarelativistic Approximation
|
Nov 29, 2022 |
|
Evolutionary Origins of Binary Neutron Star Mergers: Effects of Common Envelope Efficiency and Metallicity
|
Nov 29, 2022 |
|
Disturbed, diffuse, or just missing? A global study of the HI content of Hickson Compact Groups
|
Nov 29, 2022 |
|
Neural networks: solving the chemistry of the interstellar medium
|
Nov 29, 2022 |
|
VINTERGATAN-GM: The cosmological imprints of early mergers on Milky-Way-mass galaxies
|
Nov 29, 2022 |
|
Primordial Black Hole Formation during a Strongly Coupled Crossover
|
Nov 29, 2022 |
|
X-ray Absorption Lines in the Warm-Hot Intergalactic Medium: Probing Chandra observations with the CAMEL simulations
|
Nov 29, 2022 |
|
The Giant Accreting Protoplanet Survey GAPlanetS : Optimization Techniques for Robust Detections of Protoplanets
|
Nov 29, 2022 |
|
Forming equal mass planetary binaries by pebble accretion
|
Nov 29, 2022 |
|
Sensitivity of strong lensing observations to dark matter substructure: a case study with Euclid
|
Nov 29, 2022 |
|
Statistical Study of the Star Formation Efficiency in Bars: Is Star Formation Suppressed in Gas-Rich Bars?
|
Nov 29, 2022 |
|
Separating the blue cloud and the red sequence using Otsu's method for image segmentation
|
Nov 29, 2022 |
|
MOJAVE XX Decade-long linear polarization variability in AGN jets at parsec scales
|
Nov 29, 2022 |
|
Non-ideal magnetohydrodynamics of self-gravitating filaments
|
Nov 29, 2022 |
|
Diffuse Emission of Galactic High-Energy Neutrinos from a Global Fit of Cosmic Rays
|
Nov 29, 2022 |
|
Bar formation in submaximal disks: a challenge for Λ CDM
|
Nov 29, 2022 |
|
Observational studies of high-mass star formation
|
Nov 29, 2022 |
|
Palatini formulation for gauge theory: implications for slow-roll inflation
|
Nov 29, 2022 |
|
Exoplanet Detection by Machine Learning with Data Augmentation
|
Nov 29, 2022 |
|
A Bayesian approach for torque modelling of BeXRB pulsars with application to super-Eddington accretors
|
Nov 29, 2022 |
|
Hubble Space Telescope transmission spectroscopy for the temperate sub-Neptune TOI-270d: a possible hydrogen-rich atmosphere containing water vapour
|
Nov 29, 2022 |
|
GECAM Localization of High Energy Transients and the Systematic Error
|
Nov 29, 2022 |
|
Continuous gravitational wave emission from neutron stars with pinned superfluids in the core
|
Nov 29, 2022 |
|
FIREBall-2: flight preparation of a proven balloon payload to image the intermediate redshift circumgalactic medium
|
Nov 29, 2022 |
|
Assessing the physical reality of Milky Way open cluster candidates
|
Nov 29, 2022 |
|
A Bayesian approach to RFI mitigation
|
Nov 29, 2022 |
|
ISPY-NACO Imaging Survey for Planets around Young stars The demographics of forming planets embedded in protoplanetary disks
|
Nov 29, 2022 |
|
SILCC VII -- Gas kinematics and multiphase outflows of the simulated ISM at high gas surface densities
|
Nov 29, 2022 |
|
How has the solar wind evolved to become what it is today?
|
Nov 29, 2022 |
|
Status and prospects of the CORSIKA 8 air shower simulation framework
|
Nov 29, 2022 |
|
Stellar space weather effects on potentially habitable planets
|
Nov 29, 2022 |
|
Numerical Modeling of Energetic Electron Acceleration, Transport, and Emission in Solar Flares: Connecting Loop-top and Footpoint Hard X-Ray Sources
|
Nov 29, 2022 |
|
MAGIC observations provide compelling evidence of the hadronic multi-TeV emission from the putative PeVatron SNR G106 3+2 7
|
Nov 29, 2022 |
|
Free-form reconstruction of primordial power spectrum using Planck CMB temperature and polarization
|
Nov 29, 2022 |
|
Elements of effective machine learning datasets in astronomy
|
Nov 29, 2022 |
|
The Time-Averaged Mass-Loss Rates of Red Supergiants As Revealed by their Luminosity Functions in M31 and M33
|
Nov 29, 2022 |
|
PHANGS-JWST First Results: Dust embedded star clusters in NGC 7496 selected via 3 3 μ m PAH emission
|
Nov 29, 2022 |
|
Two lensed star candidates at z simeq4 8 behind the galaxy cluster MACS J0647 7+7015
|
Nov 29, 2022 |
|
iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs II the catalogue
|
Nov 29, 2022 |
|
PERISTOLE: PackagE that geneRates tIme delay plotS caused by graviTatiOnaL lEnsing
|
Nov 29, 2022 |
|
GD 99: Re-investigation of an old ZZ Ceti companion
|
Nov 29, 2022 |
|
A bias-free cosmological analysis with quasars alleviating H 0 tension
|
Nov 29, 2022 |
|
Ultra high energy cosmic rays from past activity of Andromeda galaxy
|
Nov 29, 2022 |
|
Posterior samples of source galaxies in strong gravitational lenses with score-based priors
|
Nov 29, 2022 |
|
Mirror Dark Sector Solution of the Hubble Tension with Time-varying Fine-structure Constant
|
Nov 29, 2022 |
|
Growth of A Massive Black Hole Via Tidal Disruption Accretion
|
Nov 29, 2022 |
|
The Circumgalactic Medium of Milky Way-like Galaxies in the TNG50 Simulation -- I: Halo Gas Properties and the Role of SMBH Feedback
|
Nov 29, 2022 |
|
ALMACAL IX: multi-band ALMA survey for dusty star-forming galaxies and the resolved fractions of the cosmic infrared background
|
Nov 29, 2022 |
|
Separating the blue cloud and the red sequence using Otsu's method for image segmentation
|
Nov 29, 2022 |
|
GECAM Localization of High Energy Transients and the Systematic Error
|
Nov 29, 2022 |
|
Continuous gravitational wave emission from neutron stars with pinned superfluids in the core
|
Nov 29, 2022 |
|
FIREBall-2: flight preparation of a proven balloon payload to image the intermediate redshift circumgalactic medium
|
Nov 29, 2022 |
|
Assessing the physical reality of Milky Way open cluster candidates
|
Nov 29, 2022 |
|
A Bayesian approach to RFI mitigation
|
Nov 29, 2022 |
|
ISPY-NACO Imaging Survey for Planets around Young stars The demographics of forming planets embedded in protoplanetary disks
|
Nov 29, 2022 |
|
SILCC VII -- Gas kinematics and multiphase outflows of the simulated ISM at high gas surface densities
|
Nov 29, 2022 |
|
How has the solar wind evolved to become what it is today?
|
Nov 29, 2022 |
|
Stellar space weather effects on potentially habitable planets
|
Nov 29, 2022 |
|
MOJAVE XX Decade-long linear polarization variability in AGN jets at parsec scales
|
Nov 29, 2022 |
|
Numerical Modeling of Energetic Electron Acceleration, Transport, and Emission in Solar Flares: Connecting Loop-top and Footpoint Hard X-Ray Sources
|
Nov 29, 2022 |
|
MAGIC observations provide compelling evidence of the hadronic multi-TeV emission from the putative PeVatron SNR G106 3+2 7
|
Nov 29, 2022 |
|
PHANGS-JWST First Results: Dust embedded star clusters in NGC 7496 selected via 3 3 μ m PAH emission
|
Nov 29, 2022 |
|
GD 99: Re-investigation of an old ZZ Ceti companion
|
Nov 29, 2022 |
|
A bias-free cosmological analysis with quasars alleviating H 0 tension
|
Nov 29, 2022 |
|
Ultra high energy cosmic rays from past activity of Andromeda galaxy
|
Nov 29, 2022 |
|
Non-ideal magnetohydrodynamics of self-gravitating filaments
|
Nov 29, 2022 |
|
Formation History of HD106906 and the Vertical Warping of Debris Disks by an External Inclined Companion
|
Nov 29, 2022 |
|
Near-infrared Extragalactic Background Light Fluctuations on Nonlinear Scales
|
Nov 29, 2022 |
|
An Effective Bias Expansion for 21 cm Cosmology in Redshift Space
|
Nov 29, 2022 |
|
Layer formation in a stably-stratified fluid cooled from above Towards an analog for Jupiter and other gas giants
|
Nov 29, 2022 |
|
The Final Season Reimagined: 30 Tidal Disruption Events from the ZTF-I Survey
|
Nov 29, 2022 |
|
Diffuse Emission of Galactic High-Energy Neutrinos from a Global Fit of Cosmic Rays
|
Nov 29, 2022 |
|
Bar formation in submaximal disks: a challenge for Λ CDM
|
Nov 29, 2022 |
|
Observational studies of high-mass star formation
|
Nov 29, 2022 |
|
Palatini formulation for gauge theory: implications for slow-roll inflation
|
Nov 29, 2022 |
|
Exoplanet Detection by Machine Learning with Data Augmentation
|
Nov 29, 2022 |
|
Hubble Space Telescope transmission spectroscopy for the temperate sub-Neptune TOI-270d: a possible hydrogen-rich atmosphere containing water vapour
|
Nov 29, 2022 |
|
Revisiting Empirical Solar Energetic Particle Scaling Relations I Solar flares
|
Nov 29, 2022 |
|
Non-thermal emission from mildly relativistic dynamical ejecta of neutron star mergers
|
Nov 29, 2022 |
|
WALLABY Pilot Survey: HI gas kinematics of galaxy pairs in cluster environment
|
Nov 29, 2022 |
|
Association of Optical, Ultraviolet and Soft X-ray excess Emissions in AGNs
|
Nov 29, 2022 |
|
Near-inflection point inflation and production of dark matter during reheating
|
Nov 29, 2022 |
|
CSS1603+19: a low-mass polar near the cataclysmic variable period minimum
|
Nov 29, 2022 |
|
Cosmic ray electron and positron spectra at TeV energies
|
Nov 29, 2022 |
|
Congruity of Crab pulsar's gamma-ray spectrum with the spectral distribution of the radiation by the current sheet in its magnetosphere
|
Nov 29, 2022 |
|
Primordial black holes and gravitational waves from non-canonical inflation
|
Nov 29, 2022 |
|
Elemental abundances in M31: Individual and Coadded Spectroscopic Fe H and α Fe throughout the M31 Halo with SPLASH
|
Nov 29, 2022 |
|
Constraining Single-Field Inflation with MegaMapper
|
Nov 29, 2022 |
|
SuNeRF: Validation of a 3D Global Reconstruction of the Solar Corona Using Simulated EUV Images
|
Nov 29, 2022 |
|
1 5D NLTE spectral synthesis of a 3D filament prominence simulation
|
Nov 29, 2022 |
|
Infrared Properties of OGLE4 Mira variables in our Galaxy
|
Nov 29, 2022 |
|
Plausible Adversarial Attacks on Direct Parameter Inference Models in Astrophysics
|
Nov 29, 2022 |
|
Resonant Dynamical Friction: Analytical Description
|
Nov 29, 2022 |
|
Spectroastrometric Reverberation Mapping of Broad-line Regions
|
Nov 29, 2022 |
|
Dark Matter Accounts for Perturbation in the GD-1 Stellar Stream
|
Nov 29, 2022 |
|
Utility of PCA and Other Data Transformation Techniques in Exoplanet Research
|
Nov 29, 2022 |
|
Disk dissipation, giant planet formation and star-formation-rate fluctuations in the past three-million-year history of Gould's Belt
|
Nov 29, 2022 |
|
The effect of saturated thermal conduction on clouds in a hot plasma
|
Nov 29, 2022 |
|
Concept of an achromatic stellar coronagraph and its application for detecting extrasolar planets
|
Nov 29, 2022 |
|
An Analytical Fourier-Transformation Model for the Production of Hard and Soft X-Ray Time Lags in AGNs: Application to 1H 0707-495
|
Nov 29, 2022 |
|
When Spectral Modeling Meets Convolutional Networks: A Method for Discovering Reionization-era Lensed Quasars in Multi-band Imaging Data
|
Nov 29, 2022 |
|
Recurrent narrow quasi-periodic fast-propagating wave trains excited by the intermittent energy release in the accompanying solar flare
|
Nov 29, 2022 |
|
Probing the tidal disruption event iPTF16axa with CLOUDY and disc-wind models
|
Nov 29, 2022 |
|
Electromagnetic draping of merging neutron stars
|
Nov 29, 2022 |
|
Elements of effective machine learning datasets in astronomy
|
Nov 29, 2022 |
|
A blazar candidate for the Fermi source 4FGL J1848 7-0129
|
Nov 29, 2022 |
|
Connecting photometric and spectroscopic granulation signals with CHEOPS and ESPRESSO
|
Nov 29, 2022 |
|
Flares in the changing look AGN Mrk 590 I: The UV response to X-ray outbursts suggests a more complex reprocessing geometry than a standard disk
|
Nov 29, 2022 |
|
Evidence for large-scale excesses associated with low HI column densities in the sky I Dust excess
|
Nov 29, 2022 |
|
Gas kinematics around filamentary structures in the Orion B cloud
|
Nov 29, 2022 |
|
A Panchromatic Study of Massive Stars in the Extremely Metal-Poor Local Group Dwarf Galaxy Leo A
|
Nov 29, 2022 |
|
The critical role of nuclear heating rates, thermalization efficiencies and opacities for kilonova modelling and parameter inference
|
Nov 29, 2022 |
|
The Hubble Constant Troubled by Dark Matter in Non-Standard Cosmologies
|
Nov 29, 2022 |
|
Foreground Separation and Constraints on Primordial Gravitational Waves with the PICO Space Mission
|
Nov 29, 2022 |
|
Outer disc edge: properties of low frequency aperiodic variability in ultracompact interacting binaries
|
Nov 29, 2022 |
|
The Pristine Inner Galaxy Survey PIGS VI: Different vertical distributions between two DIBs at 442 8 nm and 862 1 nm
|
Nov 29, 2022 |
|
Constraining dark matter decays with cosmic microwave background and weak lensing shear observations
|
Nov 29, 2022 |
|
Revisiting the atmosphere of the exoplanet 51 Eridani b with VLT SPHERE
|
Nov 29, 2022 |
|
First detections of stellar light from quasar host galaxies at z > 6
|
Nov 29, 2022 |
|
A Sample of Dust Attenuation Laws for DES Supernova Host Galaxies
|
Nov 29, 2022 |
|
The SPHERE view of three interacting twin disc systems in polarised light
|
Nov 29, 2022 |
|
De-noising non-Gaussian fields in cosmology with normalizing flows
|
Nov 29, 2022 |
|
Application of Convolutional Neural Networks to Predict Magnetic Fields Directions in Turbulent Clouds
|
Nov 29, 2022 |
|
Hybrid α -attractors, primordial black holes and gravitational wave backgrounds
|
Nov 29, 2022 |
|
Significance Mode Analysis SigMA for hierarchical structures An application to the Sco-Cen OB association
|
Nov 29, 2022 |
|
Constraints on the Model of Gamma-ray Bursts and Implications from GRB 221009A: GeV gamma rays v s High-energy Neutrinos
|
Nov 29, 2022 |
|
Searches for Neutrinos from LHAASO ultra-high-energy γ-ray sources using the IceCube Neutrino Observatory
|
Nov 29, 2022 |
|
The Time-Averaged Mass-Loss Rates of Red Supergiants As Revealed by their Luminosity Functions in M31 and M33
|
Nov 29, 2022 |
|
Reducing the Impact of Weak-lensing Errors on Gravitational-wave Standard Sirens
|
Nov 29, 2022 |
|
Machine learning cosmic inflation
|
Nov 29, 2022 |
|
The Gaia-ESO Survey: probing the lithium abundances in old metal-rich dwarf stars in the Solar vicinity
|
Nov 29, 2022 |
|
The uncertain interstellar medium of high-redshift quiescent galaxies: Impact of methodology
|
Nov 29, 2022 |
|
An efficient Monte Carlo model for the slowing down of photoelectrons Application to H- α in exoplanet atmospheres
|
Nov 29, 2022 |
|
Characterisation of the MUSIC ASIC for large-area silicon photomultipliers for gamma-ray astronomy
|
Nov 29, 2022 |
|
A Chemical Study of Nine Star-forming Regions with Evidence of Infall Motion
|
Nov 29, 2022 |
|
The giant low surface brightness galaxy Malin 1: new constraints for its molecular gas mass from GBT ARGUS observations
|
Nov 29, 2022 |
|
Multiple gas phases in supernova remnant IC 443: mapping shocked H 2 with VLT KMOS
|
Nov 29, 2022 |
|
Star & planet formation: Upcoming opportunities in the space-based infrared
|
Nov 29, 2022 |
|
A search for thermal gyro-synchrotron emission from hot stellar coronae
|
Nov 29, 2022 |
|
Solar coronal heating from small-scale magnetic braids
|
Nov 29, 2022 |
|
On the Kinematic Morphology around Halos
|
Nov 29, 2022 |
|
Rotation Measure Variations and Reversals of Repeating Fast Radio Bursts in Massive Binary Systems
|
Nov 29, 2022 |
|
Using Anisotropies as a Forensic Tool for Decoding Supernova Remnants
|
Nov 29, 2022 |
|
Constraining primordial tensor features with the anisotropies of the Cosmic Microwave Background
|
Nov 29, 2022 |
|
Free-form reconstruction of primordial power spectrum using Planck CMB temperature and polarization
|
Nov 29, 2022 |
|
The Athena X-ray Integral Field Unit: a consolidated design for the system requirement review of the preliminary definition phase
|
Nov 29, 2022 |
|
Scalar Weak Gravity Conjecture in Super Yang-Mills Inflationary Model
|
Nov 29, 2022 |
|
The Extreme Super-Eddington NLS1 RX J0134 2-4258 -- II A Weak-Line Seyfert Linking to the Weak-Line Quasar
|
Nov 29, 2022 |
|
The spins of stripped B stars support magnetic internal angular momentum transport
|
Nov 29, 2022 |
|
A Comprehensive Study on Galaxies at z~9-16 Found in the Early JWST Data: UV Luminosity Functions and Cosmic Star-Formation History at the Pre-Reionization Epoch
|
Nov 29, 2022 |
|
Muons in showers with energy E 0 geq 5 EeV and QGSjetII-04 and EPOS LHC models of hadronic interactions Is there a muon deficit in the models?
|
Nov 29, 2022 |
|
JWST NIRCam Observations of Stars and HII Regions in z simeq 6-8 Galaxies: Properties of Star Forming Complexes on 150 pc Scales
|
Nov 29, 2022 |
|
Two substellar survivor candidates; one found and one missing
|
Nov 29, 2022 |
|
Revisiting Empirical Solar Energetic Particle Scaling Relations I Solar flares
|
Nov 28, 2022 |
|
Non-thermal emission from mildly relativistic dynamical ejecta of neutron star mergers
|
Nov 28, 2022 |
|
WALLABY Pilot Survey: HI gas kinematics of galaxy pairs in cluster environment
|
Nov 28, 2022 |
|
Association of Optical, Ultraviolet and Soft X-ray excess Emissions in AGNs
|
Nov 28, 2022 |
|
Near-inflection point inflation and production of dark matter during reheating
|
Nov 28, 2022 |
|
CSS1603+19: a low-mass polar near the cataclysmic variable period minimum
|
Nov 28, 2022 |
|
Cosmic ray electron and positron spectra at TeV energies
|
Nov 28, 2022 |
|
Congruity of Crab pulsar's gamma-ray spectrum with the spectral distribution of the radiation by the current sheet in its magnetosphere
|
Nov 28, 2022 |
|
Primordial black holes and gravitational waves from non-canonical inflation
|
Nov 28, 2022 |
|
Elemental abundances in M31: Individual and Coadded Spectroscopic Fe H and α Fe throughout the M31 Halo with SPLASH
|
Nov 28, 2022 |
|
Constraining Single-Field Inflation with MegaMapper
|
Nov 28, 2022 |
|
SuNeRF: Validation of a 3D Global Reconstruction of the Solar Corona Using Simulated EUV Images
|
Nov 28, 2022 |
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1 5D NLTE spectral synthesis of a 3D filament prominence simulation
|
Nov 28, 2022 |
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Infrared Properties of OGLE4 Mira variables in our Galaxy
|
Nov 28, 2022 |
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Plausible Adversarial Attacks on Direct Parameter Inference Models in Astrophysics
|
Nov 28, 2022 |
|
Resonant Dynamical Friction: Analytical Description
|
Nov 28, 2022 |
|
Spectroastrometric Reverberation Mapping of Broad-line Regions
|
Nov 28, 2022 |
|
Dark Matter Accounts for Perturbation in the GD-1 Stellar Stream
|
Nov 28, 2022 |
|
Utility of PCA and Other Data Transformation Techniques in Exoplanet Research
|
Nov 28, 2022 |
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Disk dissipation, giant planet formation and star-formation-rate fluctuations in the past three-million-year history of Gould's Belt
|
Nov 28, 2022 |
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The effect of saturated thermal conduction on clouds in a hot plasma
|
Nov 28, 2022 |
|
Concept of an achromatic stellar coronagraph and its application for detecting extrasolar planets
|
Nov 28, 2022 |
|
An Analytical Fourier-Transformation Model for the Production of Hard and Soft X-Ray Time Lags in AGNs: Application to 1H 0707-495
|
Nov 28, 2022 |
|
When Spectral Modeling Meets Convolutional Networks: A Method for Discovering Reionization-era Lensed Quasars in Multi-band Imaging Data
|
Nov 28, 2022 |
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Recurrent narrow quasi-periodic fast-propagating wave trains excited by the intermittent energy release in the accompanying solar flare
|
Nov 28, 2022 |
|
Probing the tidal disruption event iPTF16axa with CLOUDY and disc-wind models
|
Nov 28, 2022 |
|
Electromagnetic draping of merging neutron stars
|
Nov 28, 2022 |
|
Elements of effective machine learning datasets in astronomy
|
Nov 28, 2022 |
|
A blazar candidate for the Fermi source 4FGL J1848 7-0129
|
Nov 28, 2022 |
|
Connecting photometric and spectroscopic granulation signals with CHEOPS and ESPRESSO
|
Nov 28, 2022 |
|
Flares in the changing look AGN Mrk 590 I: The UV response to X-ray outbursts suggests a more complex reprocessing geometry than a standard disk
|
Nov 28, 2022 |
|
Evidence for large-scale excesses associated with low HI column densities in the sky I Dust excess
|
Nov 28, 2022 |
|
Gas kinematics around filamentary structures in the Orion B cloud
|
Nov 28, 2022 |
|
A Panchromatic Study of Massive Stars in the Extremely Metal-Poor Local Group Dwarf Galaxy Leo A
|
Nov 28, 2022 |
|
The critical role of nuclear heating rates, thermalization efficiencies and opacities for kilonova modelling and parameter inference
|
Nov 28, 2022 |
|
The Hubble Constant Troubled by Dark Matter in Non-Standard Cosmologies
|
Nov 28, 2022 |
|
Foreground Separation and Constraints on Primordial Gravitational Waves with the PICO Space Mission
|
Nov 28, 2022 |
|
Outer disc edge: properties of low frequency aperiodic variability in ultracompact interacting binaries
|
Nov 28, 2022 |
|
The Pristine Inner Galaxy Survey PIGS VI: Different vertical distributions between two DIBs at 442 8 nm and 862 1 nm
|
Nov 28, 2022 |
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Constraining dark matter decays with cosmic microwave background and weak lensing shear observations
|
Nov 28, 2022 |
|
Revisiting the atmosphere of the exoplanet 51 Eridani b with VLT SPHERE
|
Nov 28, 2022 |
|
First detections of stellar light from quasar host galaxies at z > 6
|
Nov 28, 2022 |
|
A Sample of Dust Attenuation Laws for DES Supernova Host Galaxies
|
Nov 28, 2022 |
|
The SPHERE view of three interacting twin disc systems in polarised light
|
Nov 28, 2022 |
|
De-noising non-Gaussian fields in cosmology with normalizing flows
|
Nov 28, 2022 |
|
Application of Convolutional Neural Networks to Predict Magnetic Fields Directions in Turbulent Clouds
|
Nov 28, 2022 |
|
Hybrid α -attractors, primordial black holes and gravitational wave backgrounds
|
Nov 28, 2022 |
|
Significance Mode Analysis SigMA for hierarchical structures An application to the Sco-Cen OB association
|
Nov 28, 2022 |
|
Constraints on the Model of Gamma-ray Bursts and Implications from GRB 221009A: GeV gamma rays v s High-energy Neutrinos
|
Nov 28, 2022 |
|
Searches for Neutrinos from LHAASO ultra-high-energy γ-ray sources using the IceCube Neutrino Observatory
|
Nov 28, 2022 |
|
The Time-Averaged Mass-Loss Rates of Red Supergiants As Revealed by their Luminosity Functions in M31 and M33
|
Nov 28, 2022 |
|
Reducing the Impact of Weak-lensing Errors on Gravitational-wave Standard Sirens
|
Nov 28, 2022 |
|
Machine learning cosmic inflation
|
Nov 28, 2022 |
|
The Gaia-ESO Survey: probing the lithium abundances in old metal-rich dwarf stars in the Solar vicinity
|
Nov 28, 2022 |
|
The uncertain interstellar medium of high-redshift quiescent galaxies: Impact of methodology
|
Nov 28, 2022 |
|
An efficient Monte Carlo model for the slowing down of photoelectrons Application to H- α in exoplanet atmospheres
|
Nov 28, 2022 |
|
Characterisation of the MUSIC ASIC for large-area silicon photomultipliers for gamma-ray astronomy
|
Nov 28, 2022 |
|
A Chemical Study of Nine Star-forming Regions with Evidence of Infall Motion
|
Nov 28, 2022 |
|
The giant low surface brightness galaxy Malin 1: new constraints for its molecular gas mass from GBT ARGUS observations
|
Nov 28, 2022 |
|
Multiple gas phases in supernova remnant IC 443: mapping shocked H 2 with VLT KMOS
|
Nov 28, 2022 |
|
Star & planet formation: Upcoming opportunities in the space-based infrared
|
Nov 28, 2022 |
|
A search for thermal gyro-synchrotron emission from hot stellar coronae
|
Nov 28, 2022 |
|
Solar coronal heating from small-scale magnetic braids
|
Nov 28, 2022 |
|
On the Kinematic Morphology around Halos
|
Nov 28, 2022 |
|
Rotation Measure Variations and Reversals of Repeating Fast Radio Bursts in Massive Binary Systems
|
Nov 28, 2022 |
|
Using Anisotropies as a Forensic Tool for Decoding Supernova Remnants
|
Nov 28, 2022 |
|
Constraining primordial tensor features with the anisotropies of the Cosmic Microwave Background
|
Nov 28, 2022 |
|
Free-form reconstruction of primordial power spectrum using Planck CMB temperature and polarization
|
Nov 28, 2022 |
|
The Athena X-ray Integral Field Unit: a consolidated design for the system requirement review of the preliminary definition phase
|
Nov 28, 2022 |
|
Scalar Weak Gravity Conjecture in Super Yang-Mills Inflationary Model
|
Nov 28, 2022 |
|
The Extreme Super-Eddington NLS1 RX J0134 2-4258 -- II A Weak-Line Seyfert Linking to the Weak-Line Quasar
|
Nov 28, 2022 |
|
The spins of stripped B stars support magnetic internal angular momentum transport
|
Nov 28, 2022 |
|
A Comprehensive Study on Galaxies at z~9-16 Found in the Early JWST Data: UV Luminosity Functions and Cosmic Star-Formation History at the Pre-Reionization Epoch
|
Nov 28, 2022 |
|
Muons in showers with energy E 0 geq 5 EeV and QGSjetII-04 and EPOS LHC models of hadronic interactions Is there a muon deficit in the models?
|
Nov 28, 2022 |
|
JWST NIRCam Observations of Stars and HII Regions in z simeq 6-8 Galaxies: Properties of Star Forming Complexes on 150 pc Scales
|
Nov 28, 2022 |
|
Two substellar survivor candidates; one found and one missing
|
Nov 28, 2022 |
|
A Sample of Dust Attenuation Laws for DES Supernova Host Galaxies
|
Nov 28, 2022 |
|
Decade Long Timing Study of the Black Widow Millisecond Pulsar J1544+4937
|
Nov 28, 2022 |
|
Electron acceleration at supernova remnants
|
Nov 28, 2022 |
|
The Time-Averaged Mass-Loss Rates of Red Supergiants As Revealed by their Luminosity Functions in M31 and M33
|
Nov 28, 2022 |
|
Hidden Cooling Flows in Clusters of Galaxies II: A Wider Sample
|
Nov 28, 2022 |
|
Machine learning cosmic inflation
|
Nov 28, 2022 |
|
Sparse Bayesian mass-mapping using trans-dimensional MCMC
|
Nov 28, 2022 |
|
The Gaia-ESO Survey: probing the lithium abundances in old metal-rich dwarf stars in the Solar vicinity
|
Nov 28, 2022 |
|
Probability Distribution Functions of Sunspot Magnetic Flux
|
Nov 28, 2022 |
|
The uncertain interstellar medium of high-redshift quiescent galaxies: Impact of methodology
|
Nov 28, 2022 |
|
An efficient Monte Carlo model for the slowing down of photoelectrons Application to H- α in exoplanet atmospheres
|
Nov 28, 2022 |
|
High-energy Neutrino Productions from AGN Disk Transients Impacted by Circum-disk Medium
|
Nov 28, 2022 |
|
A search for thermal gyro-synchrotron emission from hot stellar coronae
|
Nov 28, 2022 |
|
Threshold of Primordial Black Hole Formation against Velocity Dispersion in Matter-Dominated Era
|
Nov 28, 2022 |
|
Logarithmic Duality of the Curvature Perturbation
|
Nov 28, 2022 |
|
A Generalized Analytical Model For Thermal And Bulk Comptonization In Accretion-Powered X-Ray Pulsars
|
Nov 28, 2022 |
|
Using Anisotropies as a Forensic Tool for Decoding Supernova Remnants
|
Nov 28, 2022 |
|
Modeling Hadronic Gamma-ray Emissions from Solar Flares and Prospects for Detecting Non-thermal Signatures from Protostars
|
Nov 28, 2022 |
|
The spins of stripped B stars support magnetic internal angular momentum transport
|
Nov 28, 2022 |
|
Ganymede MHD Model: Magnetospheric Context for Juno's PJ34 Flyby
|
Nov 28, 2022 |
|
Pulsar Glitches: A Review
|
Nov 28, 2022 |
|
The eROSITA Final Equatorial-Depth Survey eFEDS : X-ray properties of Subaru optically-selected clusters
|
Nov 28, 2022 |
|
Asymmetry in the number of L4 and L5 Jupiter Trojans driven by jumping Jupiter
|
Nov 28, 2022 |
|
Euclid: Cosmological forecasts from the void size function
|
Nov 28, 2022 |
|
Removal of point source leakage from time-order data filtering
|
Nov 28, 2022 |
|
Tempestuous life beyond R500: X-ray view on the Coma cluster with SRG eROSITA II Shock & Relic
|
Nov 28, 2022 |
|
A Chemical Study of Nine Star-forming Regions with Evidence of Infall Motion
|
Nov 28, 2022 |
|
Constraining cosmological phase transitions with the Parkes Pulsar Timing Array
|
Nov 28, 2022 |
|
Near-Infrared Spectroscopy of Ultracompact ion H 2 regions in W51A with NIFS ALTAIR
|
Nov 28, 2022 |
|
Detection of a bright burst from the repeating FRB 20201124A at 2 GHz
|
Nov 28, 2022 |
|
X-ray emission from a rapidly accreting narrow-line Seyfert 1 galaxy at z=6 56
|
Nov 28, 2022 |
|
A global view on star formation: The GLOSTAR Galactic plane survey VII Supernova remnants in the Galactic longitude range 28^ circ
|
Nov 28, 2022 |
|
Detection of Einstein Telescope gravitational wave signals from binary black holes using deep learning
|
Nov 28, 2022 |
|
Investigating Non-linear and Stochastic Hard X-ray Variability of Active Galactic Nuclei using Recurrence Analysis
|
Nov 28, 2022 |
|
Application of Convolutional Neural Networks to Predict Magnetic Fields Directions in Turbulent Clouds
|
Nov 28, 2022 |
|
H ^ 13 CN-HN ^ 13 C intensity ratio as a temperature indicator of interstellar clouds
|
Nov 28, 2022 |
|
Strong Dark Matter Self-interactions Diversify Halo Populations Within and Surrounding the Milky Way
|
Nov 28, 2022 |
|
X-ray Polarization Observations of BL Lacertae
|
Nov 28, 2022 |
|
MOSEL Survey: Extremely weak outflows in EoR analogues at z=3-4
|
Nov 28, 2022 |
|
Chasing Super-Massive Black Hole merging events with Athena and LISA
|
Nov 28, 2022 |
|
Water and an escaping helium tail detected in the hazy and methane-depleted atmosphere of HAT-P-18b from JWST NIRISS SOSS
|
Nov 28, 2022 |
|
Propeller states in locally super-critical ULXs
|
Nov 28, 2022 |
|
Formation of a barred galaxy in a major merger: The role of AGN feedback
|
Nov 28, 2022 |
|
Study of vibrational spectra of polycyclic aromatic hydrocarbons with phenyl side group
|
Nov 28, 2022 |
|
Evidence for non-merger co-evolution of galaxies and their supermassive black holes
|
Nov 28, 2022 |
|
Formation of the Mg II h and k polarization profiles in a solar plage model and their suitability to infer magnetic fields
|
Nov 28, 2022 |
|
Hybrid α -attractors, primordial black holes and gravitational wave backgrounds
|
Nov 28, 2022 |
|
Crustal magnetic fields do not lead to magnetar-strength amplifications in binary neutron-star mergers
|
Nov 28, 2022 |
|
BEAGLE-AGN I: Simultaneous constraints on the properties of gas in star-forming and AGN narrow-line regions in galaxies
|
Nov 28, 2022 |
|
Molecules in the peculiar age-defying source IRAS 19312+1950
|
Nov 28, 2022 |
|
Deep solar ALMA neural network estimator for image refinement and estimates of small-scale dynamics
|
Nov 28, 2022 |
|
An Hα Impression of Lyα Galaxies at z simeq6 with Deep JWST NIRCam Imaging
|
Nov 28, 2022 |
|
Supermassive black holes in merger-free galaxies have higher spins which are preferentially aligned with their host galaxy
|
Nov 28, 2022 |
|
The properties of wind and jet from a super-Eddington accretion flow around a supermassive black hole
|
Nov 28, 2022 |
|
Tidally locked rotation of the dwarf planet 136199 Eris discovered from long-term ground based and space photometry
|
Nov 28, 2022 |
|
R-process nucleosynthesis during explosion of low-mass neutron stars in close binaries
|
Nov 28, 2022 |
|
Relativistic Signatures of Flux Eruption Events Near Black Holes
|
Nov 28, 2022 |
|
The Merger Rate of Primordial Black Hole-Neutron Star Binaries in Ellipsoidal-Collapse Dark Matter Halo Models
|
Nov 28, 2022 |
|
The role of the turbulence driving mode for the Initial Mass Function
|
Nov 28, 2022 |
|
Early Results From GLASS-JWST XVII: Building the First Galaxies -- Chapter 1 Star Formation Histories at 5
|
Nov 28, 2022 |
|
New constraints on the Bray conservation-of-momentum natal kick model from multiple distinct observations
|
Nov 28, 2022 |
|
First Batch of Candidate Galaxies at Redshifts 11 to 20 Revealed by the James Webb Space Telescope Early Release Observations
|
Nov 28, 2022 |
|
Marginal Bayesian Statistics Using Masked Autoregressive Flows and Kernel Density Estimators with Examples in Cosmology
|
Nov 28, 2022 |
|
Characterisation of the MUSIC ASIC for large-area silicon photomultipliers for gamma-ray astronomy
|
Nov 28, 2022 |
|
Significance Mode Analysis SigMA for hierarchical structures An application to the Sco-Cen OB association
|
Nov 28, 2022 |
|
Tentative Evidence for Transit Timing Variations of WASP-161b
|
Nov 28, 2022 |
|
On the Jacobi capture origin of binaries with applications to the Earth-Moon system and black holes in galactic nuclei
|
Nov 28, 2022 |
|
The Second Love Number of Dark Compact Planets and Neutron Stars with Dark Matter
|
Nov 28, 2022 |
|
Cross-correlation of DES Y3 lensing and ACT it Planck thermal Sunyaev Zel'dovich Effect II: Modeling and constraints on halo pressure profiles
|
Nov 28, 2022 |
|
Timing and Spectral Studies of the X-ray Pulsar 2S 1417 - 624 During the Outburst in 2021
|
Nov 28, 2022 |
|
Constraints on the Model of Gamma-ray Bursts and Implications from GRB 221009A: GeV gamma rays v s High-energy Neutrinos
|
Nov 28, 2022 |
|
Galaxies with Abnormally High Gas Content in the Disk
|
Nov 28, 2022 |
|
PHANGS-JWST First Results: A combined HST and JWST analysis of the nuclear star cluster in NGC 628
|
Nov 28, 2022 |
|
Searches for Neutrinos from LHAASO ultra-high-energy γ-ray sources using the IceCube Neutrino Observatory
|
Nov 28, 2022 |
|
Decade Long Timing Study of the Black Widow Millisecond Pulsar J1544+4937
|
Nov 27, 2022 |
|
Electron acceleration at supernova remnants
|
Nov 27, 2022 |
|
Hidden Cooling Flows in Clusters of Galaxies II: A Wider Sample
|
Nov 27, 2022 |
|
Sparse Bayesian mass-mapping using trans-dimensional MCMC
|
Nov 27, 2022 |
|
Probability Distribution Functions of Sunspot Magnetic Flux
|
Nov 27, 2022 |
|
High-energy Neutrino Productions from AGN Disk Transients Impacted by Circum-disk Medium
|
Nov 27, 2022 |
|
Threshold of Primordial Black Hole Formation against Velocity Dispersion in Matter-Dominated Era
|
Nov 27, 2022 |
|
Logarithmic Duality of the Curvature Perturbation
|
Nov 27, 2022 |
|
A Generalized Analytical Model For Thermal And Bulk Comptonization In Accretion-Powered X-Ray Pulsars
|
Nov 27, 2022 |
|
Modeling Hadronic Gamma-ray Emissions from Solar Flares and Prospects for Detecting Non-thermal Signatures from Protostars
|
Nov 27, 2022 |
|
Ganymede MHD Model: Magnetospheric Context for Juno's PJ34 Flyby
|
Nov 27, 2022 |
|
Pulsar Glitches: A Review
|
Nov 27, 2022 |
|
Asymmetry in the number of L4 and L5 Jupiter Trojans driven by jumping Jupiter
|
Nov 27, 2022 |
|
Removal of point source leakage from time-order data filtering
|
Nov 27, 2022 |
|
A Chemical Study of Nine Star-forming Regions with Evidence of Infall Motion
|
Nov 27, 2022 |
|
Near-Infrared Spectroscopy of Ultracompact ion H 2 regions in W51A with NIFS ALTAIR
|
Nov 27, 2022 |
|
Detection of a bright burst from the repeating FRB 20201124A at 2 GHz
|
Nov 27, 2022 |
|
X-ray emission from a rapidly accreting narrow-line Seyfert 1 galaxy at z=6 56
|
Nov 27, 2022 |
|
A global view on star formation: The GLOSTAR Galactic plane survey VII Supernova remnants in the Galactic longitude range 28^ circ
|
Nov 27, 2022 |
|
Detection of Einstein Telescope gravitational wave signals from binary black holes using deep learning
|
Nov 27, 2022 |
|
Investigating Non-linear and Stochastic Hard X-ray Variability of Active Galactic Nuclei using Recurrence Analysis
|
Nov 27, 2022 |
|
H ^ 13 CN-HN ^ 13 C intensity ratio as a temperature indicator of interstellar clouds
|
Nov 27, 2022 |
|
Strong Dark Matter Self-interactions Diversify Halo Populations Within and Surrounding the Milky Way
|
Nov 27, 2022 |
|
X-ray Polarization Observations of BL Lacertae
|
Nov 27, 2022 |
|
MOSEL Survey: Extremely weak outflows in EoR analogues at z=3-4
|
Nov 27, 2022 |
|
Chasing Super-Massive Black Hole merging events with Athena and LISA
|
Nov 27, 2022 |
|
Water and an escaping helium tail detected in the hazy and methane-depleted atmosphere of HAT-P-18b from JWST NIRISS SOSS
|
Nov 27, 2022 |
|
Propeller states in locally super-critical ULXs
|
Nov 27, 2022 |
|
Formation of a barred galaxy in a major merger: The role of AGN feedback
|
Nov 27, 2022 |
|
Study of vibrational spectra of polycyclic aromatic hydrocarbons with phenyl side group
|
Nov 27, 2022 |
|
Evidence for non-merger co-evolution of galaxies and their supermassive black holes
|
Nov 27, 2022 |
|
Formation of the Mg II h and k polarization profiles in a solar plage model and their suitability to infer magnetic fields
|
Nov 27, 2022 |
|
Crustal magnetic fields do not lead to magnetar-strength amplifications in binary neutron-star mergers
|
Nov 27, 2022 |
|
BEAGLE-AGN I: Simultaneous constraints on the properties of gas in star-forming and AGN narrow-line regions in galaxies
|
Nov 27, 2022 |
|
Molecules in the peculiar age-defying source IRAS 19312+1950
|
Nov 27, 2022 |
|
Deep solar ALMA neural network estimator for image refinement and estimates of small-scale dynamics
|
Nov 27, 2022 |
|
An Hα Impression of Lyα Galaxies at z simeq6 with Deep JWST NIRCam Imaging
|
Nov 27, 2022 |
|
Supermassive black holes in merger-free galaxies have higher spins which are preferentially aligned with their host galaxy
|
Nov 27, 2022 |
|
The properties of wind and jet from a super-Eddington accretion flow around a supermassive black hole
|
Nov 27, 2022 |
|
Tidally locked rotation of the dwarf planet 136199 Eris discovered from long-term ground based and space photometry
|
Nov 27, 2022 |
|
R-process nucleosynthesis during explosion of low-mass neutron stars in close binaries
|
Nov 27, 2022 |
|
Relativistic Signatures of Flux Eruption Events Near Black Holes
|
Nov 27, 2022 |
|
The Merger Rate of Primordial Black Hole-Neutron Star Binaries in Ellipsoidal-Collapse Dark Matter Halo Models
|
Nov 27, 2022 |
|
The role of the turbulence driving mode for the Initial Mass Function
|
Nov 27, 2022 |
|
Early Results From GLASS-JWST XVII: Building the First Galaxies -- Chapter 1 Star Formation Histories at 5
|
Nov 27, 2022 |
|
New constraints on the Bray conservation-of-momentum natal kick model from multiple distinct observations
|
Nov 27, 2022 |
|
First Batch of Candidate Galaxies at Redshifts 11 to 20 Revealed by the James Webb Space Telescope Early Release Observations
|
Nov 27, 2022 |
|
Marginal Bayesian Statistics Using Masked Autoregressive Flows and Kernel Density Estimators with Examples in Cosmology
|
Nov 27, 2022 |
|
Characterisation of the MUSIC ASIC for large-area silicon photomultipliers for gamma-ray astronomy
|
Nov 27, 2022 |
|
Tentative Evidence for Transit Timing Variations of WASP-161b
|
Nov 27, 2022 |
|
On the Jacobi capture origin of binaries with applications to the Earth-Moon system and black holes in galactic nuclei
|
Nov 27, 2022 |
|
The Second Love Number of Dark Compact Planets and Neutron Stars with Dark Matter
|
Nov 27, 2022 |
|
Cross-correlation of DES Y3 lensing and ACT it Planck thermal Sunyaev Zel'dovich Effect II: Modeling and constraints on halo pressure profiles
|
Nov 27, 2022 |
|
Timing and Spectral Studies of the X-ray Pulsar 2S 1417 - 624 During the Outburst in 2021
|
Nov 27, 2022 |
|
Galaxies with Abnormally High Gas Content in the Disk
|
Nov 27, 2022 |
|
PHANGS-JWST First Results: A combined HST and JWST analysis of the nuclear star cluster in NGC 628
|
Nov 27, 2022 |
|
Costs and benefits of automation for astronomical facilities
|
Nov 25, 2022 |
|
iMaNGA: mock MaNGA galaxies based on IllustrisTNG-50 and MaStar SSPs II the catalogue
|
Nov 25, 2022 |
|
First spatially resolved Na I and He I transitions towards an MYSO Finding new tracers for the gaseous star disc interface
|
Nov 25, 2022 |
|
OI 6300Å , emission as a probe of external photoevaporation of protoplanetary discs
|
Nov 25, 2022 |
|
Deep Herschel observations of the 2Jy sample: assessing the non-thermal and AGN contributions to the far-IR continuum
|
Nov 25, 2022 |
|
A study of oxygen-rich post-AGB stars in the Milky Way to understand the production of silicates from evolved stars
|
Nov 25, 2022 |
|
Connecting Solar Orbiter remote-sensing observations and Parker Solar Probe in-situ measurements with a numerical MHD reconstruction of the Parker spiral
|
Nov 25, 2022 |
|
Tracing the ICME plasma with a MHD simulation
|
Nov 25, 2022 |
|
Investigating the origin of optical and X-ray pulsations of the transitional millisecond pulsar PSR J1023+0038
|
Nov 25, 2022 |
|
PDFchem: A new fast method to determine ISM properties and infer environmental parameters using probability distributions
|
Nov 25, 2022 |
|
FOREVER22: the first bright galaxies with population III stars at redshifts z simeq 10-20 and comparisons with JWST data
|
Nov 25, 2022 |
|
Misaligned jets from Sgr A ^* and the origin of Fermi eROSITA bubbles
|
Nov 25, 2022 |
|
Euclid preparation XXVII Covariance model validation for the 2-point correlation function of galaxy clusters
|
Nov 25, 2022 |
|
Regularization of Single Field Inflation Models
|
Nov 25, 2022 |
|
Emergence of smooth distance and apparent magnitude in a lumpy Universe
|
Nov 25, 2022 |
|
Taking a break: paused accretion in the symbiotic binary RT Cru
|
Nov 25, 2022 |
|
Nuclear Activity in the Low Metallicity Dwarf Galaxy SDSS J0944-0038: A Glimpse into the Primordial Universe
|
Nov 25, 2022 |
|
Background rejection using image residuals from large telescopes in imaging atmospheric Cherenkov telescope arrays
|
Nov 25, 2022 |
|
Newly discovered Ca II absorbers in the early universe: statistics, element abundances and dust
|
Nov 25, 2022 |
|
How Close Dark Matter Halos and MOND Are to Each Other: Three-Dimensional Tests Based on Gaia DR2
|
Nov 25, 2022 |
|
Constraints on Yukawa gravity parameters from observations of bright stars
|
Nov 24, 2022 |
|
Costs and benefits of automation for astronomical facilities
|
Nov 24, 2022 |
|
Discovery and description of two young open clusters in the primordial group of NGC 6871
|
Nov 24, 2022 |
|
iMaNGA: mock MaNGA galaxies based on IllustrisTNG-50 and MaStar SSPs II the catalogue
|
Nov 24, 2022 |
|
First estimate of the local value of the baryonic streaming velocity
|
Nov 24, 2022 |
|
First spatially resolved Na I and He I transitions towards an MYSO Finding new tracers for the gaseous star disc interface
|
Nov 24, 2022 |
|
Is there a Dynamic Difference between Stealthy and Standard CMEs?
|
Nov 24, 2022 |
|
A comparative study of source-finding techniques in HI emission line cubes using SoFiA, MTObjects, and supervised deep learning
|
Nov 24, 2022 |
|
Sub-mm mm optical properties of real protoplanetary matter derived from Rosetta MIRO observations of comet 67P
|
Nov 24, 2022 |
|
OI 6300Å , emission as a probe of external photoevaporation of protoplanetary discs
|
Nov 24, 2022 |
|
The circular polarization of the Mn I resonance lines around 280 nm for exploring chromospheric magnetism
|
Nov 24, 2022 |
|
Deep Herschel observations of the 2Jy sample: assessing the non-thermal and AGN contributions to the far-IR continuum
|
Nov 24, 2022 |
|
One-loop tensor power spectrum from an excited scalar field during inflation
|
Nov 24, 2022 |
|
A study of oxygen-rich post-AGB stars in the Milky Way to understand the production of silicates from evolved stars
|
Nov 24, 2022 |
|
Interferometric imaging of the type IIIb and U radio bursts observed with LOFAR on 22 August 2017
|
Nov 24, 2022 |
|
Connecting Solar Orbiter remote-sensing observations and Parker Solar Probe in-situ measurements with a numerical MHD reconstruction of the Parker spiral
|
Nov 24, 2022 |
|
Resonant friction on discs in galactic nuclei
|
Nov 24, 2022 |
|
Galaxy and Mass Assembly GAMA : Extended Intra-Group Light in a group at z=0 2 from deep Hyper-Suprime Cam images
|
Nov 24, 2022 |
|
Tracing the ICME plasma with a MHD simulation
|
Nov 24, 2022 |
|
Investigating the origin of optical and X-ray pulsations of the transitional millisecond pulsar PSR J1023+0038
|
Nov 24, 2022 |
|
Unresolved Binaries and Multiples in the Intermediate Mass Range in open clusters: Pleiades, Alpha Per, Praesepe, and NGC 1039
|
Nov 24, 2022 |
|
PDFchem: A new fast method to determine ISM properties and infer environmental parameters using probability distributions
|
Nov 24, 2022 |
|
FOREVER22: the first bright galaxies with population III stars at redshifts z simeq 10-20 and comparisons with JWST data
|
Nov 24, 2022 |
|
The Effects of Gas Angular Momentum on Forming Magnetically Arrested Disks and Launching Powerful Jets
|
Nov 24, 2022 |
|
Misaligned jets from Sgr A ^* and the origin of Fermi eROSITA bubbles
|
Nov 24, 2022 |
|
Sound people speak to Star people A sound experts perspective on astronomy sonification projects
|
Nov 24, 2022 |
|
Euclid preparation XXVII Covariance model validation for the 2-point correlation function of galaxy clusters
|
Nov 24, 2022 |
|
HIGlow: Conditional Normalizing Flows for High-Fidelity HI Map Modeling
|
Nov 24, 2022 |
|
Regularization of Single Field Inflation Models
|
Nov 24, 2022 |
|
Theory and Phenomenology of Stressed Ψ DM Soliton
|
Nov 24, 2022 |
|
Emergence of smooth distance and apparent magnitude in a lumpy Universe
|
Nov 24, 2022 |
|
Isochrone fitting of Galactic globular clusters -- IV NGC6362 and NGC6723
|
Nov 24, 2022 |
|
Comparison of the Core-Collapse Evolution of Two Nearly Equal Mass Progenitors
|
Nov 24, 2022 |
|
Inferring Maps of the Sun's Far-side Unsigned Magnetic Flux from Far-side Helioseismic Images using Machine Learning Techniques
|
Nov 24, 2022 |
|
On the hysteresis effect in transitions between accretion and propeller regimes
|
Nov 24, 2022 |
|
Taking a break: paused accretion in the symbiotic binary RT Cru
|
Nov 24, 2022 |
|
Identifying and Characterizing the Most Heavily Dust-Obscured Galaxies at 1 le z le 4
|
Nov 24, 2022 |
|
Tracking ALMA System Temperature with Water Vapor Data at High Frequency
|
Nov 24, 2022 |
|
Nearly Model-Independent Constraints on the Neutral Hydrogen Fraction in the Intergalactic Medium at z sim 5-7 Using Dark Pixel Fractions in Ly α and Ly β Forests
|
Nov 24, 2022 |
|
HOPS 361-C's Jet Decelerating and Precessing Through NGC 2071 IR
|
Nov 24, 2022 |
|
A Swing of the Pendulum: The Chemodynamics of the Local Stellar Halo Indicate Contributions from Several Radial Merger Events
|
Nov 24, 2022 |
|
A Study of Warm Dark Matter, the Missing Satellites Problem, and the UV Luminosity Cut-Off
|
Nov 24, 2022 |
|
The CO 2 Profile and Analytical Model for the Pioneer Venus Large Probe Neutral Mass Spectrometer
|
Nov 24, 2022 |
|
Using conditional variational autoencoders to generate images from atmospheric Cherenkov telescopes
|
Nov 24, 2022 |
|
Wideband timing of the Parkes Pulsar Timing Array UWL data
|
Nov 24, 2022 |
|
The production of ionizing photons in UV-faint z~3-7 galaxies
|
Nov 24, 2022 |
|
Radiative Transfer as a Bayesian Linear Regression problem
|
Nov 24, 2022 |
|
EAVN Astrometry toward the Extreme Outer Galaxy: Kinematic distance with the proper motion of G034 84-00 95
|
Nov 24, 2022 |
|
A dichotomy in group II Herbig disks: ALMA gas disk height measurements show both shadowed large vertically extended disks and compact flat disks
|
Nov 24, 2022 |
|
Differences in chemical evolution between isolated and embedded prestellar cores
|
Nov 24, 2022 |
|
Constraints on modified gravity from the BOSS galaxy survey
|
Nov 24, 2022 |
|
MASCOT: Molecular gas depletion times and metallicity gradients -- evidence for feedback in quenching active galaxies
|
Nov 24, 2022 |
|
Limiting the accretion disk light in two mass transferring hot subdwarf binaries
|
Nov 24, 2022 |
|
Polarization From A Radially Stratified Off-Axis GRB Outflow
|
Nov 24, 2022 |
|
Efficient exploration of reionization parameters for the upcoming 21 cm observations using a photon conserving semi-numerical model SCRIPT
|
Nov 24, 2022 |
|
Nuclear Activity in the Low Metallicity Dwarf Galaxy SDSS J0944-0038: A Glimpse into the Primordial Universe
|
Nov 24, 2022 |
|
Euclid: Modelling massive neutrinos in cosmology -- a code comparison
|
Nov 24, 2022 |
|
Can denoising diffusion probabilistic models generate realistic astrophysical fields?
|
Nov 24, 2022 |
|
Cool, Luminous, and Highly Variable Stars in the Magellanic Clouds II: Spectroscopic and Environmental Analysis of Thorne-Żytkow Object and Super-AGB Star Candidates
|
Nov 24, 2022 |
|
Pre-solar grains from novae and "Born-again giants"
|
Nov 24, 2022 |
|
Adding Gamma-ray Polarimetry to the Multi-Messenger Era
|
Nov 24, 2022 |
|
Deep X-ray and radio observations of the first outburst of the young magnetar Swift J1818 0-1607
|
Nov 24, 2022 |
|
Dust-free starburst galaxies at redshifts z>10
|
Nov 24, 2022 |
|
A closer look at supernovae as seeds for galactic magnetization
|
Nov 24, 2022 |
|
Cosmology from Galaxy Redshift Surveys with PointNet
|
Nov 24, 2022 |
|
Generation of solar chromosphere heating and coronal outflows by two-fluid waves
|
Nov 24, 2022 |
|
Hot subdwarf stars identified in LAMOST DR8 with single-lined and composite spectra
|
Nov 24, 2022 |
|
Spectral analysis of basaltic asteroids observed by the Gaia space mission
|
Nov 24, 2022 |
|
A new technique to isolate kinematically anomalous gas in HI data cubes
|
Nov 24, 2022 |
|
The spatially resolved view of star formation in galaxy clusters
|
Nov 24, 2022 |
|
Two-fluid numerical model of chromospheric heating and plasma outflows in a quiet-Sun
|
Nov 24, 2022 |
|
ALMA Fragmented Source Catalogue in Orion FraSCO I Outflow interaction within an embedded cluster in OMC-2 FIR3, FIR4, and FIR5
|
Nov 24, 2022 |
|
Towards a new era in giant exoplanet characterisation
|
Nov 24, 2022 |
|
Cosmic Topology I: Limits on Orientable Euclidean Manifolds from Circle Searches
|
Nov 24, 2022 |
|
Background rejection using image residuals from large telescopes in imaging atmospheric Cherenkov telescope arrays
|
Nov 24, 2022 |
|
The dynamical state of the globular clusters Rup 106 and IC 4499
|
Nov 24, 2022 |
|
The GRAVITY Young Stellar Object survey -- IX Spatially resolved kinematics of hot hydrogen gas in the star disk interaction region of T Tauri stars
|
Nov 24, 2022 |
|
Effects of Planetesimal Scattering: Explaining the Observed Offsets from Period Ratios 3:2 and 2:1
|
Nov 24, 2022 |
|
The structure at the centre of the giant radio galaxy GRS J0844+4627: a compact symmetric object?
|
Nov 24, 2022 |
|
Plasma lensing near the eclipses of the Black Widow pulsar B1957+20
|
Nov 24, 2022 |
|
Direct Discovery of the Inner Exoplanet in the HD206893 System
|
Nov 24, 2022 |
|
Massive black hole binaries in LISA: multimessenger prospects and electromagnetic counterparts
|
Nov 24, 2022 |
|
Newly discovered Ca II absorbers in the early universe: statistics, element abundances and dust
|
Nov 24, 2022 |
|
EMPRESS IX Extremely Metal-Poor Galaxies are Very Gas-Rich Dispersion-Dominated Systems: Will JWST Witness Gaseous Turbulent High-z Primordial Galaxies?
|
Nov 24, 2022 |
|
Constraints on the Optical Depth to Reionization from Balloon-Borne CMB Measurements
|
Nov 24, 2022 |
|
Short GRB Host Galaxies II A Legacy Sample of Redshifts, Stellar Population Properties, and Implications for their Neutron Star Merger Origins
|
Nov 24, 2022 |
|
3D Simulations of Strongly Magnetised Non-Rotating Supernovae: Explosion Dynamics and Remnant Properties
|
Nov 24, 2022 |
|
Simulating Hydrodynamics in Cosmology with CRK-HACC
|
Nov 24, 2022 |
|
Ultra-low-frequency gravitational waves from individual supermassive black hole binaries as standard sirens
|
Nov 24, 2022 |
|
Saturn's Seasonal Atmosphere at Northern Summer Solstice
|
Nov 24, 2022 |
|
How Close Dark Matter Halos and MOND Are to Each Other: Three-Dimensional Tests Based on Gaia DR2
|
Nov 24, 2022 |
|
Improving CME evolution and arrival predictions with AMR and grid stretching in Icarus
|
Nov 24, 2022 |
|
Launching the VASCO citizen science project
|
Nov 24, 2022 |
|
Observing the inspiral of coalescing massive black hole binaries with LISA in the era of Multi-Messenger Astrophysics
|
Nov 24, 2022 |
|
The CO 2 Profile and Analytical Model for the Pioneer Venus Large Probe Neutral Mass Spectrometer
|
Nov 23, 2022 |
|
Constraints on Yukawa gravity parameters from observations of bright stars
|
Nov 23, 2022 |
|
Discovery and description of two young open clusters in the primordial group of NGC 6871
|
Nov 23, 2022 |
|
First estimate of the local value of the baryonic streaming velocity
|
Nov 23, 2022 |
|
Is there a Dynamic Difference between Stealthy and Standard CMEs?
|
Nov 23, 2022 |
|
A comparative study of source-finding techniques in HI emission line cubes using SoFiA, MTObjects, and supervised deep learning
|
Nov 23, 2022 |
|
Sub-mm mm optical properties of real protoplanetary matter derived from Rosetta MIRO observations of comet 67P
|
Nov 23, 2022 |
|
The circular polarization of the Mn I resonance lines around 280 nm for exploring chromospheric magnetism
|
Nov 23, 2022 |
|
One-loop tensor power spectrum from an excited scalar field during inflation
|
Nov 23, 2022 |
|
Interferometric imaging of the type IIIb and U radio bursts observed with LOFAR on 22 August 2017
|
Nov 23, 2022 |
|
Resonant friction on discs in galactic nuclei
|
Nov 23, 2022 |
|
Galaxy and Mass Assembly GAMA : Extended Intra-Group Light in a group at z=0 2 from deep Hyper-Suprime Cam images
|
Nov 23, 2022 |
|
Unresolved Binaries and Multiples in the Intermediate Mass Range in open clusters: Pleiades, Alpha Per, Praesepe, and NGC 1039
|
Nov 23, 2022 |
|
The Effects of Gas Angular Momentum on Forming Magnetically Arrested Disks and Launching Powerful Jets
|
Nov 23, 2022 |
|
Sound people speak to Star people A sound experts perspective on astronomy sonification projects
|
Nov 23, 2022 |
|
HIGlow: Conditional Normalizing Flows for High-Fidelity HI Map Modeling
|
Nov 23, 2022 |
|
Theory and Phenomenology of Stressed Ψ DM Soliton
|
Nov 23, 2022 |
|
Isochrone fitting of Galactic globular clusters -- IV NGC6362 and NGC6723
|
Nov 23, 2022 |
|
Comparison of the Core-Collapse Evolution of Two Nearly Equal Mass Progenitors
|
Nov 23, 2022 |
|
Inferring Maps of the Sun's Far-side Unsigned Magnetic Flux from Far-side Helioseismic Images using Machine Learning Techniques
|
Nov 23, 2022 |
|
On the hysteresis effect in transitions between accretion and propeller regimes
|
Nov 23, 2022 |
|
Identifying and Characterizing the Most Heavily Dust-Obscured Galaxies at 1 le z le 4
|
Nov 23, 2022 |
|
Tracking ALMA System Temperature with Water Vapor Data at High Frequency
|
Nov 23, 2022 |
|
Nearly Model-Independent Constraints on the Neutral Hydrogen Fraction in the Intergalactic Medium at z sim 5-7 Using Dark Pixel Fractions in Ly α and Ly β Forests
|
Nov 23, 2022 |
|
HOPS 361-C's Jet Decelerating and Precessing Through NGC 2071 IR
|
Nov 23, 2022 |
|
A Swing of the Pendulum: The Chemodynamics of the Local Stellar Halo Indicate Contributions from Several Radial Merger Events
|
Nov 23, 2022 |
|
A Study of Warm Dark Matter, the Missing Satellites Problem, and the UV Luminosity Cut-Off
|
Nov 23, 2022 |
|
The CO2 Profile and Analytical Model for the Pioneer Venus Large Probe Neutral Mass Spectrometer
|
Nov 23, 2022 |
|
Using conditional variational autoencoders to generate images from atmospheric Cherenkov telescopes
|
Nov 23, 2022 |
|
Wideband timing of the Parkes Pulsar Timing Array UWL data
|
Nov 23, 2022 |
|
The production of ionizing photons in UV-faint z~3-7 galaxies
|
Nov 23, 2022 |
|
Radiative Transfer as a Bayesian Linear Regression problem
|
Nov 23, 2022 |
|
EAVN Astrometry toward the Extreme Outer Galaxy: Kinematic distance with the proper motion of G034 84-00 95
|
Nov 23, 2022 |
|
A dichotomy in group II Herbig disks: ALMA gas disk height measurements show both shadowed large vertically extended disks and compact flat disks
|
Nov 23, 2022 |
|
Differences in chemical evolution between isolated and embedded prestellar cores
|
Nov 23, 2022 |
|
Constraints on modified gravity from the BOSS galaxy survey
|
Nov 23, 2022 |
|
MASCOT: Molecular gas depletion times and metallicity gradients -- evidence for feedback in quenching active galaxies
|
Nov 23, 2022 |
|
Limiting the accretion disk light in two mass transferring hot subdwarf binaries
|
Nov 23, 2022 |
|
Polarization From A Radially Stratified Off-Axis GRB Outflow
|
Nov 23, 2022 |
|
Efficient exploration of reionization parameters for the upcoming 21 cm observations using a photon conserving semi-numerical model SCRIPT
|
Nov 23, 2022 |
|
Euclid: Modelling massive neutrinos in cosmology -- a code comparison
|
Nov 23, 2022 |
|
Can denoising diffusion probabilistic models generate realistic astrophysical fields?
|
Nov 23, 2022 |
|
Cool, Luminous, and Highly Variable Stars in the Magellanic Clouds II: Spectroscopic and Environmental Analysis of Thorne-Żytkow Object and Super-AGB Star Candidates
|
Nov 23, 2022 |
|
Pre-solar grains from novae and "Born-again giants"
|
Nov 23, 2022 |
|
Adding Gamma-ray Polarimetry to the Multi-Messenger Era
|
Nov 23, 2022 |
|
Deep X-ray and radio observations of the first outburst of the young magnetar Swift J1818 0-1607
|
Nov 23, 2022 |
|
Dust-free starburst galaxies at redshifts z>10
|
Nov 23, 2022 |
|
A closer look at supernovae as seeds for galactic magnetization
|
Nov 23, 2022 |
|
Cosmology from Galaxy Redshift Surveys with PointNet
|
Nov 23, 2022 |
|
Generation of solar chromosphere heating and coronal outflows by two-fluid waves
|
Nov 23, 2022 |
|
Hot subdwarf stars identified in LAMOST DR8 with single-lined and composite spectra
|
Nov 23, 2022 |
|
Spectral analysis of basaltic asteroids observed by the Gaia space mission
|
Nov 23, 2022 |
|
A new technique to isolate kinematically anomalous gas in HI data cubes
|
Nov 23, 2022 |
|
The spatially resolved view of star formation in galaxy clusters
|
Nov 23, 2022 |
|
Two-fluid numerical model of chromospheric heating and plasma outflows in a quiet-Sun
|
Nov 23, 2022 |
|
ALMA Fragmented Source Catalogue in Orion FraSCO I Outflow interaction within an embedded cluster in OMC-2 FIR3, FIR4, and FIR5
|
Nov 23, 2022 |
|
Towards a new era in giant exoplanet characterisation
|
Nov 23, 2022 |
|
Cosmic Topology I: Limits on Orientable Euclidean Manifolds from Circle Searches
|
Nov 23, 2022 |
|
The dynamical state of the globular clusters Rup 106 and IC 4499
|
Nov 23, 2022 |
|
The GRAVITY Young Stellar Object survey -- IX Spatially resolved kinematics of hot hydrogen gas in the star disk interaction region of T Tauri stars
|
Nov 23, 2022 |
|
Effects of Planetesimal Scattering: Explaining the Observed Offsets from Period Ratios 3:2 and 2:1
|
Nov 23, 2022 |
|
The structure at the centre of the giant radio galaxy GRS J0844+4627: a compact symmetric object?
|
Nov 23, 2022 |
|
Plasma lensing near the eclipses of the Black Widow pulsar B1957+20
|
Nov 23, 2022 |
|
Direct Discovery of the Inner Exoplanet in the HD206893 System
|
Nov 23, 2022 |
|
Massive black hole binaries in LISA: multimessenger prospects and electromagnetic counterparts
|
Nov 23, 2022 |
|
EMPRESS IX Extremely Metal-Poor Galaxies are Very Gas-Rich Dispersion-Dominated Systems: Will JWST Witness Gaseous Turbulent High-z Primordial Galaxies?
|
Nov 23, 2022 |
|
Constraints on the Optical Depth to Reionization from Balloon-Borne CMB Measurements
|
Nov 23, 2022 |
|
Short GRB Host Galaxies II A Legacy Sample of Redshifts, Stellar Population Properties, and Implications for their Neutron Star Merger Origins
|
Nov 23, 2022 |
|
3D Simulations of Strongly Magnetised Non-Rotating Supernovae: Explosion Dynamics and Remnant Properties
|
Nov 23, 2022 |
|
Simulating Hydrodynamics in Cosmology with CRK-HACC
|
Nov 23, 2022 |
|
Ultra-low-frequency gravitational waves from individual supermassive black hole binaries as standard sirens
|
Nov 23, 2022 |
|
Saturn's Seasonal Atmosphere at Northern Summer Solstice
|
Nov 23, 2022 |
|
Improving CME evolution and arrival predictions with AMR and grid stretching in Icarus
|
Nov 23, 2022 |
|
Launching the VASCO citizen science project
|
Nov 23, 2022 |
|
Observing the inspiral of coalescing massive black hole binaries with LISA in the era of Multi-Messenger Astrophysics
|
Nov 23, 2022 |
|
Limiting the accretion disk light in two mass transferring hot subdwarf binaries
|
Nov 23, 2022 |
|
On the evolution of the particle distribution and the cascade in a moving, expanding emission region in blazar jets
|
Nov 23, 2022 |
|
Winds of OB stars: impact of metallicity, rotation and binary interaction
|
Nov 23, 2022 |
|
Kilonova and Optical Afterglow from Binary Neutron Star Mergers II Optimal Search Strategy for Serendipitous Observations and Target-of-opportunity Observations of Gravitational-wave Triggers
|
Nov 23, 2022 |
|
A closer look at supernovae as seeds for galactic magnetization
|
Nov 23, 2022 |
|
Hydrostatic Mass Profiles of Galaxy Clusters in the eROSITA Survey
|
Nov 23, 2022 |
|
ALMA Fragmented Source Catalogue in Orion FraSCO I Outflow interaction within an embedded cluster in OMC-2 FIR3, FIR4, and FIR5
|
Nov 23, 2022 |
|
Cosmology from Galaxy Redshift Surveys with PointNet
|
Nov 23, 2022 |
|
Hot subdwarf stars identified in LAMOST DR8 with single-lined and composite spectra
|
Nov 23, 2022 |
|
Spectral analysis of basaltic asteroids observed by the Gaia space mission
|
Nov 23, 2022 |
|
A new technique to isolate kinematically anomalous gas in HI data cubes
|
Nov 23, 2022 |
|
Daksha: On Alert for High Energy Transients
|
Nov 23, 2022 |
|
3D RMHD simulations of the Gamma-ray binaries
|
Nov 23, 2022 |
|
The spatially resolved view of star formation in galaxy clusters
|
Nov 23, 2022 |
|
Science with the Daksha High Energy Transients Mission
|
Nov 23, 2022 |
|
Two-fluid numerical model of chromospheric heating and plasma outflows in a quiet-Sun
|
Nov 23, 2022 |
|
Towards a new era in giant exoplanet characterisation
|
Nov 23, 2022 |
|
Cosmic Topology I: Limits on Orientable Euclidean Manifolds from Circle Searches
|
Nov 23, 2022 |
|
Image plane detection of FRB121102 with the MeerKAT radio telescope
|
Nov 23, 2022 |
|
Polarization From A Radially Stratified Off-Axis GRB Outflow
|
Nov 23, 2022 |
|
The structure at the centre of the giant radio galaxy GRS J0844+4627: a compact symmetric object?
|
Nov 23, 2022 |
|
Repeating fast radio bursts produced by a strange star interacting with its planet in an eccentric orbit
|
Nov 23, 2022 |
|
Asteroseismology of the pulsating extremely low-mass white dwarf SDSS J111215 82+111745 0: a model with p -mode pulsations consistent with the observations
|
Nov 23, 2022 |
|
Massive black hole binaries in LISA: multimessenger prospects and electromagnetic counterparts
|
Nov 23, 2022 |
|
Formation, Possible Detection and Consequences of Highly Magnetized Compact Stars
|
Nov 23, 2022 |
|
Constraints on the Optical Depth to Reionization from Balloon-Borne CMB Measurements
|
Nov 23, 2022 |
|
Witnessing a Galaxy Cluster Merger with JWST and a Chandra X-ray Temperature Map
|
Nov 23, 2022 |
|
Impact of the nonthermal electron radiation effects on the horizon scale image structure of Sagittarius A*
|
Nov 23, 2022 |
|
Short GRB Host Galaxies II A Legacy Sample of Redshifts, Stellar Population Properties, and Implications for their Neutron Star Merger Origins
|
Nov 23, 2022 |
|
Launching the VASCO citizen science project
|
Nov 23, 2022 |
|
Primordial black holes from D-parity breaking in SO 10 grand unified theory
|
Nov 23, 2022 |
|
King Ghidorah Supercluster: Mapping the light and dark matter in a new supercluster at z=0 55 using the Subaru Hyper Suprime-Cam
|
Nov 23, 2022 |
|
Observing the inspiral of coalescing massive black hole binaries with LISA in the era of Multi-Messenger Astrophysics
|
Nov 23, 2022 |
|
Rarefied Broad-Line Regions in Active Galactic Nuclei: Anomalous Responses in Reverberation Mapping and Implications for Weak-Emission Line Quasars
|
Nov 23, 2022 |
|
Second order scalar perturbations induced by primordial curvature and tensor perturbations
|
Nov 23, 2022 |
|
Euclid: Modelling massive neutrinos in cosmology -- a code comparison
|
Nov 23, 2022 |
|
Mesh-free hydrodynamics in PKDGRAV3 for galaxy formation simulations
|
Nov 23, 2022 |
|
A targeted search for repeating fast radio bursts with the MWA
|
Nov 23, 2022 |
|
Traveling planetary-scale waves cause cloud variability on tidally locked aquaplanets
|
Nov 23, 2022 |
|
CLASS Survey Description: Coronal Line Needles in the SDSS Haystack
|
Nov 23, 2022 |
|
The Statistics of Negative Power Spectrum Systematics in some 21 cm Analyses
|
Nov 23, 2022 |
|
The Thousand-Pulsar-Array program on MeerKAT -- IX The time-averaged properties of the observed pulsar population
|
Nov 23, 2022 |
|
Measuring the Obliquities of the TRAPPIST-1 Planets with MAROON-X
|
Nov 23, 2022 |
|
Is the hot, dense sub-Neptune TOI-824b an exposed Neptune mantle? Spitzer detection of the hot day side and reanalysis of the interior composition
|
Nov 23, 2022 |
|
Unsupervised classification reveals new evolutionary pathways
|
Nov 23, 2022 |
|
MaNGIA: 10,000 mock galaxies for stellar population analysis
|
Nov 23, 2022 |
|
Modelling the accretion and feedback of supermassive black hole binaries in gas-rich galaxy mergers
|
Nov 23, 2022 |
|
Can denoising diffusion probabilistic models generate realistic astrophysical fields?
|
Nov 23, 2022 |
|
MeerKAT follow-up of enigmatic GLEAM 4-Jy G4Jy sources
|
Nov 23, 2022 |
|
Reconstructing and Classifying SDSS DR16 Galaxy Spectra with Machine-Learning and Dimensionality Reduction Algorithms
|
Nov 23, 2022 |
|
Quasar Factor Analysis -- An Unsupervised and Probabilistic Quasar Continuum Prediction Algorithm with Latent Factor Analysis
|
Nov 23, 2022 |
|
The dark side of galaxy stellar populations II: The dependence of star formation histories on halo mass and on the scatter of the main sequence
|
Nov 23, 2022 |
|
Density Profiles of Collapsed Rotating Massive Stars Favor Long Gamma-Ray Bursts
|
Nov 23, 2022 |
|
Removal of Hot Saturns in Mass-Radius Plane by Runaway Mass Loss
|
Nov 23, 2022 |
|
Active galactic nucleus jet feedback in hydrostatic halos
|
Nov 23, 2022 |
|
Compact object mergers: exploring uncertainties from stellar and binary evolution with SEVN
|
Nov 23, 2022 |
|
GalaxyFlow: Upsampling Hydrodynamical Simulations for Realistic Gaia Mock Catalogs
|
Nov 23, 2022 |
|
Cool, Luminous, and Highly Variable Stars in the Magellanic Clouds II: Spectroscopic and Environmental Analysis of Thorne-Żytkow Object and Super-AGB Star Candidates
|
Nov 23, 2022 |
|
Coronal seismology by slow waves in non-adiabatic conditions
|
Nov 23, 2022 |
|
The high-albedo, low polarization disk around HD 114082 harbouring a Jupiter-sized transiting planet
|
Nov 23, 2022 |
|
Consistent and simultaneous modelling of galaxy clustering and galaxy-galaxy lensing with Subhalo Abundance Matching
|
Nov 23, 2022 |
|
A tactile model of the night summer northern sky for the teaching of astronomy to the BVI
|
Nov 23, 2022 |
|
Predicting sub-millimeter flux densities from global galaxy properties
|
Nov 23, 2022 |
|
GD 99: re-investigation of an old ZZ Ceti friend
|
Nov 23, 2022 |
|
Investigating the Evolution of Amati Parameters with Redshift
|
Nov 23, 2022 |
|
Massive star cluster origin for the galactic cosmic ray population at very-high energies
|
Nov 23, 2022 |
|
Bose-Einstein Condensate Dark Matter That Involves Composites
|
Nov 23, 2022 |
|
Cosmography using strongly lensed gravitational waves from binary black holes
|
Nov 23, 2022 |
|
Pre-solar grains from novae and "Born-again giants"
|
Nov 23, 2022 |
|
Probing phase transition in neutron stars via the crust-core interfacial mode
|
Nov 23, 2022 |
|
The propertities of wind and jet from a super-Eddington accretion flow around a supermassive black hole
|
Nov 23, 2022 |
|
A General Bayesian Framework to Account for Foreground Map Errors in Global 21-cm Experiments
|
Nov 23, 2022 |
|
Line Emission Mapper LEM : Probing the physics of cosmic ecosystems
|
Nov 23, 2022 |
|
Observability of signatures of transport-induced chemistry in clear atmospheres of hot gas giant exoplanets
|
Nov 23, 2022 |
|
Bright X-ray Pulsars: how outflows influence beaming, pulsations and pulse phase lags
|
Nov 23, 2022 |
|
Non-perturbative non-Gaussianity and primordial black holes
|
Nov 23, 2022 |
|
Analysis of the arm-like structure in the outer disk of PDS 70 Spiral density wave or vortex?
|
Nov 23, 2022 |
|
Missed opportunities: GRB 211211A and the case for continual gravitational-wave coverage with a single observatory
|
Nov 23, 2022 |
|
Active Galactic Nuclei as potential Sources of Ultra-High Energy Cosmic Rays
|
Nov 23, 2022 |
|
Adding Gamma-ray Polarimetry to the Multi-Messenger Era
|
Nov 23, 2022 |
|
If dark matter is fuzzy, the first stars form in massive pancakes
|
Nov 23, 2022 |
|
On the cosmic evolution of AGN obscuration and the X-ray luminosity function: XMM-Newton and Chandra spectral analysis of the 31 3 deg ^2 Stripe 82X
|
Nov 23, 2022 |
|
A Milliarcsecond-accurate Position for Sagittarius A*
|
Nov 23, 2022 |
|
Radio Emission of Nearby Early-type Galaxies at Low and Very-Low Radio Luminosity Range
|
Nov 23, 2022 |
|
Mapping NGC 7027 in New Light: CO ^+ and HCO ^+ Emission Reveal Its Photon- and X-ray-Dominated Regions
|
Nov 23, 2022 |
|
Etherington duality breaking: gravitational lensing in non-metric spacetimes versus intrinsic alignments
|
Nov 23, 2022 |
|
First release of Apertif imaging survey data
|
Nov 23, 2022 |
|
Reconstructing the Assembly of Massive Galaxies II Galaxies Develop Massive and Dense Stellar Cores as They Evolve and Head Toward Quiescence at Cosmic Noon
|
Nov 23, 2022 |
|
Gravitational Waves from the Propagation of Long Gamma-Ray Burst jets
|
Nov 23, 2022 |
|
Application of convolutional neural networks for data analysis in TAIGA-HiSCORE experiment
|
Nov 23, 2022 |
|
Deep X-ray and radio observations of the first outburst of the young magnetar Swift J1818 0-1607
|
Nov 23, 2022 |
|
A new resonance-like feature in the outer disc of the Milky Way
|
Nov 23, 2022 |
|
The Rotation Period Distribution in the Young Open Cluster NGC 6709
|
Nov 23, 2022 |
|
Using wavelets to capture deviations from smoothness in galaxy-scale strong lenses
|
Nov 23, 2022 |
|
The Science Performance of JWST as Characterized in Commissioning
|
Nov 23, 2022 |
|
Dark matter halos and scaling relations of extremely massive spiral galaxies from extended HI rotation curves
|
Nov 23, 2022 |
|
Redshift requirements for cosmic shear with intrinsic alignment
|
Nov 23, 2022 |
|
Perihelion Activity of 3200 Phaethon Is Not Dusty
|
Nov 23, 2022 |
|
Dust-free starburst galaxies at redshifts z>10
|
Nov 23, 2022 |
|
Revisiting the Spectral-Energy Correlations of GRBs with it Fermi Data I: Model-wise Properties
|
Nov 23, 2022 |
|
The POKEMON Speckle Survey of Nearby M dwarfs I New Discoveries
|
Nov 23, 2022 |
|
New pulse profile variability associated with a glitch of PSR J0738-4042
|
Nov 23, 2022 |
|
Gravitational waves from small spin-up and spin-down events of neutron stars
|
Nov 23, 2022 |
|
PyNAPLE: Lunar Surface Impact Crater Detection
|
Nov 23, 2022 |
|
Constrains on the physics of the prompt emission from a distant and energetic gamma-ray burst GRB 220101A
|
Nov 23, 2022 |
|
Preferential Accretion and Circumbinary Disk Precession in Eccentric Binary Systems
|
Nov 23, 2022 |
|
Characterization and dynamics of the peculiar stream Jhelum, A tentative role for the Sagittarius dwarf galaxy
|
Nov 23, 2022 |
|
Properties beyond mass for unresolved haloes across redshift and cosmology using correlations with local halo environment
|
Nov 23, 2022 |
|
On the evolution of the particle distribution and the cascade in a moving, expanding emission region in blazar jets
|
Nov 22, 2022 |
|
Winds of OB stars: impact of metallicity, rotation and binary interaction
|
Nov 22, 2022 |
|
Kilonova and Optical Afterglow from Binary Neutron Star Mergers II Optimal Search Strategy for Serendipitous Observations and Target-of-opportunity Observations of Gravitational-wave Triggers
|
Nov 22, 2022 |
|
Hydrostatic Mass Profiles of Galaxy Clusters in the eROSITA Survey
|
Nov 22, 2022 |
|
ALMA Fragmented Source Catalogue in Orion FraSCO I Outflow interaction within an embedded cluster in OMC-2 FIR3, FIR4, and FIR5
|
Nov 22, 2022 |
|
Daksha: On Alert for High Energy Transients
|
Nov 22, 2022 |
|
3D RMHD simulations of the Gamma-ray binaries
|
Nov 22, 2022 |
|
Science with the Daksha High Energy Transients Mission
|
Nov 22, 2022 |
|
Image plane detection of FRB121102 with the MeerKAT radio telescope
|
Nov 22, 2022 |
|
Repeating fast radio bursts produced by a strange star interacting with its planet in an eccentric orbit
|
Nov 22, 2022 |
|
Asteroseismology of the pulsating extremely low-mass white dwarf SDSS J111215 82+111745 0: a model with p -mode pulsations consistent with the observations
|
Nov 22, 2022 |
|
Formation, Possible Detection and Consequences of Highly Magnetized Compact Stars
|
Nov 22, 2022 |
|
Witnessing a Galaxy Cluster Merger with JWST and a Chandra X-ray Temperature Map
|
Nov 22, 2022 |
|
Impact of the nonthermal electron radiation effects on the horizon scale image structure of Sagittarius A*
|
Nov 22, 2022 |
|
Primordial black holes from D-parity breaking in SO 10 grand unified theory
|
Nov 22, 2022 |
|
King Ghidorah Supercluster: Mapping the light and dark matter in a new supercluster at z=0 55 using the Subaru Hyper Suprime-Cam
|
Nov 22, 2022 |
|
Rarefied Broad-Line Regions in Active Galactic Nuclei: Anomalous Responses in Reverberation Mapping and Implications for Weak-Emission Line Quasars
|
Nov 22, 2022 |
|
Second order scalar perturbations induced by primordial curvature and tensor perturbations
|
Nov 22, 2022 |
|
Mesh-free hydrodynamics in PKDGRAV3 for galaxy formation simulations
|
Nov 22, 2022 |
|
A targeted search for repeating fast radio bursts with the MWA
|
Nov 22, 2022 |
|
Traveling planetary-scale waves cause cloud variability on tidally locked aquaplanets
|
Nov 22, 2022 |
|
CLASS Survey Description: Coronal Line Needles in the SDSS Haystack
|
Nov 22, 2022 |
|
The Statistics of Negative Power Spectrum Systematics in some 21 cm Analyses
|
Nov 22, 2022 |
|
The Thousand-Pulsar-Array program on MeerKAT -- IX The time-averaged properties of the observed pulsar population
|
Nov 22, 2022 |
|
Measuring the Obliquities of the TRAPPIST-1 Planets with MAROON-X
|
Nov 22, 2022 |
|
Is the hot, dense sub-Neptune TOI-824b an exposed Neptune mantle? Spitzer detection of the hot day side and reanalysis of the interior composition
|
Nov 22, 2022 |
|
Unsupervised classification reveals new evolutionary pathways
|
Nov 22, 2022 |
|
MaNGIA: 10,000 mock galaxies for stellar population analysis
|
Nov 22, 2022 |
|
Modelling the accretion and feedback of supermassive black hole binaries in gas-rich galaxy mergers
|
Nov 22, 2022 |
|
MeerKAT follow-up of enigmatic GLEAM 4-Jy G4Jy sources
|
Nov 22, 2022 |
|
Reconstructing and Classifying SDSS DR16 Galaxy Spectra with Machine-Learning and Dimensionality Reduction Algorithms
|
Nov 22, 2022 |
|
Quasar Factor Analysis -- An Unsupervised and Probabilistic Quasar Continuum Prediction Algorithm with Latent Factor Analysis
|
Nov 22, 2022 |
|
The dark side of galaxy stellar populations II: The dependence of star formation histories on halo mass and on the scatter of the main sequence
|
Nov 22, 2022 |
|
Density Profiles of Collapsed Rotating Massive Stars Favor Long Gamma-Ray Bursts
|
Nov 22, 2022 |
|
Removal of Hot Saturns in Mass-Radius Plane by Runaway Mass Loss
|
Nov 22, 2022 |
|
Active galactic nucleus jet feedback in hydrostatic halos
|
Nov 22, 2022 |
|
Compact object mergers: exploring uncertainties from stellar and binary evolution with SEVN
|
Nov 22, 2022 |
|
GalaxyFlow: Upsampling Hydrodynamical Simulations for Realistic Gaia Mock Catalogs
|
Nov 22, 2022 |
|
Coronal seismology by slow waves in non-adiabatic conditions
|
Nov 22, 2022 |
|
The high-albedo, low polarization disk around HD 114082 harbouring a Jupiter-sized transiting planet
|
Nov 22, 2022 |
|
Consistent and simultaneous modelling of galaxy clustering and galaxy-galaxy lensing with Subhalo Abundance Matching
|
Nov 22, 2022 |
|
A tactile model of the night summer northern sky for the teaching of astronomy to the BVI
|
Nov 22, 2022 |
|
Predicting sub-millimeter flux densities from global galaxy properties
|
Nov 22, 2022 |
|
GD 99: re-investigation of an old ZZ Ceti friend
|
Nov 22, 2022 |
|
Investigating the Evolution of Amati Parameters with Redshift
|
Nov 22, 2022 |
|
Massive star cluster origin for the galactic cosmic ray population at very-high energies
|
Nov 22, 2022 |
|
Bose-Einstein Condensate Dark Matter That Involves Composites
|
Nov 22, 2022 |
|
Cosmography using strongly lensed gravitational waves from binary black holes
|
Nov 22, 2022 |
|
Probing phase transition in neutron stars via the crust-core interfacial mode
|
Nov 22, 2022 |
|
The propertities of wind and jet from a super-Eddington accretion flow around a supermassive black hole
|
Nov 22, 2022 |
|
A General Bayesian Framework to Account for Foreground Map Errors in Global 21-cm Experiments
|
Nov 22, 2022 |
|
Line Emission Mapper LEM : Probing the physics of cosmic ecosystems
|
Nov 22, 2022 |
|
Observability of signatures of transport-induced chemistry in clear atmospheres of hot gas giant exoplanets
|
Nov 22, 2022 |
|
Bright X-ray Pulsars: how outflows influence beaming, pulsations and pulse phase lags
|
Nov 22, 2022 |
|
Non-perturbative non-Gaussianity and primordial black holes
|
Nov 22, 2022 |
|
Analysis of the arm-like structure in the outer disk of PDS 70 Spiral density wave or vortex?
|
Nov 22, 2022 |
|
Missed opportunities: GRB 211211A and the case for continual gravitational-wave coverage with a single observatory
|
Nov 22, 2022 |
|
Active Galactic Nuclei as potential Sources of Ultra-High Energy Cosmic Rays
|
Nov 22, 2022 |
|
If dark matter is fuzzy, the first stars form in massive pancakes
|
Nov 22, 2022 |
|
On the cosmic evolution of AGN obscuration and the X-ray luminosity function: XMM-Newton and Chandra spectral analysis of the 31 3 deg ^2 Stripe 82X
|
Nov 22, 2022 |
|
A Milliarcsecond-accurate Position for Sagittarius A*
|
Nov 22, 2022 |
|
Radio Emission of Nearby Early-type Galaxies at Low and Very-Low Radio Luminosity Range
|
Nov 22, 2022 |
|
Mapping NGC 7027 in New Light: CO ^+ and HCO ^+ Emission Reveal Its Photon- and X-ray-Dominated Regions
|
Nov 22, 2022 |
|
Etherington duality breaking: gravitational lensing in non-metric spacetimes versus intrinsic alignments
|
Nov 22, 2022 |
|
First release of Apertif imaging survey data
|
Nov 22, 2022 |
|
Reconstructing the Assembly of Massive Galaxies II Galaxies Develop Massive and Dense Stellar Cores as They Evolve and Head Toward Quiescence at Cosmic Noon
|
Nov 22, 2022 |
|
Gravitational Waves from the Propagation of Long Gamma-Ray Burst jets
|
Nov 22, 2022 |
|
Application of convolutional neural networks for data analysis in TAIGA-HiSCORE experiment
|
Nov 22, 2022 |
|
A new resonance-like feature in the outer disc of the Milky Way
|
Nov 22, 2022 |
|
The Rotation Period Distribution in the Young Open Cluster NGC 6709
|
Nov 22, 2022 |
|
Using wavelets to capture deviations from smoothness in galaxy-scale strong lenses
|
Nov 22, 2022 |
|
The Science Performance of JWST as Characterized in Commissioning
|
Nov 22, 2022 |
|
Dark matter halos and scaling relations of extremely massive spiral galaxies from extended HI rotation curves
|
Nov 22, 2022 |
|
Redshift requirements for cosmic shear with intrinsic alignment
|
Nov 22, 2022 |
|
Perihelion Activity of 3200 Phaethon Is Not Dusty
|
Nov 22, 2022 |
|
Revisiting the Spectral-Energy Correlations of GRBs with it Fermi Data I: Model-wise Properties
|
Nov 22, 2022 |
|
The POKEMON Speckle Survey of Nearby M dwarfs I New Discoveries
|
Nov 22, 2022 |
|
New pulse profile variability associated with a glitch of PSR J0738-4042
|
Nov 22, 2022 |
|
Gravitational waves from small spin-up and spin-down events of neutron stars
|
Nov 22, 2022 |
|
PyNAPLE: Lunar Surface Impact Crater Detection
|
Nov 22, 2022 |
|
Constrains on the physics of the prompt emission from a distant and energetic gamma-ray burst GRB 220101A
|
Nov 22, 2022 |
|
Preferential Accretion and Circumbinary Disk Precession in Eccentric Binary Systems
|
Nov 22, 2022 |
|
Characterization and dynamics of the peculiar stream Jhelum, A tentative role for the Sagittarius dwarf galaxy
|
Nov 22, 2022 |
|
Properties beyond mass for unresolved haloes across redshift and cosmology using correlations with local halo environment
|
Nov 22, 2022 |
|
Consistent and simultaneous modelling of galaxy clustering and galaxy-galaxy lensing with Subhalo Abundance Matching
|
Nov 22, 2022 |
|
Probing phase transition in neutron stars via the crust-core interfacial mode
|
Nov 22, 2022 |
|
Simulations of PBH formation at the QCD epoch and comparison with the GWTC-3 catalog
|
Nov 22, 2022 |
|
Line Emission Mapper LEM : Probing the physics of cosmic ecosystems
|
Nov 22, 2022 |
|
Peering into the Milky Way by FAST: IV Identification of two new Galactic supernova remnants G203 1+6 6 and G206 7+5 9
|
Nov 22, 2022 |
|
Observability of signatures of transport-induced chemistry in clear atmospheres of hot gas giant exoplanets
|
Nov 22, 2022 |
|
Sudden braking and turning in the single multi-stream inflation: primordial black hole formation
|
Nov 22, 2022 |
|
Analysis of the arm-like structure in the outer disk of PDS 70 Spiral density wave or vortex?
|
Nov 22, 2022 |
|
Black holes shielded by magnetic fields
|
Nov 22, 2022 |
|
If dark matter is fuzzy, the first stars form in massive pancakes
|
Nov 22, 2022 |
|
Peering into the Milky Way by FAST: III Magnetic fields in the Galactic halo and farther spiral arms revealed by the Faraday effect of faint pulsars
|
Nov 22, 2022 |
|
On the cosmic evolution of AGN obscuration and the X-ray luminosity function: XMM-Newton and Chandra spectral analysis of the 31 3 deg ^2 Stripe 82X
|
Nov 22, 2022 |
|
Peering into the Milky Way by FAST: II Ionized gas in the inner Galactic disk revealed by the piggyback line observations of the FAST GPPS survey
|
Nov 22, 2022 |
|
Peering into the Milky Way by FAST: I Exquisite HI structures in the inner Galactic disk from the piggyback line observations of the FAST GPPS survey
|
Nov 22, 2022 |
|
Radio Emission of Nearby Early-type Galaxies at Low and Very-Low Radio Luminosity Range
|
Nov 22, 2022 |
|
The RATAN-600 multi-frequency catalogue of blazars -- BLcat
|
Nov 22, 2022 |
|
Gravitational Waves from the Propagation of Long Gamma-Ray Burst jets
|
Nov 22, 2022 |
|
3D Detection and Characterisation of ALMA Sources through Deep Learning
|
Nov 22, 2022 |
|
A tactile model of the night summer northern sky for the teaching of astronomy to the BVI
|
Nov 22, 2022 |
|
Comparison of magnetic energy and helicity in coronal jet simulations
|
Nov 22, 2022 |
|
Using wavelets to capture deviations from smoothness in galaxy-scale strong lenses
|
Nov 22, 2022 |
|
Magnetic activities and parameters of 43 flare stars in the GWAC archive
|
Nov 22, 2022 |
|
The Science Performance of JWST as Characterized in Commissioning
|
Nov 22, 2022 |
|
Dark matter halos and scaling relations of extremely massive spiral galaxies from extended HI rotation curves
|
Nov 22, 2022 |
|
Rapid radio brightening of GRB 210702A
|
Nov 22, 2022 |
|
Characterising the high-mass star forming region IRAS 18144-1723 through methanol maser observations
|
Nov 22, 2022 |
|
The POKEMON Speckle Survey of Nearby M dwarfs I New Discoveries
|
Nov 22, 2022 |
|
Comparing hierarchical black hole mergers in star clusters and active galactic nuclei
|
Nov 22, 2022 |
|
Gravitational waves from small spin-up and spin-down events of neutron stars
|
Nov 22, 2022 |
|
Failed Solar Eruption of A Multi-thermal Flux Rope
|
Nov 22, 2022 |
|
Preferential Accretion and Circumbinary Disk Precession in Eccentric Binary Systems
|
Nov 22, 2022 |
|
Increasing mass-to-flux ratio from the dense core to the protostellar envelope around the Class 0 protostar HH 211
|
Nov 22, 2022 |
|
H-FISTA: A hierarchical algorithm for phase retrieval with application to pulsar dynamic spectra
|
Nov 22, 2022 |
|
The LOFAR Tied-Array All-Sky Survey: Timing of 35 radio pulsars and an overview of the properties of the LOFAR pulsar discoveries
|
Nov 22, 2022 |
|
Exhaustive Symbolic Regression
|
Nov 22, 2022 |
|
Predicting sub-millimeter flux densities from global galaxy properties
|
Nov 22, 2022 |
|
Solar energetic electron events measured by MESSENGER and Solar Orbiter Peak intensity and energy spectrum radial dependences: statistical analysis
|
Nov 22, 2022 |
|
IWDM: The fate of an interacting non-cold dark matter - vacuum scenario
|
Nov 22, 2022 |
|
Dusty plasma in active galactic nuclei
|
Nov 22, 2022 |
|
Unidentified infrared bands do not correlate with C O ratio in planetary nebulae
|
Nov 22, 2022 |
|
Finding active galactic nuclei through Fink
|
Nov 22, 2022 |
|
Open clusters: time-scales, core collapse and blue stragglers
|
Nov 22, 2022 |
|
Proximity Operations about Apophis through its 2029 Earth Flyby
|
Nov 22, 2022 |
|
Magnetic dynamo caused by axions in neutron stars
|
Nov 22, 2022 |
|
GD 99: re-investigation of an old ZZ Ceti friend
|
Nov 22, 2022 |
|
The Driving of Hot Star Winds
|
Nov 22, 2022 |
|
X-ray and optical spectroscopic study of a gamma Cassiopeiae analog source pi Aquarii
|
Nov 22, 2022 |
|
A bias-free cosmological analysis with quasars alleviating H 0 tension
|
Nov 22, 2022 |
|
Halted-Pendulum Relaxation: Application to White Dwarf Binary Initial Data
|
Nov 22, 2022 |
|
Photometric Properties of Jupiter Trojans detected by the Dark Energy Survey
|
Nov 22, 2022 |
|
The propertities of wind and jet from a super-Eddington accretion flow around a supermassive black hole
|
Nov 22, 2022 |
|
The Isaac Newton Telescope monitoring survey of Local Group dwarf galaxies--V The star formation history of Sagittarius dwarf irregular galaxy derived from long period variable stars
|
Nov 22, 2022 |
|
DESI Mock Challenge VII: halo and galaxy catalogs with the Bias Assignment Method
|
Nov 22, 2022 |
|
Venus Life Finder Habitability Mission: Motivation, Science Objectives, and Instrumentation
|
Nov 22, 2022 |
|
High and dry: billion-year trends in the aridity of river-forming climates on Mars
|
Nov 22, 2022 |
|
The luminous type Ia supernova 2022ilv and its early excess emission
|
Nov 22, 2022 |
|
Rome Precision Solar Photometric Telescope: precision solar full-disk photometry during solar cycles 23-25
|
Nov 22, 2022 |
|
Global simulations of Tayler instability in stellar interiors: a long-time multi-stage evolution of the magnetic field
|
Nov 22, 2022 |
|
Velocity-Coherent Substructure in TMC-1: Inflow and Fragmentation
|
Nov 22, 2022 |
|
Starlet higher order statistics for galaxy clustering and weak lensing
|
Nov 22, 2022 |
|
How does dark matter affect compact star properties and high density constraints of strongly interacting matter
|
Nov 22, 2022 |
|
Early Release Science of the exoplanet WASP-39b with JWST NIRISS
|
Nov 22, 2022 |
|
Rocky histories: The effect of high excitations on the formation of rocky planets
|
Nov 22, 2022 |
|
Investigating the Evolution of Amati Parameters with Redshift
|
Nov 22, 2022 |
|
Kinetically stabilized inflation
|
Nov 22, 2022 |
|
Direct Evidence of Photochemistry in an Exoplanet Atmosphere
|
Nov 22, 2022 |
|
Early Release Science of the Exoplanet WASP-39b with JWST NIRSpec G395H
|
Nov 22, 2022 |
|
Early Release Science of the exoplanet WASP-39b with JWST NIRCam
|
Nov 22, 2022 |
|
Early Release Science of the exoplanet WASP-39b with JWST NIRSpec PRISM
|
Nov 22, 2022 |
|
Scalable Bayesian Inference for Finding Strong Gravitational Lenses
|
Nov 22, 2022 |
|
Formation of Lunar Basins from Impacts of Leftover Planetesimals
|
Nov 22, 2022 |
|
The Molecular-Gas Main Sequence and Schmidt-Kennicutt relation are fundamental, the Star-Forming Main Sequence is a useful byproduct
|
Nov 22, 2022 |
|
A simple spectroscopic technique to identify rejuvenating galaxies
|
Nov 22, 2022 |
|
A General Bayesian Framework to Account for Foreground Map Errors in Global 21-cm Experiments
|
Nov 22, 2022 |
|
Investigating dark energy by electromagnetic frequency shifts II: the Pantheon+ sample
|
Nov 22, 2022 |
|
Massive star cluster origin for the galactic cosmic ray population at very-high energies
|
Nov 22, 2022 |
|
Hydrodynamical Simulations of Black-Hole Binary Formation in AGN Disks
|
Nov 22, 2022 |
|
Surviving in Ocean Worlds: Experimental Characterization of Fiber Optic Tethers across Europa-like Ice Faults and Unraveling the Sliding Behavior of Ice
|
Nov 22, 2022 |
|
A strong H- opacity signal in the near-infrared emission spectrum of the ultra-hot Jupiter KELT-9b
|
Nov 22, 2022 |
|
Understanding the role of morphology and environment on the dynamical evolution of isolated galaxy triplets
|
Nov 22, 2022 |
|
MeV-GeV Gamma-ray Emission from SNR G327 1-1 1 Discovered by the Fermi-LAT
|
Nov 22, 2022 |
|
CARMA-NRO Orion Survey: unbiased survey of dense cores and core mass functions in Orion A
|
Nov 22, 2022 |
|
Bose-Einstein Condensate Dark Matter That Involves Composites
|
Nov 22, 2022 |
|
Broadband Spectral properties of MAXI J1348--630 using AstroSat Observations
|
Nov 22, 2022 |
|
The microvariability and wavelength dependence of polarization degree angle of BL Lacertae in the outburst 2020 to 2021
|
Nov 22, 2022 |
|
Dusty winds clear JWST super-early galaxies
|
Nov 22, 2022 |
|
i-SPin: An integrator for multicomponent Schrödinger-Poisson systems with self-interactions
|
Nov 22, 2022 |
|
Eccentricity or spin precession? Distinguishing subdominant effects in gravitational-wave data
|
Nov 22, 2022 |
|
Saturn's Seasonal Variability from Four Decades of Ground-Based Mid-Infrared Observations
|
Nov 22, 2022 |
|
The unaltered pulsar: GRO J1750-27, a super-critical X-ray neutron star that does not blink an eye
|
Nov 22, 2022 |
|
The galaxy formation origin of the lensing is low problem
|
Nov 22, 2022 |
|
Diversity of dust properties in external galaxies confirmed by polarization signals from Type II supernovae
|
Nov 22, 2022 |
|
A ~200 pc-sized core of Milky Way dark matter halo constrained from the OGLE micro-lensing sky map
|
Nov 22, 2022 |
|
GRaM-X: A new GPU-accelerated dynamical spacetime GRMHD code for Exascale computing with the Einstein Toolkit
|
Nov 22, 2022 |
|
Interpreting molecular hydrogen and atomic oxygen line emission of T Tauri disks with photoevaporative disk-wind models
|
Nov 22, 2022 |
|
How to Interpret Measurements of Diffuse Light in Stacked Observations of Groups and Clusters of Galaxies
|
Nov 22, 2022 |
|
Temporal evolution and rigidity dependence of the solar modulation lag of Galactic cosmic rays
|
Nov 22, 2022 |
|
Accuracy and precision of triaxial orbit models II: Viewing angles, shape and orbital structure
|
Nov 22, 2022 |
|
Impact of Rastall gravity on mass, radius and sound speed of the pulsar PSR J0740+6620
|
Nov 22, 2022 |
|
Large Field Polynomial Inflation: Parameter Space, Predictions and Double Eternal Nature
|
Nov 22, 2022 |
|
Simulations of PBH formation at the QCD epoch and comparison with the GWTC-3 catalog
|
Nov 21, 2022 |
|
Peering into the Milky Way by FAST: IV Identification of two new Galactic supernova remnants G203 1+6 6 and G206 7+5 9
|
Nov 21, 2022 |
|
Sudden braking and turning in the single multi-stream inflation: primordial black hole formation
|
Nov 21, 2022 |
|
Black holes shielded by magnetic fields
|
Nov 21, 2022 |
|
Peering into the Milky Way by FAST: III Magnetic fields in the Galactic halo and farther spiral arms revealed by the Faraday effect of faint pulsars
|
Nov 21, 2022 |
|
Peering into the Milky Way by FAST: II Ionized gas in the inner Galactic disk revealed by the piggyback line observations of the FAST GPPS survey
|
Nov 21, 2022 |
|
Peering into the Milky Way by FAST: I Exquisite HI structures in the inner Galactic disk from the piggyback line observations of the FAST GPPS survey
|
Nov 21, 2022 |
|
The RATAN-600 multi-frequency catalogue of blazars -- BLcat
|
Nov 21, 2022 |
|
3D Detection and Characterisation of ALMA Sources through Deep Learning
|
Nov 21, 2022 |
|
Comparison of magnetic energy and helicity in coronal jet simulations
|
Nov 21, 2022 |
|
Magnetic activities and parameters of 43 flare stars in the GWAC archive
|
Nov 21, 2022 |
|
Rapid radio brightening of GRB 210702A
|
Nov 21, 2022 |
|
Characterising the high-mass star forming region IRAS 18144-1723 through methanol maser observations
|
Nov 21, 2022 |
|
Comparing hierarchical black hole mergers in star clusters and active galactic nuclei
|
Nov 21, 2022 |
|
Failed Solar Eruption of A Multi-thermal Flux Rope
|
Nov 21, 2022 |
|
Increasing mass-to-flux ratio from the dense core to the protostellar envelope around the Class 0 protostar HH 211
|
Nov 21, 2022 |
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H-FISTA: A hierarchical algorithm for phase retrieval with application to pulsar dynamic spectra
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Nov 21, 2022 |
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The LOFAR Tied-Array All-Sky Survey: Timing of 35 radio pulsars and an overview of the properties of the LOFAR pulsar discoveries
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Nov 21, 2022 |
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Exhaustive Symbolic Regression
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Nov 21, 2022 |
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Solar energetic electron events measured by MESSENGER and Solar Orbiter Peak intensity and energy spectrum radial dependences: statistical analysis
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Nov 21, 2022 |
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IWDM: The fate of an interacting non-cold dark matter - vacuum scenario
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Nov 21, 2022 |
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Dusty plasma in active galactic nuclei
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Nov 21, 2022 |
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Unidentified infrared bands do not correlate with C O ratio in planetary nebulae
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Nov 21, 2022 |
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Finding active galactic nuclei through Fink
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Nov 21, 2022 |
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Open clusters: time-scales, core collapse and blue stragglers
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Nov 21, 2022 |
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Proximity Operations about Apophis through its 2029 Earth Flyby
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Nov 21, 2022 |
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Magnetic dynamo caused by axions in neutron stars
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Nov 21, 2022 |
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The Driving of Hot Star Winds
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Nov 21, 2022 |
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X-ray and optical spectroscopic study of a gamma Cassiopeiae analog source pi Aquarii
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Nov 21, 2022 |
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A bias-free cosmological analysis with quasars alleviating H 0 tension
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Nov 21, 2022 |
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Halted-Pendulum Relaxation: Application to White Dwarf Binary Initial Data
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Nov 21, 2022 |
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Photometric Properties of Jupiter Trojans detected by the Dark Energy Survey
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Nov 21, 2022 |
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The propertities of wind and jet from a super-Eddington accretion flow around a supermassive black hole
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Nov 21, 2022 |
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The Isaac Newton Telescope monitoring survey of Local Group dwarf galaxies--V The star formation history of Sagittarius dwarf irregular galaxy derived from long period variable stars
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Nov 21, 2022 |
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DESI Mock Challenge VII: halo and galaxy catalogs with the Bias Assignment Method
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Nov 21, 2022 |
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Venus Life Finder Habitability Mission: Motivation, Science Objectives, and Instrumentation
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Nov 21, 2022 |
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High and dry: billion-year trends in the aridity of river-forming climates on Mars
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Nov 21, 2022 |
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The luminous type Ia supernova 2022ilv and its early excess emission
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Nov 21, 2022 |
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Rome Precision Solar Photometric Telescope: precision solar full-disk photometry during solar cycles 23-25
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Nov 21, 2022 |
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Global simulations of Tayler instability in stellar interiors: a long-time multi-stage evolution of the magnetic field
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Nov 21, 2022 |
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Velocity-Coherent Substructure in TMC-1: Inflow and Fragmentation
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Nov 21, 2022 |
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Starlet higher order statistics for galaxy clustering and weak lensing
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Nov 21, 2022 |
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How does dark matter affect compact star properties and high density constraints of strongly interacting matter
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Nov 21, 2022 |
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Early Release Science of the exoplanet WASP-39b with JWST NIRISS
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Nov 21, 2022 |
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Rocky histories: The effect of high excitations on the formation of rocky planets
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Nov 21, 2022 |
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Kinetically stabilized inflation
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Nov 21, 2022 |
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Direct Evidence of Photochemistry in an Exoplanet Atmosphere
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Nov 21, 2022 |
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Early Release Science of the Exoplanet WASP-39b with JWST NIRSpec G395H
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Nov 21, 2022 |
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Early Release Science of the exoplanet WASP-39b with JWST NIRCam
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Nov 21, 2022 |
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Early Release Science of the exoplanet WASP-39b with JWST NIRSpec PRISM
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Nov 21, 2022 |
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Scalable Bayesian Inference for Finding Strong Gravitational Lenses
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Nov 21, 2022 |
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Formation of Lunar Basins from Impacts of Leftover Planetesimals
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Nov 21, 2022 |
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The Molecular-Gas Main Sequence and Schmidt-Kennicutt relation are fundamental, the Star-Forming Main Sequence is a useful byproduct
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Nov 21, 2022 |
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A simple spectroscopic technique to identify rejuvenating galaxies
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Nov 21, 2022 |
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A General Bayesian Framework to Account for Foreground Map Errors in Global 21-cm Experiments
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Nov 21, 2022 |
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Investigating dark energy by electromagnetic frequency shifts II: the Pantheon+ sample
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Nov 21, 2022 |
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Hydrodynamical Simulations of Black-Hole Binary Formation in AGN Disks
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Nov 21, 2022 |
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Surviving in Ocean Worlds: Experimental Characterization of Fiber Optic Tethers across Europa-like Ice Faults and Unraveling the Sliding Behavior of Ice
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Nov 21, 2022 |
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A strong H- opacity signal in the near-infrared emission spectrum of the ultra-hot Jupiter KELT-9b
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Nov 21, 2022 |
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Understanding the role of morphology and environment on the dynamical evolution of isolated galaxy triplets
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Nov 21, 2022 |
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MeV-GeV Gamma-ray Emission from SNR G327 1-1 1 Discovered by the Fermi-LAT
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Nov 21, 2022 |
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CARMA-NRO Orion Survey: unbiased survey of dense cores and core mass functions in Orion A
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Nov 21, 2022 |
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Broadband Spectral properties of MAXI J1348--630 using AstroSat Observations
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Nov 21, 2022 |
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The microvariability and wavelength dependence of polarization degree angle of BL Lacertae in the outburst 2020 to 2021
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Nov 21, 2022 |
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Dusty winds clear JWST super-early galaxies
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Nov 21, 2022 |
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i-SPin: An integrator for multicomponent Schrödinger-Poisson systems with self-interactions
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Nov 21, 2022 |
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Eccentricity or spin precession? Distinguishing subdominant effects in gravitational-wave data
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Nov 21, 2022 |
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Saturn's Seasonal Variability from Four Decades of Ground-Based Mid-Infrared Observations
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Nov 21, 2022 |
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The unaltered pulsar: GRO J1750-27, a super-critical X-ray neutron star that does not blink an eye
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Nov 21, 2022 |
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The galaxy formation origin of the lensing is low problem
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Nov 21, 2022 |
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Diversity of dust properties in external galaxies confirmed by polarization signals from Type II supernovae
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Nov 21, 2022 |
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A ~200 pc-sized core of Milky Way dark matter halo constrained from the OGLE micro-lensing sky map
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Nov 21, 2022 |
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GRaM-X: A new GPU-accelerated dynamical spacetime GRMHD code for Exascale computing with the Einstein Toolkit
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Nov 21, 2022 |
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Interpreting molecular hydrogen and atomic oxygen line emission of T Tauri disks with photoevaporative disk-wind models
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Nov 21, 2022 |
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How to Interpret Measurements of Diffuse Light in Stacked Observations of Groups and Clusters of Galaxies
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Nov 21, 2022 |
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Temporal evolution and rigidity dependence of the solar modulation lag of Galactic cosmic rays
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Nov 21, 2022 |
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Accuracy and precision of triaxial orbit models II: Viewing angles, shape and orbital structure
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Nov 21, 2022 |
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Impact of Rastall gravity on mass, radius and sound speed of the pulsar PSR J0740+6620
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Nov 21, 2022 |
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Large Field Polynomial Inflation: Parameter Space, Predictions and Double Eternal Nature
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Nov 21, 2022 |
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The non-LTE formation of the Fe I 6173 A line in the solar atmosphere
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Nov 21, 2022 |
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Interpreting molecular hydrogen and atomic oxygen line emission of T Tauri disks with photoevaporative disk-wind models
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Nov 21, 2022 |
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Return of 4U~1730--22 after 49 years silence: the spectral properties of the 2021 2022 outbursts observed by NICER and Insight-HXMT and the soft-to-hard state transition caused by the propeller effect
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Nov 21, 2022 |
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Simulations of PBH formation at the QCD epoch and comparison with the GWTC-3 catalog
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Nov 21, 2022 |
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Transmission curves of narrow-band filters in large-FoV and fast astronomical instruments
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Nov 21, 2022 |
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Development of a trigger for acoustic neutrino candidates in KM3NeT
|
Nov 21, 2022 |
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X-ray Spectral Analysis of the Jet Termination Shock in Pictor A on Sub-Arcsecond Scales with Chandra
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Nov 21, 2022 |
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Dark dust II: Properties in the general field of the diffuse ISM
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Nov 21, 2022 |
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Primordial black holes induced stochastic axion-photon oscillations in primordial magnetic field
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Nov 21, 2022 |
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Is the core-cusp problem a matter of perspective: Jeans Anisotropic Modeling against numerical simulations
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Nov 21, 2022 |
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Jet-environment interplay in magnetized binary neutron star mergers
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Nov 21, 2022 |
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Modelling photo-evaporation in planet forming discs
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Nov 21, 2022 |
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Exploring the Phase Diagram of V-QCD with Neutron Star Merger Simulations
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Nov 21, 2022 |
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Prospects for constraining interacting dark energy models from gravitational wave and gamma ray burst joint observation
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Nov 21, 2022 |
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WISE Green Objects WGOs : the massive star candidates in the whole Galactic Plane mid b mid <2^ circ
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Nov 21, 2022 |
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Generalized equipartition method from an arbitrary viewing angle
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Nov 21, 2022 |
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Timescale-dependent X-ray to UV time lags of NGC 4593 using high-intensity XMM-Newton observations with Swift and AstroSat
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Nov 21, 2022 |
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High-Resolution Radio Study of the Dragonfly Nebula
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Nov 21, 2022 |
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Prompt emission and early optical afterglow of VHE detected GRB 201015A and GRB 201216C: onset of the external forward shock
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Nov 21, 2022 |
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Spectral Templates Optimal for Selecting Galaxies at z > 8 with JWST
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Nov 21, 2022 |
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Detection of the extended γ -ray emission from the high Galactic latitude Calvera's SNR candidate
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Nov 21, 2022 |
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First wide field-of-view X-ray observations by a lobster eye focusing telescope in orbit
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Nov 21, 2022 |
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X-ray from Outflow-Cloud Interaction and Its Application in Tidal Disruption Events
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Nov 21, 2022 |
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Changes of Magnetic Energy and Helicity in Solar Active Regions from Major Flares
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Nov 21, 2022 |
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pmwd: A Differentiable Cosmological Particle-Mesh N -body Library
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Nov 21, 2022 |
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Differentiable Cosmological Simulation with Adjoint Method
|
Nov 21, 2022 |
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Spectroscopic and Imaging Observations of Spatially Extended Magnetic Reconnection in the Splitting of a Solar Filament Structure
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Nov 21, 2022 |
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Simulating the charging of isolated free-falling masses from TeV to eV energies: detailed comparison with LISA Pathfinder results
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Nov 21, 2022 |
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Evolution of grain size distribution with enhanced abundance of small carbonaceous grains in galactic environments
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Nov 21, 2022 |
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Evidence for neutrino emission from the nearby active galaxy NGC 1068
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Nov 21, 2022 |
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Effects of Active Galactic Nucleus Feedback on Cold Gas Depletion and Quenching of Central Galaxies
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Nov 21, 2022 |
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Sub-kpc radio jets in the brightest central galaxy of the cool-core galaxy cluster RXJ1720 1+2638
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Nov 21, 2022 |
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Dominance of Bursty over Steady Heating of the 4--8 MK Coronal Plasma in a Solar Active Region: Quantification using Maps of Minimum, Maximum, and Average Brightness
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Nov 21, 2022 |
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Spectropolarimeter's optical design for the Arago space mission project
|
Nov 21, 2022 |
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CARMA-NRO Orion Survey: unbiased survey of dense cores and core mass functions in Orion A
|
Nov 21, 2022 |
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Hydrodynamical Simulations of Black-Hole Binary Formation in AGN Disks
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Nov 21, 2022 |
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How dark the sky: the JWST backgrounds
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Nov 21, 2022 |
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Recovery of Phosphine in Venus' Atmosphere from SOFIA Observations
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Nov 21, 2022 |
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Unstable Mass Transfer from a Main-Sequence Star to a Supermassive Black Hole and Quasi-Periodic Eruptions
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Nov 21, 2022 |
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Discrete Absorption Components from 3-D spot models of hot star winds
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Nov 21, 2022 |
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Astrometric Accelerations as Dynamical Beacons: Discovery and Characterization of HIP 21152 B, the First T-Dwarf Companion in the Hyades
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Nov 21, 2022 |
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JWST NIRCam Probes Young Star Clusters in the Reionization Era Sunrise Arc
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Nov 21, 2022 |
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Two decades of optical timing of the shortest-period binary star system HM Cancri
|
Nov 21, 2022 |
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Local gravitational instability of stratified rotating fluids: 3D criteria for gaseous discs
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Nov 21, 2022 |
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Detecting planetary mass companions near the water frost-line using JWST interferometry
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Nov 21, 2022 |
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A new catalogue of solar flare events from soft x-ray GOES signal in the period 1986-2020
|
Nov 21, 2022 |
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Surviving in Ocean Worlds: Experimental Characterization of Fiber Optic Tethers across Europa-like Ice Faults and Unraveling the Sliding Behavior of Ice
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Nov 21, 2022 |
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Compact jets dominate the continuum emission in low-luminosity active galactic nuclei
|
Nov 21, 2022 |
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An investigation of open clusters Berkeley 68 and Stock 20 using CCD UBV and Gaia DR3 data
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Nov 21, 2022 |
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Line Emission Mapper LEM : Probing physics of cosmic ecosystems
|
Nov 21, 2022 |
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When Does Gyrochronology Start to Work? Stellar Rotation and Structure of the α Persei Complex
|
Nov 21, 2022 |
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Mapping Tropical Forest Cover and Deforestation with Planet NICFI Satellite Images and Deep Learning in Mato Grosso State Brazil from 2015 to 2021
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Nov 21, 2022 |
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Mind the gap: The discrepancy between simulation and reality drives interpretations of the Galactic Center Excess
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Nov 21, 2022 |
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Radiometric sensitivity and resolution of synthetic tracking imaging for orbital debris monitoring
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Nov 21, 2022 |
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A Census of the Taurus Star-forming Region and Neighboring Associations with Gaia
|
Nov 21, 2022 |
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A strong H- opacity signal in the near-infrared emission spectrum of the ultra-hot Jupiter KELT-9b
|
Nov 21, 2022 |
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Void Lensing in Cubic Galileon Gravity
|
Nov 21, 2022 |
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A unified model for the co-evolution of galaxies and their circumgalactic medium: the relative roles of turbulence and atomic cooling physics
|
Nov 21, 2022 |
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As a matter of dynamical range -- scale dependent energy dynamics in MHD turbulence
|
Nov 21, 2022 |
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Exploring Earth's Ionosphere and its effect on low radio frequency observation with the uGMRT and the SKA
|
Nov 21, 2022 |
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The origin of star-forming rings in S0 galaxies
|
Nov 21, 2022 |
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Mock Galaxy Surveys for HST and JWST from the IllustrisTNG Simulations
|
Nov 21, 2022 |
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On the evaluation of solar wind's heating rates
|
Nov 21, 2022 |
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Computing First-Passage Times with the Functional Renormalisation Group
|
Nov 21, 2022 |
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The role of the magnetic fields in GRB outflows
|
Nov 21, 2022 |
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Growing evidence for high-energy neutrinos originating in radio blazars
|
Nov 21, 2022 |
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A Detailed Look at the Most Obscured Galactic Nuclei in the Mid-Infrared
|
Nov 21, 2022 |
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Radiation from Global Topological Strings using Adaptive Mesh Refinement: Massive Modes
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Nov 21, 2022 |
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Understanding the role of morphology and environment on the dynamical evolution of isolated galaxy triplets
|
Nov 21, 2022 |
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High-resolution atmospheric retrievals of WASP-121b transmission spectroscopy with ESPRESSO: Consistent relative abundance constraints across multiple epochs and instruments
|
Nov 21, 2022 |
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Detecting deviations from Gaussianity in high-redshift CMB lensing maps
|
Nov 21, 2022 |
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Deep Learning-based galaxy image deconvolution
|
Nov 21, 2022 |
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Linking the Internal Properties of Infant Globular Clusters to their Formation Environments
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Nov 21, 2022 |
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Global MHD simulations of the solar convective zone using a volleyball mesh decomposition I Pilot
|
Nov 21, 2022 |
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Asgard NOTT: L-band nulling interferometry at the VLTI I Simulating the expected high-contrast performance
|
Nov 21, 2022 |
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The hard to soft transition of GX 339-4 as seen by Insight-HXMT
|
Nov 21, 2022 |
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Locating Hidden Exoplanets in ALMA Data Using Machine Learning
|
Nov 21, 2022 |
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Spectral properties of the Be X-ray pulsar 2S 1553-542 during Type II outbursts
|
Nov 21, 2022 |
|
MeV-GeV Gamma-ray Emission from SNR G327 1-1 1 Discovered by the Fermi-LAT
|
Nov 21, 2022 |
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Variability In A Low-Mass AGN: Oscillation Or Eruption?
|
Nov 21, 2022 |
|
Growing Black Holes through Successive Mergers in Galactic Nuclei: I Methods and First Results
|
Nov 21, 2022 |
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Chandra measurements of gas homogeneity and turbulence at intermediate radii in the Perseus Cluster
|
Nov 21, 2022 |
|
StarDICE I: sensor calibration bench and absolute photometric calibration of a Sony IMX411 sensor
|
Nov 21, 2022 |
|
i cm z , a semi-analytic model for the thermodynamic properties in galaxy clusters: calibrations with mass and redshift, and implication for the hydrostatic bias
|
Nov 21, 2022 |
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Neutrinos from the Brightest Gamma-Ray Burst?
|
Nov 21, 2022 |
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Non-synchronous rotation on Europa driven by ocean currents
|
Nov 21, 2022 |
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Machine learning constraints on deviations from general relativity from the large scale structure of the Universe
|
Nov 21, 2022 |
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The mass-radius relation of intermediate-mass planets outlined by hydrodynamic escape and thermal evolution
|
Nov 21, 2022 |
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Evolution of Cosmic Voids in the Schrodinger-Poisson Formalism
|
Nov 21, 2022 |
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Decomposition of galactic X-ray emission with Phox: Contributions from hot gas and XRBs
|
Nov 21, 2022 |
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DEMNUni: comparing nonlinear power spectra prescriptions in the presence of massive neutrinos and dynamical dark energy
|
Nov 21, 2022 |
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A measure of cosmological distance using the civ Baldwin effect in quasars
|
Nov 21, 2022 |
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Three-dimensional numerical simulations of structured GRB jets
|
Nov 21, 2022 |
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Low-Energy Electron-Track Imaging for a Liquid Argon Time-Projection-Chamber Telescope Concept using Probabilistic Deep Learning
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Nov 21, 2022 |