Astro arXiv | astro-ph.GA and astro-ph.CO
By Corentin Cadiou
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Episodes: 594
Description
Daily Astro papers on the arXiv in astro-ph.GA and astro-ph.CO.
| Episode | Date |
|---|---|
|
Extreme nature of four blue-excess dust-obscured galaxies revealed by optical spectroscopy
|
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 |
|
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 |
|
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 |
|
Microlensing of gravitational waves by dark matter structures
|
Nov 30, 2022 |
|
Real-world CMB lensing quadratic estimator power spectrum response
|
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 |
|
High- z Quasar Candidate Archive: A Spectroscopic Catalog of Quasars and Contaminants in Various Quasar Searches
|
Nov 30, 2022 |
|
Insights on the origin of ORCs from cosmological simulations
|
Nov 30, 2022 |
|
Large-scale geometry of the Universe
|
Nov 30, 2022 |
|
NGC 7538 IRS2 in NeII : Shell and Cavity Kinematics of a Compact HII Region
|
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 |
|
RSD measurements from BOSS galaxy power spectrum using the halo perturbation theory model
|
Nov 30, 2022 |
|
Extreme nature of four blue-excess dust-obscured galaxies revealed by optical spectroscopy
|
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 |
|
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 |
|
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 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 |
|
The AstroSat UV Deep Field North: the far and near ultraviolet photometric catalog
|
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 |
|
Microlensing of gravitational waves by dark matter structures
|
Nov 30, 2022 |
|
Real-world CMB lensing quadratic estimator power spectrum response
|
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 |
|
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 |
|
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 |
|
Evidence for a Massive Andromeda Galaxy Using Satellite Galaxy Proper Motions
|
Nov 30, 2022 |
|
The CMB cold spot under the lens: ruling out a supervoid interpretation
|
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 |
|
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 |
|
The XQR-30 Metal Absorber Catalog: 778 Absorption Systems Spanning 2 < z < 6 5
|
Nov 30, 2022 |
|
Calibrating cosmological simulations with implicit likelihood inference using galaxy growth observables
|
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 |
|
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 |
|
The mid-infrared molecular inventory towards Orion IRc2
|
Nov 30, 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 30, 2022 |
|
Toward Accurate Modeling of Galaxy Clustering on Small Scales: Halo Model Extensions & Lingering Tension
|
Nov 30, 2022 |
|
PHANGS-JWST First Results: Duration of the early phase of massive star formation in NGC628
|
Nov 30, 2022 |
|
Disturbed, diffuse, or just missing? A global study of the HI content of Hickson Compact Groups
|
Nov 30, 2022 |
|
Neural networks: solving the chemistry of the interstellar medium
|
Nov 30, 2022 |
|
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 |
|
X-ray Absorption Lines in the Warm-Hot Intergalactic Medium: Probing Chandra observations with the CAMEL simulations
|
Nov 30, 2022 |
|
Sensitivity of strong lensing observations to dark matter substructure: a case study with Euclid
|
Nov 30, 2022 |
|
Statistical Study of the Star Formation Efficiency in Bars: Is Star Formation Suppressed in Gas-Rich Bars?
|
Nov 30, 2022 |
|
Separating the blue cloud and the red sequence using Otsu's method for image segmentation
|
Nov 30, 2022 |
|
Bar formation in submaximal disks: a challenge for Λ CDM
|
Nov 30, 2022 |
|
Observational studies of high-mass star formation
|
Nov 30, 2022 |
|
Palatini formulation for gauge theory: implications for slow-roll inflation
|
Nov 30, 2022 |
|
Assessing the physical reality of Milky Way open cluster candidates
|
Nov 30, 2022 |
|
SILCC VII -- Gas kinematics and multiphase outflows of the simulated ISM at high gas surface densities
|
Nov 30, 2022 |
|
Free-form reconstruction of primordial power spectrum using Planck CMB temperature and polarization
|
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 |
|
A bias-free cosmological analysis with quasars alleviating H 0 tension
|
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 |
|
Galaxy And Mass Assembly GAMA : The Dependence of Star Formation on Surface Brightness in Low Redshift Galaxies
|
Nov 29, 2022 |
|
Evidence for a Massive Andromeda Galaxy Using Satellite Galaxy Proper Motions
|
Nov 29, 2022 |
|
The CMB cold spot under the lens: ruling out a supervoid interpretation
|
Nov 29, 2022 |
|
Latest data constraint of some parameterized dark energy models
|
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 |
|
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 |
|
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 |
|
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 |
|
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 |
|
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 |
|
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 |
|
Assessing the physical reality of Milky Way open cluster candidates
|
Nov 29, 2022 |
|
SILCC VII -- Gas kinematics and multiphase outflows of the simulated ISM at high gas surface densities
|
Nov 29, 2022 |
|
Free-form reconstruction of primordial power spectrum using Planck CMB temperature and polarization
|
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 |
|
A bias-free cosmological analysis with quasars alleviating H 0 tension
|
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 |
|
Assessing the physical reality of Milky Way open cluster candidates
|
Nov 29, 2022 |
|
SILCC VII -- Gas kinematics and multiphase outflows of the simulated ISM at high gas surface densities
|
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 |
|
A bias-free cosmological analysis with quasars alleviating H 0 tension
|
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 |
|
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 |
|
WALLABY Pilot Survey: HI gas kinematics of galaxy pairs in cluster environment
|
Nov 29, 2022 |
|
Near-inflection point inflation and production of dark matter during reheating
|
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 |
|
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 |
|
The effect of saturated thermal conduction on clouds in a hot plasma
|
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 |
|
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 |
|
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 |
|
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 |
|
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 |
|
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 |
|
Reducing the Impact of Weak-lensing Errors on Gravitational-wave Standard Sirens
|
Nov 29, 2022 |
|
Machine learning cosmic inflation
|
Nov 29, 2022 |
|
The uncertain interstellar medium of high-redshift quiescent galaxies: Impact of methodology
|
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 |
|
On the Kinematic Morphology around Halos
|
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 |
|
Scalar Weak Gravity Conjecture in Super Yang-Mills Inflationary Model
|
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 |
|
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 |
|
WALLABY Pilot Survey: HI gas kinematics of galaxy pairs in cluster environment
|
Nov 28, 2022 |
|
Near-inflection point inflation and production of dark matter during reheating
|
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 |
|
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 |
|
The effect of saturated thermal conduction on clouds in a hot plasma
|
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 |
|
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 |
|
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 |
|
The Pristine Inner Galaxy Survey PIGS VI: Different vertical distributions between two DIBs at 442 8 nm and 862 1 nm
|
Nov 28, 2022 |
|
Constraining dark matter decays with cosmic microwave background and weak lensing shear observations
|
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 |
|
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 |
|
Reducing the Impact of Weak-lensing Errors on Gravitational-wave Standard Sirens
|
Nov 28, 2022 |
|
Machine learning cosmic inflation
|
Nov 28, 2022 |
|
The uncertain interstellar medium of high-redshift quiescent galaxies: Impact of methodology
|
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 |
|
On the Kinematic Morphology around Halos
|
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 |
|
Scalar Weak Gravity Conjecture in Super Yang-Mills Inflationary Model
|
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 |
|
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 |
|
A Sample of Dust Attenuation Laws for DES Supernova Host Galaxies
|
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 uncertain interstellar medium of high-redshift quiescent galaxies: Impact of methodology
|
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 |
|
The eROSITA Final Equatorial-Depth Survey eFEDS : X-ray properties of Subaru optically-selected clusters
|
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 |
|
A global view on star formation: The GLOSTAR Galactic plane survey VII Supernova remnants in the Galactic longitude range 28^ circ
|
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 |
|
MOSEL Survey: Extremely weak outflows in EoR analogues at z=3-4
|
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 |
|
Hybrid α -attractors, primordial black holes and gravitational wave backgrounds
|
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 |
|
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 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 |
|
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 |
|
Significance Mode Analysis SigMA for hierarchical structures An application to the Sco-Cen OB association
|
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 |
|
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 |
|
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 |
|
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 |
|
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 |
|
A global view on star formation: The GLOSTAR Galactic plane survey VII Supernova remnants in the Galactic longitude range 28^ circ
|
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 |
|
MOSEL Survey: Extremely weak outflows in EoR analogues at z=3-4
|
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 |
|
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 |
|
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 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 |
|
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 |
|
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 |
|
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 |
|
iMaNGA: mock MaNGA galaxies based on IllustrisTNG-50 and MaStar SSPs II the catalogue
|
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 |
|
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 |
|
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 |
|
Nuclear Activity in the Low Metallicity Dwarf Galaxy SDSS J0944-0038: A Glimpse into the Primordial Universe
|
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 |
|
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 |
|
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 |
|
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 |
|
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 |
|
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 |
|
Identifying and Characterizing the Most Heavily Dust-Obscured Galaxies at 1 le z le 4
|
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 production of ionizing photons in UV-faint z~3-7 galaxies
|
Nov 24, 2022 |
|
EAVN Astrometry toward the Extreme Outer Galaxy: Kinematic distance with the proper motion of G034 84-00 95
|
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 |
|
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 |
|
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 |
|
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 |
|
ALMA Fragmented Source Catalogue in Orion FraSCO I Outflow interaction within an embedded cluster in OMC-2 FIR3, FIR4, and FIR5
|
Nov 24, 2022 |
|
Cosmic Topology I: Limits on Orientable Euclidean Manifolds from Circle Searches
|
Nov 24, 2022 |
|
The structure at the centre of the giant radio galaxy GRS J0844+4627: a compact symmetric object?
|
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 |
|
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 |
|
How Close Dark Matter Halos and MOND Are to Each Other: Three-Dimensional Tests Based on Gaia DR2
|
Nov 24, 2022 |
|
Constraints on Yukawa gravity parameters from observations of bright stars
|
Nov 23, 2022 |
|
First estimate of the local value of the baryonic streaming velocity
|
Nov 23, 2022 |
|
One-loop tensor power spectrum from an excited scalar field during inflation
|
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 |
|
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 |
|
Identifying and Characterizing the Most Heavily Dust-Obscured Galaxies at 1 le z le 4
|
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 production of ionizing photons in UV-faint z~3-7 galaxies
|
Nov 23, 2022 |
|
EAVN Astrometry toward the Extreme Outer Galaxy: Kinematic distance with the proper motion of G034 84-00 95
|
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 |
|
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 |
|
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 |
|
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 |
|
ALMA Fragmented Source Catalogue in Orion FraSCO I Outflow interaction within an embedded cluster in OMC-2 FIR3, FIR4, and FIR5
|
Nov 23, 2022 |
|
Cosmic Topology I: Limits on Orientable Euclidean Manifolds from Circle Searches
|
Nov 23, 2022 |
|
The structure at the centre of the giant radio galaxy GRS J0844+4627: a compact symmetric object?
|
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 |
|
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 |
|
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 |
|
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 |
|
Cosmic Topology I: Limits on Orientable Euclidean Manifolds from Circle Searches
|
Nov 23, 2022 |
|
The structure at the centre of the giant radio galaxy GRS J0844+4627: a compact symmetric object?
|
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 |
|
Short GRB Host Galaxies II A Legacy Sample of Redshifts, Stellar Population Properties, and Implications for their Neutron Star Merger Origins
|
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 |
|
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 |
|
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 |
|
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 |
|
Active galactic nucleus jet feedback in hydrostatic halos
|
Nov 23, 2022 |
|
GalaxyFlow: Upsampling Hydrodynamical Simulations for Realistic Gaia Mock Catalogs
|
Nov 23, 2022 |
|
Consistent and simultaneous modelling of galaxy clustering and galaxy-galaxy lensing with Subhalo Abundance Matching
|
Nov 23, 2022 |
|
Predicting sub-millimeter flux densities from global galaxy properties
|
Nov 23, 2022 |
|
Investigating the Evolution of Amati Parameters with Redshift
|
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 |
|
A General Bayesian Framework to Account for Foreground Map Errors in Global 21-cm Experiments
|
Nov 23, 2022 |
|
Non-perturbative non-Gaussianity and primordial black holes
|
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 |
|
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 |
|
A new resonance-like feature in the outer disc of the Milky Way
|
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 |
|
Dust-free starburst galaxies at redshifts z>10
|
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 |
|
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 |
|
Witnessing a Galaxy Cluster Merger with JWST and a Chandra X-ray Temperature Map
|
Nov 22, 2022 |
|
Primordial black holes from D-parity breaking in SO 10 grand unified theory
|
Nov 22, 2022 |
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King Ghidorah Supercluster: Mapping the light and dark matter in a new supercluster at z=0 55 using the Subaru Hyper Suprime-Cam
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Nov 22, 2022 |
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Rarefied Broad-Line Regions in Active Galactic Nuclei: Anomalous Responses in Reverberation Mapping and Implications for Weak-Emission Line Quasars
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Nov 22, 2022 |
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Second order scalar perturbations induced by primordial curvature and tensor perturbations
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Nov 22, 2022 |
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Mesh-free hydrodynamics in PKDGRAV3 for galaxy formation simulations
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Nov 22, 2022 |
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CLASS Survey Description: Coronal Line Needles in the SDSS Haystack
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Nov 22, 2022 |
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The Statistics of Negative Power Spectrum Systematics in some 21 cm Analyses
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Nov 22, 2022 |
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Unsupervised classification reveals new evolutionary pathways
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Nov 22, 2022 |
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MaNGIA: 10,000 mock galaxies for stellar population analysis
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Nov 22, 2022 |
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Modelling the accretion and feedback of supermassive black hole binaries in gas-rich galaxy mergers
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Nov 22, 2022 |
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MeerKAT follow-up of enigmatic GLEAM 4-Jy G4Jy sources
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Nov 22, 2022 |
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Reconstructing and Classifying SDSS DR16 Galaxy Spectra with Machine-Learning and Dimensionality Reduction Algorithms
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Nov 22, 2022 |
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Quasar Factor Analysis -- An Unsupervised and Probabilistic Quasar Continuum Prediction Algorithm with Latent Factor Analysis
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Nov 22, 2022 |
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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
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Nov 22, 2022 |
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Active galactic nucleus jet feedback in hydrostatic halos
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Nov 22, 2022 |
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GalaxyFlow: Upsampling Hydrodynamical Simulations for Realistic Gaia Mock Catalogs
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Nov 22, 2022 |
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Consistent and simultaneous modelling of galaxy clustering and galaxy-galaxy lensing with Subhalo Abundance Matching
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Nov 22, 2022 |
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Predicting sub-millimeter flux densities from global galaxy properties
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Nov 22, 2022 |
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Investigating the Evolution of Amati Parameters with Redshift
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Nov 22, 2022 |
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Bose-Einstein Condensate Dark Matter That Involves Composites
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Nov 22, 2022 |
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Cosmography using strongly lensed gravitational waves from binary black holes
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Nov 22, 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 22, 2022 |
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Non-perturbative non-Gaussianity and primordial black holes
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Nov 22, 2022 |
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If dark matter is fuzzy, the first stars form in massive pancakes
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Nov 22, 2022 |
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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
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Nov 22, 2022 |
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A Milliarcsecond-accurate Position for Sagittarius A*
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Nov 22, 2022 |
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Radio Emission of Nearby Early-type Galaxies at Low and Very-Low Radio Luminosity Range
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Nov 22, 2022 |
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Mapping NGC 7027 in New Light: CO ^+ and HCO ^+ Emission Reveal Its Photon- and X-ray-Dominated Regions
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Nov 22, 2022 |
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Etherington duality breaking: gravitational lensing in non-metric spacetimes versus intrinsic alignments
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Nov 22, 2022 |
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Reconstructing the Assembly of Massive Galaxies II Galaxies Develop Massive and Dense Stellar Cores as They Evolve and Head Toward Quiescence at Cosmic Noon
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Nov 22, 2022 |
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A new resonance-like feature in the outer disc of the Milky Way
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Nov 22, 2022 |
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Dark matter halos and scaling relations of extremely massive spiral galaxies from extended HI rotation curves
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Nov 22, 2022 |
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Redshift requirements for cosmic shear with intrinsic alignment
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Nov 22, 2022 |
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Characterization and dynamics of the peculiar stream Jhelum, A tentative role for the Sagittarius dwarf galaxy
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Nov 22, 2022 |
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Properties beyond mass for unresolved haloes across redshift and cosmology using correlations with local halo environment
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Nov 22, 2022 |
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Consistent and simultaneous modelling of galaxy clustering and galaxy-galaxy lensing with Subhalo Abundance Matching
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Nov 22, 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 22, 2022 |
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Peering into the Milky Way by FAST: IV Identification of two new Galactic supernova remnants G203 1+6 6 and G206 7+5 9
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Nov 22, 2022 |
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Sudden braking and turning in the single multi-stream inflation: primordial black hole formation
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Nov 22, 2022 |
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If dark matter is fuzzy, the first stars form in massive pancakes
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Nov 22, 2022 |
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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
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Nov 22, 2022 |
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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
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Nov 22, 2022 |
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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
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Nov 22, 2022 |
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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
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Nov 22, 2022 |
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Radio Emission of Nearby Early-type Galaxies at Low and Very-Low Radio Luminosity Range
|
Nov 22, 2022 |
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Dark matter halos and scaling relations of extremely massive spiral galaxies from extended HI rotation curves
|
Nov 22, 2022 |
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Exhaustive Symbolic Regression
|
Nov 22, 2022 |
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Predicting sub-millimeter flux densities from global galaxy properties
|
Nov 22, 2022 |
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IWDM: The fate of an interacting non-cold dark matter - vacuum scenario
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Nov 22, 2022 |
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Dusty plasma in active galactic nuclei
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Nov 22, 2022 |
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Unidentified infrared bands do not correlate with C O ratio in planetary nebulae
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Nov 22, 2022 |
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A bias-free cosmological analysis with quasars alleviating H 0 tension
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Nov 22, 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 22, 2022 |
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DESI Mock Challenge VII: halo and galaxy catalogs with the Bias Assignment Method
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Nov 22, 2022 |
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Velocity-Coherent Substructure in TMC-1: Inflow and Fragmentation
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Nov 22, 2022 |
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Starlet higher order statistics for galaxy clustering and weak lensing
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Nov 22, 2022 |
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Investigating the Evolution of Amati Parameters with Redshift
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Nov 22, 2022 |
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Kinetically stabilized inflation
|
Nov 22, 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
|
Nov 22, 2022 |
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A simple spectroscopic technique to identify rejuvenating galaxies
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Nov 22, 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 22, 2022 |
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Investigating dark energy by electromagnetic frequency shifts II: the Pantheon+ sample
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Nov 22, 2022 |
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Understanding the role of morphology and environment on the dynamical evolution of isolated galaxy triplets
|
Nov 22, 2022 |
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CARMA-NRO Orion Survey: unbiased survey of dense cores and core mass functions in Orion A
|
Nov 22, 2022 |
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Bose-Einstein Condensate Dark Matter That Involves Composites
|
Nov 22, 2022 |
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The microvariability and wavelength dependence of polarization degree angle of BL Lacertae in the outburst 2020 to 2021
|
Nov 22, 2022 |
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Dusty winds clear JWST super-early galaxies
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Nov 22, 2022 |
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i-SPin: An integrator for multicomponent Schrödinger-Poisson systems with self-interactions
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Nov 22, 2022 |
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The galaxy formation origin of the lensing is low problem
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Nov 22, 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 22, 2022 |
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A ~200 pc-sized core of Milky Way dark matter halo constrained from the OGLE micro-lensing sky map
|
Nov 22, 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 22, 2022 |
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Accuracy and precision of triaxial orbit models II: Viewing angles, shape and orbital structure
|
Nov 22, 2022 |
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Large Field Polynomial Inflation: Parameter Space, Predictions and Double Eternal Nature
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Nov 22, 2022 |
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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 |
|
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 |
|
Exhaustive Symbolic Regression
|
Nov 21, 2022 |
|
IWDM: The fate of an interacting non-cold dark matter - vacuum scenario
|
Nov 21, 2022 |
|
Dusty plasma in active galactic nuclei
|
Nov 21, 2022 |
|
Unidentified infrared bands do not correlate with C O ratio in planetary nebulae
|
Nov 21, 2022 |
|
A bias-free cosmological analysis with quasars alleviating H 0 tension
|
Nov 21, 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 21, 2022 |
|
DESI Mock Challenge VII: halo and galaxy catalogs with the Bias Assignment Method
|
Nov 21, 2022 |
|
Velocity-Coherent Substructure in TMC-1: Inflow and Fragmentation
|
Nov 21, 2022 |
|
Starlet higher order statistics for galaxy clustering and weak lensing
|
Nov 21, 2022 |
|
Kinetically stabilized inflation
|
Nov 21, 2022 |
|
The Molecular-Gas Main Sequence and Schmidt-Kennicutt relation are fundamental, the Star-Forming Main Sequence is a useful byproduct
|
Nov 21, 2022 |
|
A simple spectroscopic technique to identify rejuvenating galaxies
|
Nov 21, 2022 |
|
A General Bayesian Framework to Account for Foreground Map Errors in Global 21-cm Experiments
|
Nov 21, 2022 |
|
Investigating dark energy by electromagnetic frequency shifts II: the Pantheon+ sample
|
Nov 21, 2022 |
|
Understanding the role of morphology and environment on the dynamical evolution of isolated galaxy triplets
|
Nov 21, 2022 |
|
CARMA-NRO Orion Survey: unbiased survey of dense cores and core mass functions in Orion A
|
Nov 21, 2022 |
|
The microvariability and wavelength dependence of polarization degree angle of BL Lacertae in the outburst 2020 to 2021
|
Nov 21, 2022 |
|
Dusty winds clear JWST super-early galaxies
|
Nov 21, 2022 |
|
i-SPin: An integrator for multicomponent Schrödinger-Poisson systems with self-interactions
|
Nov 21, 2022 |
|
The galaxy formation origin of the lensing is low problem
|
Nov 21, 2022 |
|
Diversity of dust properties in external galaxies confirmed by polarization signals from Type II supernovae
|
Nov 21, 2022 |
|
A ~200 pc-sized core of Milky Way dark matter halo constrained from the OGLE micro-lensing sky map
|
Nov 21, 2022 |
|
How to Interpret Measurements of Diffuse Light in Stacked Observations of Groups and Clusters of Galaxies
|
Nov 21, 2022 |
|
Accuracy and precision of triaxial orbit models II: Viewing angles, shape and orbital structure
|
Nov 21, 2022 |
|
Large Field Polynomial Inflation: Parameter Space, Predictions and Double Eternal Nature
|
Nov 21, 2022 |
|
Simulations of PBH formation at the QCD epoch and comparison with the GWTC-3 catalog
|
Nov 21, 2022 |
|
Dark dust II: Properties in the general field of the diffuse ISM
|
Nov 21, 2022 |
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Primordial black holes induced stochastic axion-photon oscillations in primordial magnetic field
|
Nov 21, 2022 |
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Is the core-cusp problem a matter of perspective: Jeans Anisotropic Modeling against numerical simulations
|
Nov 21, 2022 |
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Prospects for constraining interacting dark energy models from gravitational wave and gamma ray burst joint observation
|
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
|
Nov 21, 2022 |
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Spectral Templates Optimal for Selecting Galaxies at z > 8 with JWST
|
Nov 21, 2022 |
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Evolution of grain size distribution with enhanced abundance of small carbonaceous grains in galactic environments
|
Nov 21, 2022 |
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Effects of Active Galactic Nucleus Feedback on Cold Gas Depletion and Quenching of Central Galaxies
|
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
|
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 |
|
JWST NIRCam Probes Young Star Clusters in the Reionization Era Sunrise Arc
|
Nov 21, 2022 |
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Local gravitational instability of stratified rotating fluids: 3D criteria for gaseous discs
|
Nov 21, 2022 |
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An investigation of open clusters Berkeley 68 and Stock 20 using CCD UBV and Gaia DR3 data
|
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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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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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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Computing First-Passage Times with the Functional Renormalisation Group
|
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
|
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 |
|
Detecting deviations from Gaussianity in high-redshift CMB lensing maps
|
Nov 21, 2022 |
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Linking the Internal Properties of Infant Globular Clusters to their Formation Environments
|
Nov 21, 2022 |
|
Growing Black Holes through Successive Mergers in Galactic Nuclei: I Methods and First Results
|
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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Machine learning constraints on deviations from general relativity from the large scale structure of the Universe
|
Nov 21, 2022 |
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Evolution of Cosmic Voids in the Schrodinger-Poisson Formalism
|
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 |