Astro arXiv | astro-ph.GA and astro-ph.CO

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Daily Astro papers on the arXiv in astro-ph.GA and astro-ph.CO.

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Recent Episodes
  • Large Field Polynomial Inflation: Parameter Space, Predictions and Double Eternal Nature
    Nov 21, 2022 – 01:02
  • Accuracy and precision of triaxial orbit models II: Viewing angles, shape and orbital structure
    Nov 21, 2022 – 00:56
  • A measure of cosmological distance using the civ Baldwin effect in quasars
    Nov 21, 2022 – 00:21
  • DEMNUni: comparing nonlinear power spectra prescriptions in the presence of massive neutrinos and dynamical dark energy
    Nov 21, 2022 – 01:10
  • How to Interpret Measurements of Diffuse Light in Stacked Observations of Groups and Clusters of Galaxies
    Nov 21, 2022 – 00:53
  • Evolution of Cosmic Voids in the Schrodinger-Poisson Formalism
    Nov 21, 2022 – 00:29
  • A ~200 pc-sized core of Milky Way dark matter halo constrained from the OGLE micro-lensing sky map
    Nov 21, 2022 – 00:37
  • Diversity of dust properties in external galaxies confirmed by polarization signals from Type II supernovae
    Nov 21, 2022 – 01:00
  • The galaxy formation origin of the lensing is low problem
    Nov 21, 2022 – 00:31
  • Machine learning constraints on deviations from general relativity from the large scale structure of the Universe
    Nov 21, 2022 – 00:55
  • 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 – 01:16
  • i-SPin: An integrator for multicomponent Schrödinger-Poisson systems with self-interactions
    Nov 21, 2022 – 00:34
  • Dusty winds clear JWST super-early galaxies
    Nov 21, 2022 – 00:27
  • The microvariability and wavelength dependence of polarization degree angle of BL Lacertae in the outburst 2020 to 2021
    Nov 21, 2022 – 00:44
  • Growing Black Holes through Successive Mergers in Galactic Nuclei: I Methods and First Results
    Nov 21, 2022 – 01:03
  • CARMA-NRO Orion Survey: unbiased survey of dense cores and core mass functions in Orion A
    Nov 21, 2022 – 01:09
  • Understanding the role of morphology and environment on the dynamical evolution of isolated galaxy triplets
    Nov 21, 2022 – 01:08
  • Linking the Internal Properties of Infant Globular Clusters to their Formation Environments
    Nov 21, 2022 – 00:46
  • Detecting deviations from Gaussianity in high-redshift CMB lensing maps
    Nov 21, 2022 – 00:31
  • Understanding the role of morphology and environment on the dynamical evolution of isolated galaxy triplets
    Nov 21, 2022 – 01:12
  • Radiation from Global Topological Strings using Adaptive Mesh Refinement: Massive Modes
    Nov 21, 2022 – 00:37
  • Investigating dark energy by electromagnetic frequency shifts II: the Pantheon+ sample
    Nov 21, 2022 – 00:34
  • A General Bayesian Framework to Account for Foreground Map Errors in Global 21-cm Experiments
    Nov 21, 2022 – 00:50
  • A Detailed Look at the Most Obscured Galactic Nuclei in the Mid-Infrared
    Nov 21, 2022 – 00:53
  • A simple spectroscopic technique to identify rejuvenating galaxies
    Nov 21, 2022 – 00:13
  • The Molecular-Gas Main Sequence and Schmidt-Kennicutt relation are fundamental, the Star-Forming Main Sequence is a useful byproduct
    Nov 21, 2022 – 00:51
  • Computing First-Passage Times with the Functional Renormalisation Group
    Nov 21, 2022 – 00:46
  • Mock Galaxy Surveys for HST and JWST from the IllustrisTNG Simulations
    Nov 21, 2022 – 00:45
  • The origin of star-forming rings in S0 galaxies
    Nov 21, 2022 – 00:59
  • As a matter of dynamical range -- scale dependent energy dynamics in MHD turbulence
    Nov 21, 2022 – 01:00
  • 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 – 00:55
  • Void Lensing in Cubic Galileon Gravity
    Nov 21, 2022 – 00:47
  • Kinetically stabilized inflation
    Nov 21, 2022 – 00:22
  • A Census of the Taurus Star-forming Region and Neighboring Associations with Gaia
    Nov 21, 2022 – 00:57
  • Starlet higher order statistics for galaxy clustering and weak lensing
    Nov 21, 2022 – 00:45
  • Velocity-Coherent Substructure in TMC-1: Inflow and Fragmentation
    Nov 21, 2022 – 00:54
  • An investigation of open clusters Berkeley 68 and Stock 20 using CCD UBV and Gaia DR3 data
    Nov 21, 2022 – 01:21
  • Local gravitational instability of stratified rotating fluids: 3D criteria for gaseous discs
    Nov 21, 2022 – 00:39
  • DESI Mock Challenge VII: halo and galaxy catalogs with the Bias Assignment Method
    Nov 21, 2022 – 00:41
  • 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 – 01:19
  • JWST NIRCam Probes Young Star Clusters in the Reionization Era Sunrise Arc
    Nov 21, 2022 – 00:40
  • A bias-free cosmological analysis with quasars alleviating H 0 tension
    Nov 21, 2022 – 01:01
  • CARMA-NRO Orion Survey: unbiased survey of dense cores and core mass functions in Orion A
    Nov 21, 2022 – 00:54
  • Sub-kpc radio jets in the brightest central galaxy of the cool-core galaxy cluster RXJ1720 1+2638
    Nov 21, 2022 – 00:37
  • Unidentified infrared bands do not correlate with C O ratio in planetary nebulae
    Nov 21, 2022 – 00:33
  • Effects of Active Galactic Nucleus Feedback on Cold Gas Depletion and Quenching of Central Galaxies
    Nov 21, 2022 – 00:56
  • Dusty plasma in active galactic nuclei
    Nov 21, 2022 – 00:21
  • IWDM: The fate of an interacting non-cold dark matter - vacuum scenario
    Nov 21, 2022 – 00:40
  • Evolution of grain size distribution with enhanced abundance of small carbonaceous grains in galactic environments
    Nov 21, 2022 – 00:54
  • Exhaustive Symbolic Regression
    Nov 21, 2022 – 00:47
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