Astro arXiv | all categories

Daily Astro papers on the arXiv in all categories.

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Recent Episodes
  • Low-Energy Electron-Track Imaging for a Liquid Argon Time-Projection-Chamber Telescope Concept using Probabilistic Deep Learning
    Nov 21, 2022 – 00:57
  • Large Field Polynomial Inflation: Parameter Space, Predictions and Double Eternal Nature
    Nov 21, 2022 – 01:02
  • Three-dimensional numerical simulations of structured GRB jets
    Nov 21, 2022 – 00:44
  • Impact of Rastall gravity on mass, radius and sound speed of the pulsar PSR J0740+6620
    Nov 21, 2022 – 01:18
  • 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
  • Temporal evolution and rigidity dependence of the solar modulation lag of Galactic cosmic rays
    Nov 21, 2022 – 00:43
  • Decomposition of galactic X-ray emission with Phox: Contributions from hot gas and XRBs
    Nov 21, 2022 – 01:03
  • How to Interpret Measurements of Diffuse Light in Stacked Observations of Groups and Clusters of Galaxies
    Nov 21, 2022 – 00:53
  • Interpreting molecular hydrogen and atomic oxygen line emission of T Tauri disks with photoevaporative disk-wind models
    Nov 21, 2022 – 01:07
  • Evolution of Cosmic Voids in the Schrodinger-Poisson Formalism
    Nov 21, 2022 – 00:29
  • GRaM-X: A new GPU-accelerated dynamical spacetime GRMHD code for Exascale computing with the Einstein Toolkit
    Nov 21, 2022 – 01:00
  • A ~200 pc-sized core of Milky Way dark matter halo constrained from the OGLE micro-lensing sky map
    Nov 21, 2022 – 00:37
  • The mass-radius relation of intermediate-mass planets outlined by hydrodynamic escape and thermal evolution
    Nov 21, 2022 – 00:13
  • 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
  • Non-synchronous rotation on Europa driven by ocean currents
    Nov 21, 2022 – 00:38
  • The unaltered pulsar: GRO J1750-27, a super-critical X-ray neutron star that does not blink an eye
    Nov 21, 2022 – 01:08
  • Neutrinos from the Brightest Gamma-Ray Burst?
    Nov 21, 2022 – 00:32
  • 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
  • Saturn's Seasonal Variability from Four Decades of Ground-Based Mid-Infrared Observations
    Nov 21, 2022 – 01:00
  • StarDICE I: sensor calibration bench and absolute photometric calibration of a Sony IMX411 sensor
    Nov 21, 2022 – 01:13
  • Eccentricity or spin precession? Distinguishing subdominant effects in gravitational-wave data
    Nov 21, 2022 – 00:50
  • 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
  • Chandra measurements of gas homogeneity and turbulence at intermediate radii in the Perseus Cluster
    Nov 21, 2022 – 00:47
  • 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
  • Variability In A Low-Mass AGN: Oscillation Or Eruption?
    Nov 21, 2022 – 01:06
  • MeV-GeV Gamma-ray Emission from SNR G327 1-1 1 Discovered by the Fermi-LAT
    Nov 21, 2022 – 00:51
  • Broadband Spectral properties of MAXI J1348--630 using AstroSat Observations
    Nov 21, 2022 – 00:39
  • Spectral properties of the Be X-ray pulsar 2S 1553-542 during Type II outbursts
    Nov 21, 2022 – 00:58
  • CARMA-NRO Orion Survey: unbiased survey of dense cores and core mass functions in Orion A
    Nov 21, 2022 – 01:09
  • Locating Hidden Exoplanets in ALMA Data Using Machine Learning
    Nov 21, 2022 – 00:26
  • The hard to soft transition of GX 339-4 as seen by Insight-HXMT
    Nov 21, 2022 – 00:44
  • MeV-GeV Gamma-ray Emission from SNR G327 1-1 1 Discovered by the Fermi-LAT
    Nov 21, 2022 – 00:51
  • Understanding the role of morphology and environment on the dynamical evolution of isolated galaxy triplets
    Nov 21, 2022 – 01:08
  • Asgard NOTT: L-band nulling interferometry at the VLTI I Simulating the expected high-contrast performance
    Nov 21, 2022 – 01:04
  • Global MHD simulations of the solar convective zone using a volleyball mesh decomposition I Pilot
    Nov 21, 2022 – 00:47
  • A strong H- opacity signal in the near-infrared emission spectrum of the ultra-hot Jupiter KELT-9b
    Nov 21, 2022 – 01:08
  • Surviving in Ocean Worlds: Experimental Characterization of Fiber Optic Tethers across Europa-like Ice Faults and Unraveling the Sliding Behavior of Ice
    Nov 21, 2022 – 00:54
  • Linking the Internal Properties of Infant Globular Clusters to their Formation Environments
    Nov 21, 2022 – 00:46
  • Hydrodynamical Simulations of Black-Hole Binary Formation in AGN Disks
    Nov 21, 2022 – 00:32
  • Deep Learning-based galaxy image deconvolution
    Nov 21, 2022 – 00:40
  • Detecting deviations from Gaussianity in high-redshift CMB lensing maps
    Nov 21, 2022 – 00:31
  • High-resolution atmospheric retrievals of WASP-121b transmission spectroscopy with ESPRESSO: Consistent relative abundance constraints across multiple epochs and instruments
    Nov 21, 2022 – 01:16
  • 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
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