**Latest preprints on astro-ph:**

› Accurate Gaunt factors for non-relativistic quadrupole bremsstrahlung. (arXiv:2103.03248v1 [astro-ph.CO])

› The Hubble Tension as a Hint of Leptogenesis and Neutrino Mass Generation. (arXiv:2103.03249v1 [hep-ph])

› Reconstructing the Last Major Merger of the Milky Way with the H3 Survey. (arXiv:2103.03251v1 [astro-ph.GA])

› Constraining the Epoch of Reionization With Highly Dispersed Fast Radio Bursts. (arXiv:2103.03252v1 [astro-ph.CO])

› Freeze-In Dark Matter within the Seesaw mechanism. (arXiv:2103.03253v1 [hep-ph])

› Heavy decaying dark matter at future neutrino radio telescopes. (arXiv:2103.03254v1 [hep-ph])

› Early Science with the Large Millimeter Telescope: Constraining the Gas Fraction of a Compact Quiescent Galaxy at z=1.883. (arXiv:2103.03255v1 [astro-ph.GA])

› Strong lens modelling: comparing and combining Bayesian neural networks and parametric profile fitting. (arXiv:2103.03257v1 [astro-ph.IM])

› On the Zero Point Constant of the Bolometric Correction Scale. (arXiv:2103.03258v1 [astro-ph.SR])

› Revisiting the Kepler field with TESS: Improved ephemerides using TESS 2min data. (arXiv:2103.03259v1 [astro-ph.EP])

› Implications of the $z>5$ Lyman-$\alpha$ forest for the 21-cm power spectrum from the epoch of reionization. (arXiv:2103.03261v1 [astro-ph.CO])

› The HOSTS survey: evidence for an extended dust disk and constraints on the presence of giant planets in the Habitable Zone of $\beta$ Leo. (arXiv:2103.03268v1 [astro-ph.EP])

› External gas accretion provides a fresh gas supply to the active S0 galaxy NGC 5077. (arXiv:2103.03277v1 [astro-ph.GA])

› Cosmological Constraints from Galaxy Cluster Sparsity, Cluster Gas Mass Fraction and Baryon Acoustic Oscillations Data. (arXiv:2103.03283v1 [astro-ph.CO])

› Interstellar Objects in the Solar System: 1. Isotropic Kinematics from the Gaia Early Data Release 3. (arXiv:2103.03289v1 [astro-ph.EP])

› Probing inflation with large-scale structure data: the contribution of information at small scales. (arXiv:2103.03291v1 [astro-ph.CO])

› The discovery of a highly accreting, radio-loud quasar at z=6.82. (arXiv:2103.03295v1 [astro-ph.CO])

› Earth-skimming Ultra-high Energy Tau Neutrinos simulated with MonteCarlo method and CONEX code. (arXiv:2103.03303v1 [hep-ph])

› Fitting an Analytic Magnetic Field to a Prestellar Core. (arXiv:2103.03324v1 [astro-ph.SR])

› PSFs for mapping artificial night sky luminance over large territories. (arXiv:2103.03341v1 [astro-ph.IM])

› Broadband Imaging of Meteor Radio Afterglows. (arXiv:2103.03347v1 [astro-ph.EP])

› Atom-in-jellium equations of state and melt curves in the white dwarf regime. (arXiv:2103.03371v1 [astro-ph.SR])

› Electromagnetic Signatures from the Tidal Tail of a Black Hole - Neutron Star Merger. (arXiv:2103.03378v1 [astro-ph.HE])

› The Merger Dynamics of the Galaxy Cluster Abell 1775: New Insights from Chandra and XMM-Newton for a Cluster Simultaneously Hosting a WAT and a NAT Radio Sources. (arXiv:2103.03382v1 [astro-ph.CO])

› Fermi-LAT Detection of GeV Gamma-Ray Emission from The Highly Asymmetric Shell Supernova Remnant: SNR G317.3-0.2. (arXiv:2103.03415v1 [astro-ph.HE])

› The Constraint of H0from Galaxy clusters and Hubble parameter data. (arXiv:2103.03440v1 [astro-ph.CO])

› Implications of the Environments of Radio-detected AGN in a Complex Proto-structure at z$\sim$3.3. (arXiv:2103.03441v1 [astro-ph.GA])

› On the Detection of Habitable Trojan Planets in the Kepler Circumbinary Systems. (arXiv:2103.03455v1 [astro-ph.EP])

› Entropy production due to electroweak phase transition in the framework of two Higgs doublet model. (arXiv:2103.03477v1 [hep-ph])

› Resolving the Radio Emission from the Quasar P172+18 at $z = 6.82$. (arXiv:2103.03481v1 [astro-ph.GA])

› Planck Cold Clumps in the lambda Orionis Complex. III. A chemical probe of stellar feedback on cores in the lambda Orionis cloud. (arXiv:2103.03499v1 [astro-ph.GA])

› Velocity-resolved Reverberation Mapping of Changing-look AGN NGC 2617. (arXiv:2103.03508v1 [astro-ph.GA])

› The response of the Convolutional Neural Network to the transient noise in Gravitational wave detection. (arXiv:2103.03557v1 [gr-qc])

› Mid-IR cosmological spectrophotometric surveys from space: Measuring AGN and star formation at the Cosmic Noon with a SPICA-like mission. (arXiv:2103.03584v1 [astro-ph.GA])

› Confirmation and physical characterization of the new bulge globular cluster Patchick 99 from the VVV and Gaia surveys. (arXiv:2103.03592v1 [astro-ph.GA])

› Experimental study of clusters in dense granular gas and implications for the particle stopping time in protoplanetary disks. (arXiv:2103.03609v1 [astro-ph.IM])

› Black Hole Superradiance in the Presence of Lorentz Symmetry Violation. (arXiv:2103.03611v1 [gr-qc])

› Inhomogeneous Hubble diagram from vector K-mouflage. (arXiv:2103.03627v1 [astro-ph.CO])

› Mass of prominences experiencing failed eruptions. (arXiv:2103.03634v1 [astro-ph.SR])

› Relative field line helicity of a large eruptive solar active region. (arXiv:2103.03643v1 [astro-ph.SR])

› Rediscussion of eclipsing binaries. Paper IV. The evolved G-type system AN Camelopardalis. (arXiv:2103.03644v1 [astro-ph.SR])

› The OTELO survey: Faint end of the luminosity function of [OII] emitters at = 1.43. (arXiv:2103.03645v1 [astro-ph.GA])

› The role of CP-conserving annihilations in generating cosmological particle-antiparticle asymmetries. (arXiv:2103.03650v1 [hep-ph])

› XMMU J050722.1-684758: Discovery of a new Be X-ray binary pulsar likely associated with the supernova remnant MCSNR J0507-6847. (arXiv:2103.03657v1 [astro-ph.HE])

› Cosmological Constraints on the Coupling Model from Observational Hubble Parameter and Baryon Acoustic Oscillation Measurements. (arXiv:2103.03670v1 [astro-ph.CO])

› Convective core sizes in rotating massive stars: I. Constraints from solar metallicity OB field stars. (arXiv:2103.03672v1 [astro-ph.SR])

› SALT observations of the supernova remnant MCSNR J0127-7332 and its associated Be X-ray binary SXP 1062 in the SMC. (arXiv:2103.03707v1 [astro-ph.HE])

› Could switchbacks originate in the lower solar atmosphere? I. Formation mechanisms of switchbacks. (arXiv:2103.03726v1 [astro-ph.SR])

› Occultation mapping of Io's surface in the near-infrared I: Inferring static maps. (arXiv:2103.03758v1 [astro-ph.EP])

› Amplitude of solar gravity modes generated by penetrative plumes. (arXiv:2103.03760v1 [astro-ph.SR])

› FUV Variable Sources in M31. (arXiv:2103.03772v1 [astro-ph.GA])

› From Photometric Redshifts to Improved Weather Forecasts: machine learning and proper scoring rules as a basis for interdisciplinary work. (arXiv:2103.03780v1 [astro-ph.IM])

› First and second-generation black hole and neutron star mergers in 2+2 quadruples: population statistics. (arXiv:2103.03782v1 [astro-ph.HE])

› Relationship between magnetic field properties and statistical flow using numerical simulation and magnetic feature tracking on solar photosphere. (arXiv:2103.03789v1 [astro-ph.SR])

› Discovery of the propargyl radical (CH2CCH) in TMC-1: one of the most abundant radicals ever found and a key species for cyclization to benzene in cold dark clouds. (arXiv:2103.03807v1 [astro-ph.GA])

› Quantum study of reaction O(3P) + H2(v,j) $\rightarrow$ OH + H: OH formation in strongly UV-irradiated gas. (arXiv:2103.03810v1 [astro-ph.GA])

› Generalized Emergent Dark Energy Model and the Hubble Constant Tension. (arXiv:2103.03815v1 [astro-ph.CO])

› Optical constants of a solar system organic analog and the Allende meteorite in the near and mid-infrared (1.5-13 {\mu}m). (arXiv:2103.03822v1 [astro-ph.EP])

› On single-point inversions of magnetic dipole lines in the corona. (arXiv:2103.03824v1 [astro-ph.SR])

› The Post-impact Evolution of the X-ray Emitting Gas in SNR 1987A Viewed by XMM-Newton. (arXiv:2103.03844v1 [astro-ph.HE])

› Evolution of Splashback Boundaries and Gaseous Outskirts: Insights from Mergers of Self-similar Galaxy Clusters. (arXiv:2103.03850v1 [astro-ph.CO])

› Shadows of parametrized axially symmetric black holes allowing for separation of variables. (arXiv:2103.03855v1 [gr-qc])

› KMOS study of the mass accretion rate from Class I to Class II in NGC 1333. (arXiv:2103.03863v1 [astro-ph.SR])

› Effects of the shape of curvature peaks on the size of primordial black holes. (arXiv:2103.03867v1 [gr-qc])

› Atomic Carbon [CI]$(^3P_1-^3P_0)$ Mapping of the Nearby Galaxy M83. (arXiv:2103.03876v1 [astro-ph.GA])

› Testing noncommutativity-like model as a galactic density profile. (arXiv:1610.02464v3 [astro-ph.GA] UPDATED)

› Observational Aspect of Black Hole Dark Matter. (arXiv:1912.01325v2 [astro-ph.CO] UPDATED)

› Calibration Method and Uncertainty for the Primordial Inflation Explorer (PIXIE). (arXiv:2002.00976v2 [astro-ph.IM] UPDATED)

› Axisymmetric Radiative Transfer Models of Kilonovae. (arXiv:2004.00102v2 [astro-ph.HE] UPDATED)

› Searching for solar axions using data from the Sudbury Neutrino Observatory. (arXiv:2004.02733v3 [hep-ph] UPDATED)

› Atmospheric Escape of Close-in Giants around Hot Stars: Far-Ultraviolet Radiation and Photoelectric Heating Effect. (arXiv:2005.08676v2 [astro-ph.EP] UPDATED)

› The thermal and gravitational energy densities in the large-scale structure of the Universe. (arXiv:2007.01679v3 [astro-ph.CO] UPDATED)

› Information content in the redshift-space galaxy power spectrum and bispectrum. (arXiv:2007.04340v2 [astro-ph.CO] UPDATED)

› Reheating in holographic cosmology and connecting to $\Lambda$-MSSM constructions for particle physics. (arXiv:2008.06144v3 [hep-th] UPDATED)

› A new era of fine structure constant measurements at high redshift. (arXiv:2008.10619v2 [astro-ph.CO] UPDATED)

› Small-Scale Dynamo in Supernova-Driven Interstellar Turbulence. (arXiv:2010.01833v5 [astro-ph.GA] UPDATED)

› Probing Fundamental Physics with Gravitational Waves: The Next Generation. (arXiv:2010.09010v3 [gr-qc] UPDATED)

› The exact WKB for cosmological particle production. (arXiv:2010.14835v2 [hep-ph] UPDATED)

› Gravitational-wave Signals From Three-dimensional Supernova Simulations With Different Neutrino-Transport Methods. (arXiv:2011.10499v2 [astro-ph.HE] UPDATED)

› Exoplanet Detection using Machine Learning. (arXiv:2011.14135v2 [astro-ph.EP] UPDATED)

› Renormalization group analysis of superradiant growth of self-interacting axion cloud. (arXiv:2012.03473v3 [gr-qc] UPDATED)

› Extending the $Z^2_n$ and $H$ statistics to generic pulsed profiles. (arXiv:2012.11397v3 [astro-ph.IM] UPDATED)

› Application of Regge-theory to astronomical objects. (arXiv:2012.14276v5 [physics.class-ph] UPDATED)

› Evidence for an 8 MeV line in the SN 1987A neutrino spectrum and five reasons to expect one. (arXiv:2101.08128v8 [astro-ph.HE] UPDATED)

› Transport properties of superfluid phonons in neutron stars. (arXiv:2101.09000v2 [nucl-th] UPDATED)

› HI-MaNGA: Tracing the physics of the neutral and ionized ISM with the second data release. (arXiv:2101.12680v2 [astro-ph.GA] UPDATED)

› Estimate on dust scale height from ALMA dust continuum image of the HD 163296 protoplanetary disk. (arXiv:2102.06209v2 [astro-ph.EP] UPDATED)

› `Oumuamua is not Artificial. (arXiv:2102.07871v2 [physics.pop-ph] UPDATED)

› A Far Ultraviolet Spectroscopic Explorer Survey of Interstellar Molecular Hydrogen in the Galactic Disk. (arXiv:2102.11301v2 [astro-ph.GA] UPDATED)

› Absorption effects in the blazar's gamma-ray spectra due to luminous stars crossing the jet. (arXiv:2102.11589v2 [astro-ph.HE] UPDATED)

› Baryogenesis and gravity waves from a UV-completed electroweak phase transition. (arXiv:2102.12490v2 [hep-ph] UPDATED)

› Survival of the Fittest: Numerical Modeling of Supernova 2014C. (arXiv:2102.12581v2 [astro-ph.HE] UPDATED)

› The miniJPAS survey: Identification and characterization of galaxy populations with the J-PAS photometric system. (arXiv:2102.13121v2 [astro-ph.GA] UPDATED)

› Finite Action Principle and Horava-Lifshitz Gravity: early universe, black holes and wormholes. (arXiv:2102.13556v2 [gr-qc] UPDATED)

› Determination of Planetary Nebulae angular diameters from radio continuum Spectral Energy Distribution modeling. (arXiv:2103.00004v2 [astro-ph.GA] UPDATED)

› Lyman continuum leakage from low-mass galaxies with Mstar < 1.E8 Msun. (arXiv:2103.01514v2 [astro-ph.GA] UPDATED)

› A Relativistic Quantum Approach to Neutrino and Antineutrino Emissions via the Direct Urca Process in Strongly Magnetized Neutron-Star Matter. (arXiv:2103.01703v3 [nucl-th] UPDATED)

› A Unified Calibration Framework for 21 cm Cosmology. (arXiv:2004.08463v2 [astro-ph.IM] CROSS LISTED)