Latest preprints on astro-ph:

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› GLOSTAR -- Radio Source Catalog I: $28^{\circ}< \textit{l} < 36^{\circ}$ and $|b| < 1^{\circ}$. (arXiv:1905.09281v1 [astro-ph.GA])
› Pre-Supernova Neutrinos in Large Dark Matter Direct Detection Experiments. (arXiv:1905.09283v1 [hep-ph])
› Supernova signals of light dark matter. (arXiv:1905.09284v1 [hep-ph])
› Through thick or thin: Multiple components of the magneto-ionic medium towards the nearby ${\rm H\,{\small II}}$ region Sharpless 2-27 revealed by Faraday tomography. (arXiv:1905.09285v1 [astro-ph.GA])
› OSSOS XVII: Probing the Distant Solar System with Observed Scattering TNOs. (arXiv:1905.09286v1 [astro-ph.EP])
› AGN-Driven Outflows in Dwarf Galaxies. (arXiv:1905.09287v1 [astro-ph.GA])
› $\bar T$: A New Cosmological Parameter?. (arXiv:1905.09288v1 [astro-ph.CO])
› Do star clusters form in a completely mass-segregated way?. (arXiv:1905.09289v1 [astro-ph.GA])
› Stellar Properties of z ~ 8 Galaxies in the Reionization Lensing Cluster Survey. (arXiv:1905.09295v1 [astro-ph.GA])
› The Wolf-Rayet binaries of the nitrogen sequence in the Large Magellanic Cloud: spectroscopy, orbital analysis, formation, and evolution. (arXiv:1905.09296v1 [astro-ph.SR])
› Dynamical Friction in Superfluids. (arXiv:1905.09297v1 [hep-ph])
› Establishing a New Technique for Discovering Large-Scale Structure Using the ORELSE Survey. (arXiv:1905.09298v1 [astro-ph.GA])
› Reconstructing Probability Distributions with Gaussian Processes. (arXiv:1905.09299v1 [astro-ph.CO])
› CASI: A Convolutional Neural Network Approach for Shell Identification. (arXiv:1905.09310v1 [astro-ph.IM])
› Element Abundances: A New Diagnostic for the Solar Wind. (arXiv:1905.09319v1 [astro-ph.SR])
› H0LiCOW XII. Lens mass model of WFI2033-4723 and blind measurement of its time-delay distance and $H_0$. (arXiv:1905.09338v1 [astro-ph.CO])
› Physical Correlations of the Scatter between Galaxy Mass, Stellar Content, and Halo Mass. (arXiv:1905.09353v1 [astro-ph.CO])
› Multi-epoch Low Radio Frequency Surveys of the Kepler K2 Mission Campaign Fields 3, 4, and 5 with the Murchison Widefield Array. (arXiv:1905.09392v1 [astro-ph.HE])
› Enhanced Habitability on High Obliquity Bodies near the Outer Edge of the Habitable Zone of Sun-like Stars. (arXiv:1905.09398v1 [astro-ph.EP])
› Discovery of exceptionally strong nuclear transition sheds new light on the fate of intermediate-mass stars. (arXiv:1905.09407v1 [astro-ph.SR])
› A Pseudodisk Threaded with a Toroidal and Pinched Poloidal Magnetic Field Morphology in the HH 211 Protostellar System. (arXiv:1905.09417v1 [astro-ph.GA])
› A general class of gravitational theories as alternatives to dark matter where the speed of gravity always equals the speed of light. (arXiv:1905.09465v1 [gr-qc])
› On the deviation from Maxwellian of the ion velocity distribution functions in the turbulent magnetosheath. (arXiv:1905.09466v1 [physics.space-ph])
› Constraining Lyman-alpha spatial offsets at $3
› Tidal disruption events onto stellar black holes in triples. (arXiv:1905.09471v1 [astro-ph.GA])
› Modified Gravity (MOG) fits to observed radial acceleration of SPARC galaxies. (arXiv:1905.09476v1 [gr-qc])
› WALLABY Early Science - III. An HI Study of the Spiral Galaxy NGC 1566. (arXiv:1905.09491v1 [astro-ph.GA])
› Cyclotron emission, absorption, and the two faces of X-ray pulsar A 0535+262. (arXiv:1905.09496v1 [astro-ph.HE])
› Ab initio spectroscopic characterization of the radical CH$_3$OCH$_2$ at low temperatures. (arXiv:1905.09506v1 [physics.chem-ph])
› Forward Modeling of the Type III Radio Burst Exciter. (arXiv:1905.09510v1 [astro-ph.SR])
› Comparison of Theoretical Starburst Photoionisation Models for Optical Diagnostics. (arXiv:1905.09528v1 [astro-ph.GA])
› Projected Pupil Plane Pattern (PPPP) with artificial Neural Networks. (arXiv:1905.09535v1 [astro-ph.IM])
› Modelling the X-ray power spectra of AGN by using reprocessing echoes from an extended corona. (arXiv:1905.09559v1 [astro-ph.HE])
› How Many Twists Do Solar Coronal Jets Release?. (arXiv:1905.09576v1 [astro-ph.SR])
› Thermodynamic Evolution of Secluded Vector Dark Matter: Conventional WIMPs and Nonconventional WIMPs. (arXiv:1905.09582v1 [hep-ph])
› Stellar escapers from M67 can reach solar-like Galactic orbits. (arXiv:1905.09586v1 [astro-ph.GA])
› Improving the muon track reconstruction of IceCube and IceCube-Gen2. (arXiv:1905.09612v1 [astro-ph.IM])
› Testing Modified Gravity with Wide Binaries in GAIA DR2. (arXiv:1905.09619v1 [astro-ph.CO])
› Revisiting the dust properties in the molecular clouds of the Large Magellanic Cloud. (arXiv:1905.09622v1 [astro-ph.GA])
› HST unveils a compact mildly relativistic Broad Line Region in the candidate true type 2 NGC 3147. (arXiv:1905.09627v1 [astro-ph.HE])
› Observational signature of a wind bubble environment for double neutron star mergers. (arXiv:1905.09663v1 [astro-ph.HE])
› Effects of dark matter pressure on the ellipticity of cosmic voids. (arXiv:1905.09664v1 [astro-ph.CO])
› Constraints on the collimated X-ray emission of SS 433 from the reflection on molecular clouds. (arXiv:1905.09667v1 [astro-ph.HE])
› Modified Gravity and Dark Energy models Beyond $w(z)$CDM Testable by LSST. (arXiv:1905.09687v1 [astro-ph.CO])
› An estimate of the dark matter density from galaxy clusters and supernovae data. (arXiv:1905.09689v1 [astro-ph.CO])
› Different Signatures of Chromospheric Evaporation in Two Solar Flares Observed with IRIS. (arXiv:1905.09709v1 [astro-ph.SR])
› The Role of Asymmetries in Thermal Non-Equilibrium. (arXiv:1905.09767v1 [astro-ph.SR])
› Can fermionic dark matter mimic supermassive black holes?. (arXiv:1905.09776v1 [astro-ph.GA])
› Model-independent determination of $H_0$ and $\Omega_{K0}$ from strong lensing and type Ia supernovae. (arXiv:1905.09781v1 [astro-ph.CO])
› Hinode EIS line widths in the quiet corona up to 1.5 Rsun. (arXiv:1905.09783v1 [astro-ph.SR])
› Puzzling Blue Dips in the Black Hole Candidate Swift J1357.2-0933, from ULTRACAM, SALT, ATCA, Swift and NuSTAR. (arXiv:1905.09784v1 [astro-ph.HE])
› ALMA Polarimetry of AT2018cow. (arXiv:1905.09785v1 [astro-ph.HE])
› Deuterated methanol toward NGC 7538-IRS1. (arXiv:1905.09798v1 [astro-ph.GA])
› Gaussbock: Fast parallel-iterative cosmological parameter estimation with Bayesian nonparametrics. (arXiv:1905.09800v1 [astro-ph.CO])
› MIFAL: fully automated Multiple-Image Finder ALgorithm for strong-lens modelling -- proof of concept. (arXiv:1905.09802v1 [astro-ph.CO])
› Disk masses in the Orion Molecular Cloud-2: distinguishing time and environment. (arXiv:1905.09804v1 [astro-ph.SR])
› Peculiar motion of the solar system derived from a dipole anisotropy in the redshift distribution of distant quasars. (arXiv:1405.4796v2 [astro-ph.CO] UPDATED)
› Quantum Cosmic No-Hair Theorem and Inflation. (arXiv:1802.09554v2 [hep-th] UPDATED)
› A Cosmological Signature of the SM Higgs Instability: Gravitational Waves. (arXiv:1804.07732v3 [hep-ph] UPDATED)
› Constraining the relativistic mean-field model equations of state with gravitational wave observations. (arXiv:1809.07108v3 [astro-ph.HE] UPDATED)
› Extended $\Lambda$CDM model and viscous dark energy: A Bayesian analysis. (arXiv:1810.03759v4 [astro-ph.CO] UPDATED)
› Affine-null metric formulation of General Relativity at two intersecting null hypersurfaces. (arXiv:1810.04743v3 [gr-qc] UPDATED)
› Constraining Compact Object Formation with 2M0521. (arXiv:1810.08206v2 [astro-ph.HE] UPDATED)
› Distinguishing standard and modified gravity cosmologies with machine learning. (arXiv:1810.11030v2 [astro-ph.CO] UPDATED)
› Titans of the Early Universe: The Prato Statement on the Origin of the First Supermassive Black Holes. (arXiv:1810.12310v2 [astro-ph.GA] UPDATED)
› Hypervelocity Stars from a Supermassive Black Hole-Intermediate-mass Black Hole binary. (arXiv:1810.12354v3 [astro-ph.GA] UPDATED)
› The Self-consistent Matter Coupling of a Class of Minimally Modified Gravity Theories. (arXiv:1811.02467v4 [gr-qc] UPDATED)
› 2D chemical evolution model: the impact of galactic disc asymmetries on azimuthal chemical abundance variations. (arXiv:1811.11196v2 [astro-ph.GA] UPDATED)
› A Finite Measure for the Initial Conditions of Inflation. (arXiv:1812.07095v4 [gr-qc] UPDATED)
› Generic absence of strong singularities and geodesic completeness in modified loop quantum cosmologies. (arXiv:1812.08937v2 [gr-qc] UPDATED)
› Properties and magnetic origins of solar S-bursts. (arXiv:1901.07424v2 [astro-ph.SR] UPDATED)
› Percent-Level Test of Isotropic Expansion Using Type Ia Supernovae. (arXiv:1902.07189v2 [astro-ph.CO] UPDATED)
› 21 cm cosmology and spin temperature reduction via spin-dependent dark matter interactions. (arXiv:1902.09552v2 [astro-ph.CO] UPDATED)
› Excitation and charge transfer in low-energy hydrogen atom collisions with neutral carbon and nitrogen. (arXiv:1904.00210v2 [astro-ph.SR] UPDATED)
› An old, metal-poor globular cluster in Sextans A and the metallicity floor of globular cluster systems. (arXiv:1904.01084v2 [astro-ph.GA] UPDATED)
› Stokes Inversion based on Convolutional Neural Networks. (arXiv:1904.03714v2 [astro-ph.SR] UPDATED)
› Barium & related stars and their white-dwarf companions I. Giant stars. (arXiv:1904.03975v2 [astro-ph.SR] UPDATED)
› Electron-positron pairs in hot plasma of accretion column in bright X-ray pulsars. (arXiv:1904.04604v2 [astro-ph.HE] UPDATED)
› Delineating the properties of matter in cold, dense QCD. (arXiv:1904.05080v2 [astro-ph.HE] UPDATED)
› Axion-Dilaton Destabilization and the Hubble Tension. (arXiv:1904.08912v4 [astro-ph.CO] UPDATED)
› Determination of the Cosmic Infrared Background from COBE/FIRAS and Planck HFI Observations. (arXiv:1904.11556v2 [astro-ph.CO] UPDATED)
› Detection of Planetary and Stellar Companions to Neighboring Stars via a Combination of Radial Velocity and Direct Imaging Techniques. (arXiv:1904.12931v2 [astro-ph.EP] UPDATED)
› Super-CMB fluctuations can resolve the Hubble tension. (arXiv:1905.02278v2 [astro-ph.CO] UPDATED)
› On physics of a highly relativistic spinning particle in the gravitational field. (arXiv:1905.04342v2 [gr-qc] UPDATED)
› Global distribution of far-ultraviolet emissions from highly ionized gas in the Milky Way. (arXiv:1905.07823v3 [astro-ph.GA] UPDATED)
› Fast and inefficient star formation due to short-lived molecular clouds and rapid feedback. (arXiv:1905.08801v2 [astro-ph.GA] UPDATED)
› Nested sampling on non-trivial geometries. (arXiv:1905.09110v2 [stat.CO] UPDATED)
› A Multi-epoch X-ray Study of the Spiral Galaxy NGC 7331. (arXiv:1905.09133v2 [astro-ph.HE] UPDATED)
› Non-Abelian basis tensor gauge theory. (arXiv:1905.08363v1 [hep-th] CROSS LISTED)
› Stochastic Gravitational Waves from Inflaton Decays. (arXiv:1905.08510v1 [hep-ph] CROSS LISTED)
› A Predictive Mirror Twin Higgs with Small $\mathbf{Z}_2$ Breaking. (arXiv:1905.08798v1 [hep-ph] CROSS LISTED)
› Black holes in the quantum universe. (arXiv:1905.08807v1 [hep-th] CROSS LISTED)

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