Latest preprints on astro-ph:

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› An Explanation of the Vaughan - Preston Gap. (arXiv:1810.06558v1 [astro-ph.SR])
› STARRY: Analytic Occultation Light Curves. (arXiv:1810.06559v1 [astro-ph.IM])
› The COS Absorption Survey of Baryon Harbors (CASBaH): Warm-hot Circumgalactic Gas Reservoirs Traced by Ne VIII Absorption. (arXiv:1810.06560v1 [astro-ph.GA])
› Measurement of the primordial helium abundance from the intergalactic medium. (arXiv:1810.06561v1 [astro-ph.CO])
› Discovering AGN-driven winds through their infrared emission: I. General method and wind location. (arXiv:1810.06562v1 [astro-ph.GA])
› Science with an ngVLA: Accreting Supermassive Black Holes in Nearby Low-mass Galaxies. (arXiv:1810.06564v1 [astro-ph.GA])
› Science with an ngVLA: Stellar Emission as a Source of Flux Bias in Debris Disks. (arXiv:1810.06565v1 [astro-ph.SR])
› Figuring Out Gas and Galaxies in Enzo (FOGGIE). I. Resolving Simulated Circumgalactic Absorption at 2 < z < 2.5. (arXiv:1810.06566v1 [astro-ph.GA])
› Science with an ngVLA: SETI Searches for Evidence of Intelligent Life in the Galaxy. (arXiv:1810.06568v1 [astro-ph.IM])
› Simulating the M-R Relation from APF follow up of TESS targets: Survey design and strategies for overcoming mass biases. (arXiv:1810.06569v1 [astro-ph.EP])
› Investigating the X-ray enhancements of highly radio-loud quasars at z > 4. (arXiv:1810.06572v1 [astro-ph.HE])
› Is the ring inside or outside the planet?: The effect of planet migration on dust rings. (arXiv:1810.06573v1 [astro-ph.EP])
› Science with an ngVLA: Neutral Atomic Hydrogen in the Local Universe. (arXiv:1810.06575v1 [astro-ph.GA])
› ngVLA: Astrometry and Long Baseline Science. (arXiv:1810.06577v1 [astro-ph.GA])
› The Limited Contribution of Low- and High-Luminosity Gamma-Ray Bursts to Ultra-High Energy Cosmic Rays. (arXiv:1810.06579v1 [astro-ph.HE])
› Science with an ngVLA: Resolving the Radio Complexity of EXor and FUor-type Systems with the ngVLA. (arXiv:1810.06580v1 [astro-ph.EP])
› Probing the Jets of Blazars Using the Temporal Symmetry of Their Multi-Wavelength Outbursts. (arXiv:1810.06585v1 [astro-ph.GA])
› Science with an ngVLA: Prebiotic Molecules. (arXiv:1810.06586v1 [astro-ph.GA])
› Zombie Vortex Instability. III. Persistence with Nonuniform Stratification and Radiative Damping. (arXiv:1810.06588v1 [astro-ph.SR])
› Gravitoturbulent dynamos in astrophysical discs. (arXiv:1810.06589v1 [astro-ph.HE])
› Science with an ngVLA: New Frontiers in Protostellar Multiplicity with the ngVLA. (arXiv:1810.06590v1 [astro-ph.GA])
› Science with the Next-Generation VLA and Pulsar Timing Arrays. (arXiv:1810.06594v1 [astro-ph.IM])
› Resolved Kinematics of Runaway and Field OB Stars in the Small Magellanic Cloud. (arXiv:1810.06596v1 [astro-ph.GA])
› Science with an ngVLA: Resolved Substructures in Protoplanetary Disks. (arXiv:1810.06598v1 [astro-ph.EP])
› Science with an ngVLA: Tracing the Water Snowline in Protoplanetary disks with the ngVLA. (arXiv:1810.06604v1 [astro-ph.EP])
› Science with an ngVLA: Characterizing Feedback Through Molecular Outflows Across Cosmic Time. (arXiv:1810.06605v1 [astro-ph.GA])
› Science with an ngVLA: Offset Active Galactic Nuclei. (arXiv:1810.06609v1 [astro-ph.GA])
› Science with an ngVLA: Precision Gas-dynamical Mass Measurement of Supermassive Black Holes with the ngVLA. (arXiv:1810.06615v1 [astro-ph.GA])
› The Changing-Look Quasar Mrk 590 is Awakening. (arXiv:1810.06616v1 [astro-ph.GA])
› Science with an ngVLA: ngVLA Observations of Coronal Magnetic Fields. (arXiv:1810.06622v1 [astro-ph.SR])
› Galactic Center Pulsars with the ngVLA. (arXiv:1810.06623v1 [astro-ph.HE])
› Diffraction of light by the gravitational field of the Sun and the solar corona. (arXiv:1810.06627v1 [gr-qc])
› Torsional oscillations of magnetised neutron stars with mixed poloidal-toroidal fields. (arXiv:1810.06628v1 [astro-ph.HE])
› Science with an ngVLA: Observations of the Solar Wind. (arXiv:1810.06633v1 [astro-ph.SR])
› Structure of high-redshift galaxies in cosmological simulations. (arXiv:1810.06647v1 [astro-ph.GA])
› Lyman-alpha power spectrum as a probe of modified gravity. (arXiv:1810.06661v1 [astro-ph.CO])
› Science with an ngVLA: Radio Recombination Lines from HII Regions. (arXiv:1810.06664v1 [astro-ph.GA])
› Science with an ngVLA: Evolved Stars. (arXiv:1810.06666v1 [astro-ph.SR])
› Science with a ngVLA: Imaging planetary systems in the act of forming with the ngVLA. (arXiv:1810.06671v1 [astro-ph.EP])
› Probing $\Lambda$CDM cosmology with the Evolutionary Map of the Universe survey. (arXiv:1810.06672v1 [astro-ph.CO])
› Probing dark matter and galaxy evolution with proper motions of galaxies. (arXiv:1810.06674v1 [astro-ph.GA])
› Massive and Evolved Stars with the ngVLA. (arXiv:1810.06676v1 [astro-ph.SR])
› Science with an ngVLA: Tidal disruption events. (arXiv:1810.06677v1 [astro-ph.HE])
› Future ground arrays for ultrahigh-energy cosmic rays: recent updates and perspectives. (arXiv:1810.06678v1 [astro-ph.HE])
› Science with an ngVLA: Probing Strong Binary Interactions and Accretion in AGB stars with the ngVLA. (arXiv:1810.06685v1 [astro-ph.SR])
› Science with the ngVLA: H$_2$O Megamaser Cosmology. (arXiv:1810.06686v1 [astro-ph.CO])
› Convective overshooting and penetration in a Boussinesq spherical shell. (arXiv:1810.06700v1 [astro-ph.SR])
› Science with an ngVLA: Star-forming Filaments and Cores on a Galactic Scale. (arXiv:1810.06701v1 [astro-ph.SR])
› A Design for an Electromagnetic Filter for Precision Energy Measurements at the Tritium Endpoint. (arXiv:1810.06703v1 [astro-ph.IM])
› Science with an ngVLA: Molecular Clouds in Galaxies. (arXiv:1810.06706v1 [astro-ph.GA])
› Science with an ngVLA: Gas Density Across the Universe. (arXiv:1810.06709v1 [astro-ph.GA])
› Science with the ngVLA: Planetary Nebulae. (arXiv:1810.06712v1 [astro-ph.SR])
› Science with an ngVLA: Debris disk structure and composition. (arXiv:1810.06719v1 [astro-ph.GA])
› Science with an ngVLA: Organics in Disk Midplanes with the ngVLA. (arXiv:1810.06724v1 [astro-ph.GA])
› Science with an ngVLA: Accretion and Jets in Local Compact Objects. (arXiv:1810.06727v1 [astro-ph.HE])
› Forward modelling of brightness variations in Sun-like stars I. Emergence and surface transport of magnetic flux. (arXiv:1810.06728v1 [astro-ph.SR])
› Science with an ngVLA: How Do Cold Gas Outflows Shape Galaxies?. (arXiv:1810.06737v1 [astro-ph.GA])
› An alternative stable solution for the Kepler-419 system, obtained with the use of a genetic algorithm. (arXiv:1810.06769v1 [astro-ph.EP])
› Science with an ngVLA - The Molecular High-z Universe on Large Scales: Low-surface-brightness CO and the strength of the ngVLA Core. (arXiv:1810.06770v1 [astro-ph.GA])
› Science with an ngVLA: A six-dimensional tomographic view of Galactic star-formation. (arXiv:1810.06779v1 [astro-ph.GA])
› Graphene and Carbon Nanotubes in Space. (arXiv:1810.06786v1 [astro-ph.GA])
› Narrow Transient Absorptions in Late-Time Optical Spectra of Type Ia Supernovae: Evidence for Large Clumps of Iron-Rich Ejecta?. (arXiv:1810.06788v1 [astro-ph.HE])
› Science with an ngVLA: ngVLA Studies of Classical Novae. (arXiv:1810.06790v1 [astro-ph.IM])
› Comment on "keV Neutrino Dark Matter in a Fast Expanding Universe" by Biswas et al. (arXiv:1810.06795v1 [hep-ph])
› A systematic study of Galactic infrared bubbles along the Galactic plane with AKARI and Herschel. (arXiv:1810.06799v1 [astro-ph.GA])
› Science with an ngVLA: Local Constraints on Supermassive Black Hole Seeds. (arXiv:1810.06814v1 [astro-ph.HE])
› Outlying H$\alpha$ blobs in SDSS IV MaNGA. (arXiv:1810.06821v1 [astro-ph.GA])
› Science with an ngVLA. Cold gas in High-z Galaxies: CO as redshift beacon. (arXiv:1810.06841v1 [astro-ph.GA])
› STIM map: detection map for exoplanets imaging beyond asymptotic Gaussian residual speckle noise. (arXiv:1810.06895v1 [astro-ph.IM])
› Understanding mechanical feedback from HERGs and LERGs. (arXiv:1810.06899v1 [astro-ph.GA])
› $\alpha$-attractor-type Double Inflation. (arXiv:1810.06914v1 [hep-th])
› Overcoming the limitations of the energy-limited approximation for planet atmospheric escape. (arXiv:1810.06920v1 [astro-ph.EP])
› ALMA Reveals a Misaligned Inner Gas Disk inside the Large Cavity of a Transitional Disk. (arXiv:1810.06941v1 [astro-ph.EP])
› Cosmic Ray Extremely Distributed Observatory: a global network of detectors to probe contemporary physics mysteries. (arXiv:1810.06953v1 [astro-ph.IM])
› Gamma-ray bursts as cool synchrotron sources. (arXiv:1810.06965v1 [astro-ph.HE])
› Impact of measurement errors on the inferred stellar asteroseismic ages. Statistical models for intermediate age main sequence and red giant branch stars. (arXiv:1810.06997v1 [astro-ph.SR])
› Science with the ngVLA: Extreme Scattering Events and Symmetric Achromatic Variations. (arXiv:1810.07009v1 [astro-ph.GA])
› A systematic survey of grain growth in discs around post-AGB binaries with PACS and SPIRE photometry. (arXiv:1810.07011v1 [astro-ph.SR])
› Impact of Plasma Instability on Constraint of the Intergalactic Magnetic Field. (arXiv:1810.07013v1 [astro-ph.HE])
› Fundamental Concepts. (arXiv:1810.07032v1 [astro-ph.HE])
› NuSTAR Detection of Nonthermal Bremsstrahlung from the Supernova Remnant W49B. (arXiv:1810.07036v1 [astro-ph.HE])
› Accreting Black Holes. (arXiv:1810.07041v1 [astro-ph.HE])
› Can magnetic fields stabilize or destabilize twin stars?. (arXiv:1810.07046v1 [nucl-th])
› Pebble dynamics and accretion onto rocky planets. II. Radiative models. (arXiv:1810.07048v1 [astro-ph.EP])
› The optimal gravitational softening length for cosmological N-body simulations. (arXiv:1810.07055v1 [astro-ph.CO])
› The Substellar Transition Zone: A Stretched Temperature Canyon in Brown Dwarf Population due to Unsteady Hydrogen Fusion. (arXiv:1810.07071v1 [astro-ph.SR])
› Science with an ngVLA: Probing Obscured MBH Accretion and Growth since Cosmic Dawn. (arXiv:1810.07098v1 [astro-ph.GA])
› S stars and s-process in the Gaia era I. Stellar parameters and chemical abundances in a sub-sample of S stars with new MARCS model atmospheres. (arXiv:1810.07105v1 [astro-ph.SR])
› Spin response and neutrino mean free path in neutron matter. (arXiv:1810.07110v1 [nucl-th])
› Study of the reflection spectra of SAX J1748.9-2021. (arXiv:1810.07115v1 [astro-ph.HE])
› On gravitational echoes from ultracompact exotic stars. (arXiv:1810.07137v1 [gr-qc])
› Science with an ngVLA: New Parameter Space for Deep Field Radio Continuum Surveys. (arXiv:1810.07143v1 [astro-ph.GA])
› New Formation Models for the Kepler-36 System. (arXiv:1810.07160v1 [astro-ph.EP])
› Science with an ngVLA: Deuteration in starless and prestellar cores. (arXiv:1810.07163v1 [astro-ph.IM])
› Monte-Carlo methods for NLTE spectral synthesis of supernovae. (arXiv:1810.07165v1 [astro-ph.SR])
› Deep lensing with a twist: E and B modes in a field with multiple lenses. (arXiv:1709.09721v2 [astro-ph.CO] UPDATED)
› The APOGEE-2 survey: \textit{H}-band discovery of additional Second-Generation stars in the Galactic Bulge Globular Cluster NGC 6522. (arXiv:1801.07136v2 [astro-ph.GA] UPDATED)
› Shape and angular distribution of the 4.438-MeV line from proton inelastic scattering off 12C. (arXiv:1802.00658v2 [nucl-ex] UPDATED)
› FITS Data Source for Apache Spark. (arXiv:1804.07501v2 [astro-ph.IM] UPDATED)
› Lack of time dilation in type Ia supernovae and Gamma-Ray Bursts. (arXiv:1804.10274v3 [astro-ph.HE] UPDATED)
› With and without spectroscopy: Gaia DR2 proper motions of seven Ultra-Faint Dwarf Galaxies. (arXiv:1805.01839v2 [astro-ph.GA] UPDATED)
› Tree-less 3d Friends-of-Friends using Spatial Hashing. (arXiv:1805.04911v2 [astro-ph.CO] UPDATED)
› How Li & Paczynski Model of Kilonova Fits GW170817 Optical Counterpart. (arXiv:1805.09043v3 [astro-ph.HE] UPDATED)
› A Zeldovich reconstruction method for measuring redshift space distortions using cosmic voids. (arXiv:1805.09349v2 [astro-ph.CO] UPDATED)
› Properties of the binary neutron star merger GW170817. (arXiv:1805.11579v2 [gr-qc] UPDATED)
› Stability of Condensed Fuzzy Dark Matter Halos. (arXiv:1805.12147v2 [astro-ph.CO] UPDATED)
› Science with an ngVLA: Understanding Massive Star Formation through Maser Imaging. (arXiv:1806.06981v2 [astro-ph.GA] UPDATED)
› Novel constraints on non-cold (non-thermal) Dark Matter from Lyman-$\alpha$ forest data. (arXiv:1806.08371v2 [astro-ph.CO] UPDATED)
› CLUMPY v3: $\gamma$-ray and $\nu$ signals from dark matter at all scales. (arXiv:1806.08639v2 [astro-ph.CO] UPDATED)
› An almanac of predicted microlensing events for the 21st century. (arXiv:1806.10003v3 [astro-ph.SR] UPDATED)
› Re-visiting the case of R Mon: Is CO removed at R
› Galaxy Two-Point Correlation Function in General Relativity. (arXiv:1807.09796v2 [astro-ph.CO] UPDATED)
› Measuring Linear and Non-linear Galaxy Bias Using Counts-in-Cells in the Dark Energy Survey Science Verification Data. (arXiv:1807.10331v2 [astro-ph.CO] UPDATED)
› E and B polarizations from inhomogeneous and solar surface turbulence. (arXiv:1807.11457v2 [astro-ph.SR] UPDATED)
› On the requirement for mixing-heating to utilize bubble cosmic rays to heat the intracluster medium. (arXiv:1808.04715v2 [astro-ph.GA] UPDATED)
› Modified Axion Electrodynamics through Oscillating Vacuum Polarization and Magnetization and Low Mass Detection. (arXiv:1809.01654v3 [hep-ph] UPDATED)
› Turbulent Action at a Distance due to Stellar Feedback in Magnetized Clouds. (arXiv:1809.03513v2 [astro-ph.SR] UPDATED)
› Experimental results from the ST7 mission on LISA Pathfinder. (arXiv:1809.08969v2 [astro-ph.IM] UPDATED)
› New HARPS and FEROS observations of GJ1046. (arXiv:1809.09638v2 [astro-ph.EP] UPDATED)
› Baryogenesis and Dark Matter from $B$ Mesons. (arXiv:1810.00880v2 [hep-ph] UPDATED)
› Shedding light on the Milky Way rotation curve with Gaia DR2. (arXiv:1810.04445v2 [astro-ph.GA] UPDATED)
› Bayesian cosmic density field inference from redshift space dark matter maps. (arXiv:1810.05189v2 [astro-ph.CO] UPDATED)
› Testing velocity-dependent CPT-violating gravitational forces with radio pulsars. (arXiv:1810.06332v1 [gr-qc] CROSS LISTED)

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