Latest preprints on astro-ph:

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› Constraints on Dark Matter-Photon Coupling in the Presence of Time-Varying Dark Energy. (arXiv:1907.05886v1 [astro-ph.CO])
› The Importance of Telescope Training in Data Interpretation. (arXiv:1907.05889v1 [astro-ph.IM])
› The Carnegie Chicago Hubble Program VI: Tip of the Red Giant Branch Distances to M66 and M96 of the Leo I Group. (arXiv:1907.05891v1 [astro-ph.GA])
› $Z'$ Mediated WIMPs: Dead, Dying, or Soon to be Detected?. (arXiv:1907.05893v1 [hep-ph])
› On the Diversity of Fallback Rates from Tidal Disruption Events with Accurate Stellar Structure. (arXiv:1907.05895v1 [astro-ph.HE])
› Rotational and rotational-vibrational Raman spectroscopy of air to characterize astronomical spectrographs. (arXiv:1907.05897v1 [astro-ph.IM])
› X-ray Plateaus in Gamma Ray Bursts' light-curves from jets viewed slightly off-axis. (arXiv:1907.05899v1 [astro-ph.HE])
› Kinematical evolution of multiple stellar populations in star clusters. (arXiv:1907.05901v1 [astro-ph.GA])
› The CGM-GRB Study. I. Uncovering The CircumGalactic Medium around GRB hosts at redshifts 2-6. (arXiv:1907.05903v1 [astro-ph.GA])
› Astro2020: Astrophotonics White Paper. (arXiv:1907.05904v1 [astro-ph.IM])
› The Hubble PanCET program: an extensive search for metallic ions in the exosphere of GJ 436 b. (arXiv:1907.05906v1 [astro-ph.EP])
› Can Assembly Bias Explain the Lensing Amplitude of the BOSS CMASS Sample in a Planck Cosmology?. (arXiv:1907.05909v1 [astro-ph.CO])
› Matter And Gravitation In Collisions of heavy ions and neutron stars: equation of state. (arXiv:1907.05921v1 [hep-ph])
› The Carnegie-Chicago Hubble Program. VIII. An Independent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch. (arXiv:1907.05922v1 [astro-ph.CO])
› Analysis of Helium-Rich White Dwarfs Polluted by Heavy Elements in the Gaia Era. (arXiv:1907.05932v1 [astro-ph.SR])
› Neutron star sensitivities in Ho\v{r}ava gravity after GW170817. (arXiv:1907.05958v1 [gr-qc])
› The impact of improved plasma diagnostics on modeling the X-ray Universe. (arXiv:1907.05963v1 [astro-ph.HE])
› A possibility of interpretation of the cosmic ray kneenear 10 TV as a contribution of a single close source. (arXiv:1907.05987v1 [astro-ph.HE])
› Elemental abundances in the remnant of the ancient eruption of CK Vulpeculae. (arXiv:1907.05998v1 [astro-ph.SR])
› An extensive-air-shower-like event registered with the TUS orbital detector. (arXiv:1907.06028v1 [astro-ph.HE])
› Overcoming the structural surface effect with a realistic treatment of turbulent convection in 1D stellar models. (arXiv:1907.06039v1 [astro-ph.SR])
› Astro2020 Activities and Projects White Paper: Arecibo Observatory in the Next Decade. (arXiv:1907.06052v1 [astro-ph.IM])
› Ghostly Damped Ly$\alpha$ Systems: Tracers of Gas Flows in the Close Vicinity of Quasars ?. (arXiv:1907.06056v1 [astro-ph.GA])
› Galactic diffuse gamma-ray emission at TeV energy. (arXiv:1907.06061v1 [astro-ph.HE])
› Energy Density, Temperature and Entropy Dynamics in Perturbative Reheating. (arXiv:1907.06084v1 [astro-ph.CO])
› Seeker based Adaptive Guidance via Reinforcement Meta-Learning Applied to Asteroid Close Proximity Operations. (arXiv:1907.06098v1 [eess.SY])
› Bondi-Hoyle-Lyttleton accretion in Supergiant X-ray binaries: stability and disk formation. (arXiv:1907.06108v1 [astro-ph.HE])
› Formation and delivery of complex organic molecules to the Solar System and early Earth. (arXiv:1907.06127v1 [astro-ph.EP])
› Shock fronts in the long GRB031203 host galaxy. (arXiv:1907.06175v1 [astro-ph.GA])
› Metadata Extraction from Raw Astroparticle Data of TAIGA Experiment. (arXiv:1907.06183v1 [astro-ph.IM])
› The Galactic magnetic field in the light of starburst-generated ultrahigh-energy cosmic rays. (arXiv:1907.06207v1 [astro-ph.HE])
› Dust destruction in non-radiative shocks. (arXiv:1907.06213v1 [astro-ph.GA])
› Quartic inflation and radiative corrections with non-minimal coupling. (arXiv:1907.06215v1 [astro-ph.CO])
› POEMMA (Probe of Extreme Multi-Messenger Astrophysics) design. (arXiv:1907.06217v1 [astro-ph.HE])
› Robust Archives Maximize Scientific Accessibility. (arXiv:1907.06234v1 [astro-ph.IM])
› Downward Terrestrial Gamma-ray Flash observed in Winter Thunderstorm. (arXiv:1907.06239v1 [physics.ao-ph])
› Observational constraints on the magnetic field of the bright transient Be/X-ray pulsar SXP 4.78. (arXiv:1907.06241v1 [astro-ph.HE])
› Vector Coherent Oscillation Dark Matter. (arXiv:1907.06243v1 [hep-ph])
› Extending light WIMP searches to single scintillation photons in LUX. (arXiv:1907.06272v1 [astro-ph.CO])
› Cosmology with galaxy-galaxy lensing on non-perturbative scales: Emulation method and application to BOSS LOWZ. (arXiv:1907.06293v1 [astro-ph.CO])
› The HST Large Programme on NGC 6752. III. Detection of the Peak of the White Dwarf Luminosity Function. (arXiv:1907.06300v1 [astro-ph.SR])
› The pros and cons of beyond standard model interpretations of ANITA events. (arXiv:1907.06308v1 [hep-ph])
› Assessing the photometric redshift precision of the S-PLUS survey: the Stripe-82 as a test-case. (arXiv:1907.06315v1 [astro-ph.GA])
› Astro2020 APC White Paper: Astronomy should be in the clouds. (arXiv:1907.06320v1 [astro-ph.IM])
› New nearby hypervelocity stars and their spatial distribution from Gaia DR2. (arXiv:1907.06348v1 [astro-ph.GA])
› Unified Dark Matter, Dark Energy and Baryogenesis via a "Cosmological Wetting Transition''. (arXiv:1907.06353v1 [hep-th])
› Quasi-static contraction during runaway gas accretion onto giant planets. (arXiv:1907.06362v1 [astro-ph.EP])
› Validating Planck SZ2 Clusters with Optical Counterparts. (arXiv:1907.06364v1 [astro-ph.CO])
› Magnetic helicity and eruptivity in active region 12673. (arXiv:1907.06365v1 [astro-ph.SR])
› Tracing the outer disk of NGC 300: An ultraviolet view. (arXiv:1907.06366v1 [astro-ph.GA])
› The initial mass-final luminosity relation of type II supernova progenitors. Hints of new physics?. (arXiv:1907.06367v1 [astro-ph.SR])
› Pulsar Timing Array Constraints on the Induced Gravitational Waves. (arXiv:1907.06372v1 [astro-ph.CO])
› PG 1610$+$062: a runaway B star challenging classical ejection mechanisms. (arXiv:1907.06375v1 [astro-ph.SR])
› Stellar atmospheric parameters for 754 spectra from the X-shooter Spectral Library. (arXiv:1907.06391v1 [astro-ph.SR])
› Record-breaking coronal magnetic field in solar active region 12673. (arXiv:1907.06398v1 [astro-ph.SR])
› Improved model-dependent corollary analyses after the first six annual cycles of DAMA/LIBRA-phase2. (arXiv:1907.06405v1 [hep-ph])
› A rotating fast bipolar wind and disk system around the B[e]-type star MWC 922. (arXiv:1907.06415v1 [astro-ph.SR])
› Resonance line in rotating accretion disc. (arXiv:1907.06416v1 [astro-ph.SR])
› A multi-wavelength study of the debris disc around 49 Cet. (arXiv:1907.06427v1 [astro-ph.EP])
› Observational limits on the X-ray emission from the bubble nebula surrounding Ho IX X-1. (arXiv:1907.06439v1 [astro-ph.HE])
› A Roadmap for Astrophysics and Cosmology with High-Redshift 21 cm Intensity Mapping. (arXiv:1907.06440v1 [astro-ph.IM])
› A convolutional neural network approach for reconstructing polarization information of photoelectric X-ray polarimeters. (arXiv:1907.06442v1 [astro-ph.IM])
› Radiation intensity and polarization from accretion discs with progressive increasing height. (arXiv:1907.06443v1 [astro-ph.SR])
› Final spin states of eccentric ocean planets. (arXiv:1907.06451v1 [astro-ph.EP])
› KM3NeT front-end and readout electronics system: hardware, firmware and software. (arXiv:1907.06453v1 [astro-ph.IM])
› Would the Sun's photosphere be negatively charged and magnetised ?. (arXiv:1907.06476v1 [astro-ph.SR])
› The Laser Interferometer Space Antenna: Unveiling the Millihertz Gravitational Wave Sky. (arXiv:1907.06482v1 [astro-ph.IM])
› CMB constraints on ultra-light primordial black holes with extended mass distributions. (arXiv:1907.06485v1 [astro-ph.CO])
› Reconstructing solar magnetic fields from historical observations V. Sunspot magnetic field measurements at Mount Wilson Observatory. (arXiv:1907.06492v1 [astro-ph.SR])
› Zinc isotope analyses of singularly small samples (
› The gas depletion factor in galaxy clusters: implication from Atacama Cosmology Telescope Polarization experiment measurements. (arXiv:1907.06509v1 [astro-ph.CO])
› StePar: an automatic code to infer stellar atmospheric parameters. (arXiv:1907.06512v1 [astro-ph.SR])
› Fuse and IUE Spectroscopy of the Prototype Dwarf Nova ER Ursa Majoris During Quiescence. (arXiv:1907.06513v1 [astro-ph.SR])
› Searches for Lorentz-Violating Signals with Astrophysical Polarization Measurements. (arXiv:1907.06514v1 [astro-ph.HE])
› Virtual European Solar & Planetary Access (VESPA): a Planetary Science Virtual Observatory cornerstone. (arXiv:1907.06521v1 [astro-ph.IM])
› Are most Cataclysmic Variables in Globular Clusters dynamically formed?. (arXiv:1907.06527v1 [astro-ph.GA])
› CosmoDC2: A Synthetic Sky Catalog for Dark Energy Science with LSST. (arXiv:1907.06530v1 [astro-ph.CO])
› Small-scale structure of primordial black hole dark matter and its implications for accretion. (arXiv:1907.06533v1 [astro-ph.CO])
› Kepler Object of Interest Network III. Kepler-82f: A new non-transiting $21 M_\bigoplus$ planet from photodynamical modelling. (arXiv:1907.06534v1 [astro-ph.EP])
› Noise spectral estimation methods and their impact on gravitational wave measurement of compact binary mergers. (arXiv:1907.06540v1 [gr-qc])
› Predictions for solar flares activity in solar cycle 25. (arXiv:1907.06545v1 [astro-ph.SR])
› Partitioning the universe into gravitational basins using the cosmic velocity field. (arXiv:1907.06555v1 [astro-ph.CO])
› Phases of Hadron-Quark Matter in (Proto) Neutron Stars. (arXiv:1907.06591v1 [nucl-th])
› Hot quark matter and (proto-) neutron stars. (arXiv:1907.06597v1 [nucl-th])
› Weighing neutrinos with the halo environment. (arXiv:1907.06598v1 [astro-ph.CO])
› Lens modelling of the strongly lensed Type Ia supernova iPTF16geu. (arXiv:1907.06609v1 [astro-ph.CO])
› Covariance matrices for galaxy cluster weak lensing: from virial regime to uncorrelated large-scale structure. (arXiv:1907.06611v1 [astro-ph.CO])
› The prevalence of repeating fast radio bursts. (arXiv:1907.06619v1 [astro-ph.HE])
› Distinguishing Between Stellar and Planetary Companions With Phase Monitoring. (arXiv:1205.5812v2 [astro-ph.EP] UPDATED)
› GMRT observations of IC 711 -- The longest head-tail radio galaxy known. (arXiv:1610.07783v2 [astro-ph.GA] UPDATED)
› Pseudo-Periodic Natural Higgs Inflation. (arXiv:1705.10276v2 [astro-ph.CO] UPDATED)
› Habitable Snowballs: Temperate Land Conditions, Liquid Water, and Implications for CO$_2$ Weathering. (arXiv:1803.00511v4 [astro-ph.EP] UPDATED)
› The Sloan Digital Sky Survey Reverberation Mapping Project: Accretion-Disk Sizes from Continuum Lags. (arXiv:1806.08360v2 [astro-ph.GA] UPDATED)
› The Equation of State of MH-III: a possible deep CH$_4$ reservoir in Titan, Super-Titan exoplanets and moons. (arXiv:1808.07925v3 [astro-ph.EP] UPDATED)
› Planck Mass Charged Gravitino Dark Matter. (arXiv:1809.01441v3 [hep-ph] UPDATED)
› Topological Gravity motivated by Renormalization Group. (arXiv:1809.02344v2 [hep-th] UPDATED)
› Explanation of Detailed Spectral Properties of FRBs by Axion Star Model. (arXiv:1810.07270v4 [astro-ph.HE] UPDATED)
› Tidal disruption events from massive black hole binaries: predictions for ongoing and future surveys. (arXiv:1811.01960v2 [astro-ph.GA] UPDATED)
› Decays of Long-Lived Relics and Their Signatures at IceCube. (arXiv:1811.04939v3 [hep-ph] UPDATED)
› (P)reheating after minimal Plateau Inflation and constraints from CMB. (arXiv:1811.11173v4 [astro-ph.CO] UPDATED)
› On the road to percent accuracy: nonlinear reaction of the matter power spectrum to dark energy and modified gravity. (arXiv:1812.05594v2 [astro-ph.CO] UPDATED)
› Gravitational Waves in the Presence of Viscosity. (arXiv:1901.00767v3 [gr-qc] UPDATED)
› Observation data pre-processing and scientific data products generation of POLAR. (arXiv:1901.00800v3 [astro-ph.IM] UPDATED)
› The time step constraint in radiation hydrodynamics. (arXiv:1901.06385v2 [astro-ph.SR] UPDATED)
› The Escape Fraction of Ionizing Photons During the Epoch of Reionization: observability with the Square Kilometre Array. (arXiv:1902.01611v2 [astro-ph.GA] UPDATED)
› Convolutional Neural Networks on the HEALPix sphere: a pixel-based algorithm and its application to CMB data analysis. (arXiv:1902.04083v2 [astro-ph.IM] UPDATED)
› Charged spherically symmetric black holes in $f(R)$ gravity and their stability analysis. (arXiv:1902.06783v4 [gr-qc] UPDATED)
› Dark sector interaction: a remedy of the tensions between CMB and LSS data. (arXiv:1903.04865v2 [astro-ph.CO] UPDATED)
› The impact of Stellar feedback from velocity-dependent ionised gas maps. -- A MUSE view of Haro 11. (arXiv:1903.11662v2 [astro-ph.GA] UPDATED)
› CMB Constraints on the Stochastic Gravitational-Wave Background at Mpc scales. (arXiv:1904.02115v2 [astro-ph.CO] UPDATED)
› The Optical to Mid-Infrared Extinction Law Based on the APOGEE, Gaia DR2, Pan-STARRS1, SDSS, APASS, 2MASS and WISE Surveys. (arXiv:1904.04575v3 [astro-ph.GA] UPDATED)
› Prompt optical emission as a signature of synchrotron radiation in gamma-ray bursts. (arXiv:1904.11086v2 [astro-ph.HE] UPDATED)
› Scaling laws for the oblique impact cratering on an inclined granular surface. (arXiv:1904.11636v2 [astro-ph.EP] UPDATED)
› High energy muons in extensive air showers. (arXiv:1904.12547v4 [hep-ph] UPDATED)
› The Quasar Main Sequence explained by the combination of Eddington ratio, metallicity and orientation. (arXiv:1905.01729v2 [astro-ph.HE] UPDATED)
› Turnaround size of non-spherical structures. (arXiv:1905.04263v2 [gr-qc] UPDATED)
› ExoMol Molecular linelists -- XXXIII. The spectrum of Titanium Oxide. (arXiv:1905.04587v2 [astro-ph.SR] UPDATED)
› Electron capture rates in $^{20}$Ne for a forbidden transition to the ground state of $^{20}$F relevant to final evolution of high density O-Ne-Mg cores. (arXiv:1905.10400v3 [astro-ph.SR] UPDATED)
› Neutron stars in general relativity and scalar-tensor theory of gravity. (arXiv:1905.10767v2 [gr-qc] UPDATED)
› Glancing Through Massive Binary Radio Lenses: Hardware-Aware Interferometry With 1-Bit Sensors. (arXiv:1905.12528v2 [astro-ph.IM] UPDATED)
› Insight-HXMT observations of Swift J0243.6+6124 during its 2017-2018 outburst. (arXiv:1906.01938v2 [astro-ph.HE] UPDATED)
› Spiral instabilities: Mechanism for recurrence. (arXiv:1906.04191v2 [astro-ph.GA] UPDATED)
› A comprehensive and uniform sample of broad-line active galactic nuclei from the SDSS DR7. (arXiv:1906.05597v2 [astro-ph.GA] UPDATED)
› Early Solar System $r$-process Abundances Limit Collapsar Origin. (arXiv:1906.07210v2 [astro-ph.HE] UPDATED)
› Is gravity getting weaker at low z? Observational evidence and theoretical implications. (arXiv:1907.03176v2 [astro-ph.CO] UPDATED)
› Monte-Carlo simulations of black hole mergers in AGN disks: Low $\chi_{\rm eff}$ mergers and predictions for LIGO. (arXiv:1907.04356v2 [astro-ph.HE] UPDATED)
› CosmicNet I: Physics-driven implementation of neural networks within Boltzmann-Einstein solvers. (arXiv:1907.05764v2 [astro-ph.CO] UPDATED)
› Euclid-era cosmology for everyone: Neural net assisted MCMC sampling for the joint 3x2 likelihood. (arXiv:1907.05881v2 [astro-ph.CO] UPDATED)
› On neutralization of charged black holes. (arXiv:1907.05239v1 [gr-qc] CROSS LISTED)

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