Latest preprints on astro-ph:

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› Reverberation Mapping of Luminous Quasars at High-z. (arXiv:1806.08358v1 [astro-ph.GA])
› Significant Luminosity Differences of Two Twin Type Ia Supernovae. (arXiv:1806.08359v1 [astro-ph.HE])
› The Sloan Digital Sky Survey Reverberation Mapping Project: Accretion-Disk Sizes from Continuum Lags. (arXiv:1806.08360v1 [astro-ph.GA])
› Mining Gravitational-wave Catalogs To Understand Binary Stellar Evolution: A New Hierarchical Bayesian Framework. (arXiv:1806.08365v1 [astro-ph.HE])
› A Compact Multi-Planet System With A Significantly Misaligned Ultra Short Period Planet. (arXiv:1806.08368v1 [astro-ph.EP])
› Distant monsters: high redshift AGN predictions from a $\Lambda$CDM cosmological model. (arXiv:1806.08370v1 [astro-ph.GA])
› Novel constraints on non-cold (non-thermal) Dark Matter from Lyman-$\alpha$ forest data. (arXiv:1806.08371v1 [astro-ph.CO])
› The observable 21cm signal from reionization may be perturbative. (arXiv:1806.08372v1 [astro-ph.CO])
› The initial mass function in the Coma Berenices dwarf galaxy from deep near-infrared HST observations. (arXiv:1806.08380v1 [astro-ph.GA])
› Tidal Disruption Events and Gravitational Waves from Intermediate Mass Black Holes in Evolving Globular Clusters Across Space and Time. (arXiv:1806.08385v1 [astro-ph.GA])
› Revisiting the "forbidden" region: AGN radiative feedback with radiation trapping. (arXiv:1806.08387v1 [astro-ph.GA])
› Polar alignment of a protoplanetary disc around an eccentric binary II: Effect of binary and disc parameters. (arXiv:1806.08388v1 [astro-ph.EP])
› The New Horizons Kuiper Belt Extended Mission. (arXiv:1806.08393v1 [astro-ph.EP])
› Observations of the MIssing Baryons in the warm-hot intergalactic medium. (arXiv:1806.08395v1 [astro-ph.GA])
› The Next Generation Very Large Array: A Technical Overview. (arXiv:1806.08405v1 [astro-ph.IM])
› Galaxy pre-processing in substructures around z$\sim$0.4 galaxy clusters. (arXiv:1806.08435v1 [astro-ph.GA])
› X-ray Limits on the Progenitor System of the Type Ia Supernova 2017ejb. (arXiv:1806.08436v1 [astro-ph.HE])
› Flares from coalescing black holes in the centimeter-wavelength transient sky. (arXiv:1806.08446v1 [astro-ph.HE])
› OGLE-2017-BLG-0537: Microlensing Event with a Resolvable Lens in $\lesssim 5$ years from High-resolution Follow-up Observations. (arXiv:1806.08453v1 [astro-ph.SR])
› Spectral feature extraction for DB white dwarfs through machine learning applied to new discoveries in the SDSS DR12 and DR14. (arXiv:1806.08473v1 [astro-ph.SR])
› Optical Observations of the Young Type Ic Supernova SN 2014L in M99. (arXiv:1806.08477v1 [astro-ph.HE])
› Limitations of Pseudo-Newtonian approach in studying the accretion flow around Kerr black hole. (arXiv:1806.08481v1 [astro-ph.HE])
› Reconciling the Quasar Microlensing Disk Size Problem with a Wind Model of Active Galactic Nucleus. (arXiv:1806.08496v1 [astro-ph.HE])
› Dynamical Model of Binary Asteroid Systems Using Binary Octahedrons. (arXiv:1806.08524v1 [astro-ph.EP])
› The SPHERE view of Wolf-Rayet 104. (arXiv:1806.08525v1 [astro-ph.SR])
› Improving angular resolution of telescopes through probabilistic single-photon amplification?. (arXiv:1806.08528v1 [astro-ph.IM])
› Isotropic non-Gaussian $g_\mathrm{NL}$-like toy models that reproduce the Cosmic Microwave Background anomalies. (arXiv:1806.08531v1 [astro-ph.CO])
› A Model of Zebra Patterns in Solar Radio Emission. (arXiv:1806.08532v1 [astro-ph.SR])
› 2D solar wind speeds from 6 to 26 solar radii in solar cycle 24 by using Fourier filtering. (arXiv:1806.08540v1 [astro-ph.SR])
› The PAU Survey: star-galaxy classification with multi narrow-band data. (arXiv:1806.08545v1 [astro-ph.IM])
› FLARECAST: an I4.0 technology for space weather using satellite data. (arXiv:1806.08560v1 [astro-ph.IM])
› Synthetic C$^{18}$O observations of fibrous filaments: the problems of mapping from PPV to PPP. (arXiv:1806.08564v1 [astro-ph.GA])
› ALPino to ALP: Solution to Small-Scale Problems. (arXiv:1806.08569v1 [hep-ph])
› Modelling of the quasar main sequence in the optical plane. (arXiv:1806.08571v1 [astro-ph.HE])
› Winds Can "Blow Up" AGN Accretion Disk Sizes. (arXiv:1806.08575v1 [astro-ph.GA])
› Calibrating the system dynamics of LISA Pathfinder. (arXiv:1806.08581v1 [astro-ph.IM])
› Highly ionized Calcium and Argon X-ray spectra from a large solar flare. (arXiv:1806.08584v1 [astro-ph.SR])
› Variable Stars in Local Group Galaxies. IV. RR Lyrae stars in the central regions of the low-density galaxy Crater II. (arXiv:1806.08595v1 [astro-ph.GA])
› Young Blue Straggler Stars in the Galactic Field. (arXiv:1806.08605v1 [astro-ph.SR])
› Relations between physical observables: what is better?. (arXiv:1806.08611v1 [astro-ph.CO])
› A quantitative spectral analysis of 14 hypervelocity stars from the MMT survey. (arXiv:1806.08630v1 [astro-ph.SR])
› CLUMPY v3: $\gamma$-ray and $\nu$ signals from dark matter at all scales. (arXiv:1806.08639v1 [astro-ph.CO])
› Synthetic simulations of the extragalactic sky seen by eROSITA. I. Pre-launch selection functions from Monte-Carlo simulations. (arXiv:1806.08652v1 [astro-ph.CO])
› Interferometric Observations of the Quiet Sun at 20 and 25 MHz in May 2014. (arXiv:1806.08660v1 [astro-ph.SR])
› Two-dimensional hybrid simulations of filamentary structures and kinetic slow waves downstream of a quasi-parallel shock. (arXiv:1806.08669v1 [physics.space-ph])
› saturation effect on photoionization-driven broad absorption line variability. (arXiv:1806.08673v1 [astro-ph.GA])
› Unbiased constraints on reionization model parameters in presence of the foreground wedge. (arXiv:1806.08687v1 [astro-ph.CO])
› Resolution and accuracy of non-linear regression of PSF with artificial neural networks. (arXiv:1806.08689v1 [eess.IV])
› Bracketing the impact of astrophysical uncertainties on local dark matter searches. (arXiv:1806.08714v1 [hep-ph])
› Constraining the multiplicity statistics of the coolest brown dwarfs: binary fraction continues to decrease with spectral type. (arXiv:1806.08737v1 [astro-ph.SR])
› ESO telbib: learning from experience, preparing for the future. (arXiv:1806.08746v1 [astro-ph.IM])
› Line-driven ablation of circumstellar discs: III. Accounting for and analyzing the effects of continuum optical depth. (arXiv:1806.08753v1 [astro-ph.SR])
› The longest period transiting planet candidate from K2. (arXiv:1806.08757v1 [astro-ph.EP])
› Gauge Field and Fermion Production during Axion Inflation. (arXiv:1806.08769v1 [hep-ph])
› Modified Newtonian Mechanics from an interpolating metric. (arXiv:1601.00376v5 [astro-ph.CO] UPDATED)
› Scalar-multi-tensorial equivalence for higher order $f\left( R,\nabla_{\mu} R,\nabla_{\mu_{1}}\nabla_{\mu_{2}}R,...,\nabla_{\mu_{1}}...\nabla_{\mu_{n} }R\right)$ theories of gravity. (arXiv:1603.01563v3 [gr-qc] UPDATED)
› The Class of Jsolated Stars and Luminous Planetary Nebulae in old stellar populations. (arXiv:1704.05395v3 [astro-ph.SR] UPDATED)
› Measuring the reionization 21 cm fluctuations using clustering wedges. (arXiv:1708.02824v2 [astro-ph.CO] UPDATED)
› Comparing dark energy models with current observational data. (arXiv:1708.03143v3 [astro-ph.CO] UPDATED)
› Tests of Catastrophic Outlier Prediction in Empirical Photometric Redshift Estimation with Redshift Probability Distributions. (arXiv:1709.01576v3 [astro-ph.GA] UPDATED)
› On the Optimal Choice of Nucleosynthetic Yields, IMF and Number of SNe Ia for Chemical Evolution Modelling. (arXiv:1712.05686v2 [astro-ph.GA] UPDATED)
› The rate of Type-Ia supernovae in galaxy clusters and the delay-time distribution out to redshift 1.75. (arXiv:1803.04421v3 [astro-ph.GA] UPDATED)
› A machine learning method to separate cosmic ray electrons from protons from 10 to 100 GeV using DAMPE data. (arXiv:1803.06628v2 [astro-ph.IM] UPDATED)
› ASASSN-15nx: A luminous Type II supernova with a "perfect" linear decline. (arXiv:1804.00025v2 [astro-ph.HE] UPDATED)
› Odd-parity stability of hairy black holes in $U(1)$ gauge-invariant scalar-vector-tensor theories. (arXiv:1804.00535v2 [gr-qc] UPDATED)
› Solar wind interaction with the Martian upper atmosphere: Roles of the cold thermosphere and hot oxygen corona. (arXiv:1804.00937v2 [astro-ph.EP] UPDATED)
› A compact and light-weight refractive telescope for the observation of extensive air showers. (arXiv:1804.01781v2 [astro-ph.IM] UPDATED)
› New Interpretation of the mass-temperature relation and mass calibration of galaxy clusters based on the fundamental plane. (arXiv:1804.05070v2 [astro-ph.GA] UPDATED)
› The hour-timescale GeV flares of PSR B1259-63 in 2017. (arXiv:1804.09861v2 [astro-ph.HE] UPDATED)
› Radiative Charge Transfer Between the Helium Ion and Argon. (arXiv:1804.10108v2 [astro-ph.GA] UPDATED)
› Primeval very low-mass stars and brown dwarfs - III. The halo transitional brown dwarfs. (arXiv:1805.08033v2 [astro-ph.SR] UPDATED)
› Numerical simulations of black hole accretion flows. (arXiv:1805.11305v2 [astro-ph.HE] UPDATED)
› The structure of detonation waves in supernovae revisited. (arXiv:1806.01286v2 [astro-ph.HE] UPDATED)
› An analytical template for gravitational-wave echoes: signal characterization and prospects of detection with current and future interferometers. (arXiv:1806.04253v2 [gr-qc] UPDATED)
› Formation of S0 galaxies through mergers. Morphological properties: tidal relics, lenses, ovals, and other inner components. (arXiv:1806.06070v2 [astro-ph.GA] UPDATED)
› Comparing the emission spectra of U and Th hollow cathode lamps and a new U line-list. (arXiv:1806.07361v3 [astro-ph.IM] UPDATED)
› The importance of binarity in the formation and evolution of planetary nebulae. (arXiv:1806.08244v2 [astro-ph.SR] UPDATED)

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