Latest preprints on astro-ph:

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› From quarks to nucleons in dark matter direct detection. (arXiv:1707.06998v1 [hep-ph])
› Magnetic Inflation and Stellar Mass I: Revised Parameters for the Component Stars of the Kepler Low-mass Eclipsing Binary T-Cyg1-12664. (arXiv:1707.07001v1 [astro-ph.SR])
› Witnessing galaxy assembly in an extended z~3 structure. (arXiv:1707.07003v1 [astro-ph.GA])
› Gas Content and Kinematics in Clumpy, Turbulent Star-forming Disks. (arXiv:1707.07005v1 [astro-ph.GA])
› Reduced Diversity of Life Around Proxima Centauri and TRAPPIST-1. (arXiv:1707.07007v1 [astro-ph.EP])
› How To Model Supernovae in Simulations of Star and Galaxy Formation. (arXiv:1707.07010v1 [astro-ph.GA])
› Pulsar Wind Blowout from a Supernova. (arXiv:1707.07021v1 [astro-ph.HE])
› Observable Emission Features of Black Hole GRMHD Jets on Event Horizon Scales. (arXiv:1707.07023v1 [astro-ph.HE])
› Optical/Near-IR spatially resolved study of the H II galaxy Tol 02. (arXiv:1707.07025v1 [astro-ph.GA])
› The real population of star clusters in the bar of the Large Magellanic Cloud. (arXiv:1707.07032v1 [astro-ph.GA])
› Shocks and cold fronts in merging galaxy clusters: new detections with Chandra. (arXiv:1707.07038v1 [astro-ph.HE])
› Exomoon Habitability and Tidal Evolution in Low-Mass Star Systems. (arXiv:1707.07040v1 [astro-ph.EP])
› Nonlinear transverse cascade and sustenance of MRI-turbulence in Keplerian disks with an azimuthal magnetic field. (arXiv:1707.07044v1 [astro-ph.EP])
› Using CMB spectral distortions to distinguish between dark matter solutions to the small-scale crisis. (arXiv:1707.07050v1 [astro-ph.CO])
› Solar twins and the Barium puzzle. (arXiv:1707.07051v1 [astro-ph.SR])
› An explanation of remarkable emission line profiles in post-flare coronal rain. (arXiv:1707.07069v1 [astro-ph.SR])
› Are all flare ribbons simply connected to the corona?. (arXiv:1707.07072v1 [astro-ph.SR])
› On the Fine Structure Splitting of the 3p43d 4D5/2 and 3p43d 4D7/2 Levels of Fe X. (arXiv:1707.07077v1 [astro-ph.SR])
› Acceleration of Cosmic Ray Electrons at Weak Shocks in Galaxy Clusters. (arXiv:1707.07085v1 [astro-ph.HE])
› Atomic physics and modern solar spectro-polarimetry. (arXiv:1707.07090v1 [astro-ph.IM])
› HATS-43b, HATS-44b, HATS-45b, and HATS-46b: Four Short Period Transiting Giant Planets in the Neptune-Jupiter Mass Range. (arXiv:1707.07093v1 [astro-ph.EP])
› Intrapixel effects of CCD and CMOS detectors. (arXiv:1707.07106v1 [astro-ph.IM])
› Active Galactic Nuclei: what's in a name?. (arXiv:1707.07134v1 [astro-ph.GA])
› On the use of the autonomous Birkhoff equations in Lie series perturbation theory. (arXiv:1707.07138v1 [astro-ph.EP])
› Planet formation and disk-planet interactions. (arXiv:1707.07148v1 [astro-ph.EP])
› VLA observations of the disk around the young brown dwarf 2MASS J044427+2512. (arXiv:1707.07197v1 [astro-ph.EP])
› Linear feature detection algorithm for astronomical surveys - II. Defocusing effects on meteor tracks. (arXiv:1707.07223v1 [astro-ph.EP])
› A novel strategy to seek bio-signatures at Enceladus and Europa. (arXiv:1707.07230v1 [astro-ph.EP])
› Consistent dust and gas models for protoplanetary disks: II. Chemical networks and rates. (arXiv:1707.07281v1 [astro-ph.SR])
› Identification of Young Stellar Variables with KELT for K2 II: The Upper Scorpius Association. (arXiv:1707.07313v1 [astro-ph.SR])
› Discovering New Variable Stars at Key Stage 3. (arXiv:1707.07337v1 [physics.ed-ph])
› General relativistic radiation magnetohydrodynamics simulations of supercritical accretion onto magnetized neutron star; -modeling of ultra luminous x-ray pulsars. (arXiv:1707.07356v1 [astro-ph.HE])
› Star Formation of Merging Disk Galaxies with AGN Feedback Effects. (arXiv:1707.07382v1 [astro-ph.GA])
› Energy Conditions in Modified $f(G)$ Gravity. (arXiv:1707.07386v1 [gr-qc])
› Merging of a CO WD and a He-rich white dwarf to produce a type Ia supernovae. (arXiv:1707.07387v1 [astro-ph.SR])
› Extrasolar Planets and Their Host Stars. (arXiv:1707.07405v1 [astro-ph.EP])
› New 50-m-class single-dish telescope: Large Submillimeter Telescope (LST). (arXiv:1707.07407v1 [astro-ph.IM])
› On the Origin of the 3.3 Micron Unidentified Infrared Emission Feature. (arXiv:1707.07415v1 [astro-ph.GA])
› Timing of AB And eclipses. (arXiv:1707.07430v1 [astro-ph.SR])
› Detection of CH+, SH+, and their 13C- and 34S- isotopologues toward PKS1830-211. (arXiv:1707.07446v1 [astro-ph.GA])
› Origin of the Galactic Halo: accretion vs. in situ formation. (arXiv:1707.07450v1 [astro-ph.GA])
› Chemical element transport in stellar evolution models. (arXiv:1707.07454v1 [astro-ph.SR])
› VLBA imaging of the 3mm SiO maser emission in the disk-wind from the massive protostellar system Orion Source I. (arXiv:1707.07455v1 [astro-ph.GA])
› Pulsar Glitches in a Strangeon Star Model. (arXiv:1707.07471v1 [astro-ph.HE])
› Metallicity effect on stellar granulation detected from oscillating red giants in open clusters. (arXiv:1707.07474v1 [astro-ph.SR])
› Accelerating Approximate Bayesian Computation with Quantile Regression: Application to Cosmological Redshift Distributions. (arXiv:1707.07498v1 [astro-ph.CO])
› Shape and spin determination of Barbarian asteroids. (arXiv:1707.07503v1 [astro-ph.EP])
› Estimation of mass outflow rates from dissipative accretion disc around rotating black holes. (arXiv:1707.07511v1 [astro-ph.HE])
› The faint radio sky: VLBA observations of the COSMOS field. (arXiv:1707.07512v1 [astro-ph.GA])
› The EBLM Project IV. Spectroscopic orbits of over 100 eclipsing M dwarfs masquerading as transiting hot-Jupiters. (arXiv:1707.07521v1 [astro-ph.SR])
› The ionising effect of low energy cosmic rays from a class II object on its protoplanetary disk. (arXiv:1707.07522v1 [astro-ph.SR])
› Classifications of Twin Star Solutions for a Constant Speed of Sound Parameterized Equation of State. (arXiv:1707.07524v1 [astro-ph.HE])
› Probing supervoids with weak lensing. (arXiv:1707.07535v1 [astro-ph.CO])
› Does Viscosity turn inflation into the CMB and $\Lambda$. (arXiv:1707.07566v1 [gr-qc])
› Propagating mass accretion rate fluctuations in X-ray binaries under the influence of viscous diffusion. (arXiv:1707.07578v1 [astro-ph.HE])
› Metal enrichment signatures of the first stars on high-z DLAs. (arXiv:1707.07580v1 [astro-ph.GA])
› Closing remarks and Outlook. (arXiv:1707.07602v1 [astro-ph.GA])
› Millimetre-wave Emission from an Intermediate-Mass Black Hole Candidate in the Milky Way. (arXiv:1707.07603v1 [astro-ph.GA])
› The spatial distribution of carbon dust in the early solar nebula and the carbon content of planetesimals. (arXiv:1707.07611v1 [astro-ph.EP])
› Local properties and global structure of McVittie spacetimes with non-flat FLRW backgrounds. (arXiv:1707.07612v1 [gr-qc])
› Nuclear absorption and emission in the AGN merger NGC 6240: the hard X-ray view. (arXiv:1707.07613v1 [astro-ph.HE])
› The Carnegie Supernova Project I: analysis of stripped-envelope supernova light curves. (arXiv:1707.07614v1 [astro-ph.HE])
› The Carnegie Supernova Project I: methods to estimate host-galaxy reddening of stripped-envelope supernovae. (arXiv:1707.07615v1 [astro-ph.HE])
› The Carnegie Supernova Project I: photometry data release of low-redshift stripped-envelope supernovae. (arXiv:1707.07616v1 [astro-ph.HE])
› Validation of the in-flight calibration procedures for the MICROSCOPE space mission. (arXiv:1707.07630v1 [astro-ph.IM])
› No large population of unbound or wide-orbit Jupiter-mass planets. (arXiv:1707.07634v1 [astro-ph.EP])
› Cosmological parameter forecasts for HI intensity mapping experiments using the angular power spectrum. (arXiv:1707.07647v1 [astro-ph.CO])
› Developing a Method to Determine Electrical Conductivity in Meteoritic Materials with Applications to Induction Heating Theory (2008 Student Thesis). (arXiv:1707.07648v1 [astro-ph.EP])
› Probing the imprints of generalized interacting dark energy on the growth of perturbations. (arXiv:1707.07667v1 [astro-ph.CO])
› Unlocking Sensitivity for Visibility-based Estimators of the 21 cm Reionization Power Spectrum. (arXiv:1707.07668v1 [astro-ph.IM])
› Light propagation in the gravitational field of N arbitrarily moving bodies in 1PN approximation for high-precision astrometry. (arXiv:1509.07279v4 [astro-ph.IM] UPDATED)
› Phenomenology in minimal theory of massive gravity. (arXiv:1512.04008v2 [hep-th] UPDATED)
› SpECTRE: A Task-based Discontinuous Galerkin Code for Relativistic Astrophysics. (arXiv:1609.00098v2 [astro-ph.HE] UPDATED)
› Variations between Dust and Gas in the Diffuse Interstellar Medium. 2. Search for Cold Gas. (arXiv:1611.04475v2 [astro-ph.GA] UPDATED)
› Primordial black holes from supersymmetry in the early universe. (arXiv:1612.02529v3 [astro-ph.CO] UPDATED)
› A robust mass estimator for dark matter subhalo perturbations in strong gravitational lenses. (arXiv:1612.05250v2 [astro-ph.GA] UPDATED)
› Measurement of Hubble constant with stellar-mass binary black holes. (arXiv:1612.06060v2 [astro-ph.CO] UPDATED)
› Neutron stars structure in the context of massive gravity. (arXiv:1701.01039v2 [gr-qc] UPDATED)
› Non-convex optimization for self-calibration of direction-dependent effects in radio interferometric imaging. (arXiv:1701.03689v2 [astro-ph.IM] UPDATED)
› Manybody aspects of gravity in compact stars. (arXiv:1701.06189v2 [gr-qc] UPDATED)
› Flux Accretion and Coronal Mass Ejection Dynamics. (arXiv:1701.09082v2 [astro-ph.SR] UPDATED)
› 3FHL: The Third Catalog of Hard Fermi-LAT Sources. (arXiv:1702.00664v3 [astro-ph.HE] UPDATED)
› $\textit{Siriusly}$, a newly identified intermediate-age Milky Way stellar cluster: A spectroscopic study of $\textit{Gaia}$ 1. (arXiv:1703.03823v3 [astro-ph.GA] UPDATED)
› Perturbation Theory for BAO reconstructed fields: one-loop results in real-space matter density field. (arXiv:1703.07878v2 [astro-ph.CO] UPDATED)
› Light axion-like dark matter must be present during inflation. (arXiv:1703.08798v2 [astro-ph.CO] UPDATED)
› Tests of Gravity Theories Using Supermassive Black Holes. (arXiv:1704.02425v2 [astro-ph.CO] UPDATED)
› Magnetized Reverse Shock: Density-fluctuation-induced Field Distortion, Polarization Degree Reduction, and Application to GRBs. (arXiv:1704.03468v2 [astro-ph.HE] UPDATED)
› Winds and radiation in unison: a new semi-analytic feedback model for cloud dissolution. (arXiv:1704.04240v2 [astro-ph.GA] UPDATED)
› Black hole ringdown echoes and howls. (arXiv:1704.07175v3 [gr-qc] UPDATED)
› Gentle heating by mixing in cooling flow clusters. (arXiv:1704.07797v2 [astro-ph.GA] UPDATED)
› Cosmological constraints from a joint analysis of cosmic growth and expansion. (arXiv:1705.07903v2 [astro-ph.CO] UPDATED)
› Climbing the cosmic ladder with stellar twins in RAVE with Gaia. (arXiv:1705.11049v2 [astro-ph.SR] UPDATED)
› Near-Infrared Variability Study of the Central 2.3 arcmin x 2.3 arcmin of the Galactic Centre I. Catalog of Variable Sources. (arXiv:1706.03243v2 [astro-ph.GA] UPDATED)
› Near-Infrared Variability Study of the Central 2.3 arcmin x 2.3 arcmin of the Galactic Centre II. Identification of RR Lyrae Stars in the Milky Way Nuclear Star Cluster. (arXiv:1706.03299v2 [astro-ph.GA] UPDATED)
› Detection of X-ray spectral state transitions in mini-outbursts of black hole transient GRS 1739-278. (arXiv:1706.06472v2 [astro-ph.HE] UPDATED)
› Gravitational effects of condensed dark matter on strange stars. (arXiv:1706.07272v2 [gr-qc] UPDATED)
› Mapping the hot gas temperature in galaxy clusters using X-ray and Sunyaev-Zel'dovich imaging. (arXiv:1706.10230v2 [astro-ph.CO] UPDATED)
› Constraints on cometary surface evolution derived from a statistical analysis of 67P's topography. (arXiv:1707.00734v2 [astro-ph.EP] UPDATED)
› Galaxy evolution in merging clusters: The passive core of the "Train Wreck" cluster of galaxies, A520. (arXiv:1707.03208v2 [astro-ph.GA] UPDATED)
› Big Bang Nucleosynthesis with Stable $^8$Be and the Primordial Lithium Problem. (arXiv:1707.03852v2 [astro-ph.CO] UPDATED)
› The "Folk Theorem" on Effective Field Theory: How Does It Fare in Nuclear Physics?. (arXiv:1707.04857v2 [nucl-th] UPDATED)
› CHEERS: The chemical evolution RGS sample. (arXiv:1707.05076v2 [astro-ph.GA] UPDATED)
› Penitentes as the origin of the bladed terrain of Tartarus Dorsa, Pluto. (arXiv:1707.06670v2 [astro-ph.EP] UPDATED)
› Detection of radio emission from the gamma-ray pulsar J1732-3131 at 327 MHz. (arXiv:1706.08613v1 [astro-ph.HE] CROSS LISTED)

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