Latest preprints on astro-ph:

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› High resolution spectroscopy of the extended narrow-line region of IC 5063 and NGC 7212. (arXiv:1706.08970v1 [astro-ph.GA])
› Bayesian power-spectrum inference with foreground and target contamination treatment. (arXiv:1706.08971v1 [astro-ph.CO])
› Investigating Cluster Astrophysics and Cosmology with Cross-Correlation of the Thermal Sunyaev-Zel'dovich Effect and Weak Lensing. (arXiv:1706.08972v1 [astro-ph.CO])
› Hubble Space Telescope Proper Motion (HSTPROMO) Catalogs of Galactic Globular Clusters. V. The rapid rotation of 47 Tuc traced and modeled in three dimensions. (arXiv:1706.08974v1 [astro-ph.GA])
› Effect of dust radial drift on viscous evolution of gaseous disk. (arXiv:1706.08975v1 [astro-ph.EP])
› A Millimeter Continuum Size-Luminosity Relationship for Protoplanetary Disks. (arXiv:1706.08977v1 [astro-ph.EP])
› An Improved Age-Activity Relationship for Cool Stars older than a Gigayear. (arXiv:1706.08979v1 [astro-ph.SR])
› NuSTAR and XMM-Newton observations of the 2015 outburst decay of GX 339-4. (arXiv:1706.08980v1 [astro-ph.HE])
› General Relativistic Radiation Magnetohydrodynamic Simulations of Thin Magnetically Arrested Disks. (arXiv:1706.08982v1 [astro-ph.HE])
› Coronal Heating Topology: the Interplay of Current Sheets and Magnetic Field Lines. (arXiv:1706.08983v1 [astro-ph.SR])
› AGN feedback on molecular gas reservoirs in quasars at $z\sim2.4$. (arXiv:1706.08987v1 [astro-ph.GA])
› Early Blue Excess from the Type Ia Supernova 2017cbv and Implications for its Progenitor. (arXiv:1706.08990v1 [astro-ph.HE])
› Dissipation in a tidally perturbed body librating in longitude. (arXiv:1706.08999v1 [astro-ph.EP])
› Tidal viscosity of Enceladus. (arXiv:1706.09000v1 [astro-ph.EP])
› Primordial black holes from scalar field evolution in the early universe. (arXiv:1706.09003v1 [astro-ph.CO])
› Validating a novel angular power spectrum estimator using simulated low frequency radio-interferometric data. (arXiv:1706.09033v1 [astro-ph.CO])
› The AGN-Star Formation Connection: Future Prospects with JWST. (arXiv:1706.09056v1 [astro-ph.GA])
› First-principles Equation of State and Shock Compression Predictions of Warm Dense Hydrocarbons. (arXiv:1706.09073v1 [physics.plasm-ph])
› The Peculiar Globular Cluster Palomar 1 and Persistence in the SDSS-APOGEE Database. (arXiv:1706.09074v1 [astro-ph.GA])
› Magnetic Flux Cancelation as the Origin of Solar Quiet Region Pre-Jet Minifilaments. (arXiv:1706.09079v1 [astro-ph.SR])
› Analysis of solar gamma rays and solar neutrons detected on March 7th and September 25th of 2011 by Ground Level Neutron Telescopes, SEDA-FIB and FERMI-LAT. (arXiv:1706.09082v1 [astro-ph.HE])
› Can Turbulence Dominate Depolarization of Optical Blazars?. (arXiv:1706.09097v1 [astro-ph.HE])
› Application of Coupled Harmonic Oscillator model to Solar Activity and El Ni\~no Phenomena. (arXiv:1706.09105v1 [astro-ph.SR])
› Heating of an erupting prominence associated with a solar coronal mass ejection on 2012 January 27. (arXiv:1706.09116v1 [astro-ph.SR])
› A measurement of the Hubble constant using galaxy redshift surveys. (arXiv:1706.09149v1 [astro-ph.CO])
› Radial pulsations of red giant branch stars. (arXiv:1706.09166v1 [astro-ph.SR])
› Onset of a Large Ejective Solar Eruption from a Typical Coronal-Jet-Base Field Configuration. (arXiv:1706.09176v1 [astro-ph.SR])
› The application of the Quark-Hadron Chiral Parity-Doublet Model to neutron star matter. (arXiv:1706.09191v1 [nucl-th])
› Generating Log-normal Mock Catalog of Galaxies in Redshift Space. (arXiv:1706.09195v1 [astro-ph.CO])
› The complex magnetic field topology of the cool Ap star 49 Cam. (arXiv:1706.09196v1 [astro-ph.SR])
› Stability analysis of VBT Echelle spectrograph for precise radial velocity measurements. (arXiv:1706.09202v1 [astro-ph.IM])
› Shedding new light on the Crab with polarized X-rays. (arXiv:1706.09203v1 [astro-ph.HE])
› Asteroid mass estimation using Markov-chain Monte Carlo. (arXiv:1706.09208v1 [astro-ph.EP])
› Stellar laboratories. IX. New Se V, Sr IV - VII, Te VI, and I VI oscillator strengths and the Se, Sr, Te, and I abundances in the hot white dwarfs G191-B2B and RE 0503-289. (arXiv:1706.09215v1 [astro-ph.SR])
› Time-Dependent Cooling in Photoionized Plasma. (arXiv:1706.09220v1 [astro-ph.GA])
› Safely smoothing spacetime: backreaction in relativistic cosmological simulations. (arXiv:1706.09309v1 [astro-ph.CO])
› Traces of highest energy astrophysical muon and tau neutrinos in the Moon shadow. (arXiv:1706.09352v1 [astro-ph.HE])
› Dark Energy Survey Year 1 Results: Multi-Probe Methodology and Simulated Likelihood Analyses. (arXiv:1706.09359v1 [astro-ph.CO])
› Phase transition effects on the dynamical stability of hybrid neutron stars. (arXiv:1706.09371v1 [gr-qc])
› Towards a medium-scale axion helioscope and haloscope. (arXiv:1706.09378v1 [hep-ph])
› Weak gravitational lensing of finite beams. (arXiv:1706.09383v1 [gr-qc])
› The Factory and the Beehive III: PTFEB132.707+19.810, a Low-Mass Eclipsing Binary in Praesepe Observed by PTF and K2. (arXiv:1706.09390v1 [astro-ph.SR])
› Deforming regular black holes. (arXiv:1508.06701v3 [gr-qc] UPDATED)
› The Romulus Cosmological Simulations: A Physical Approach to the Formation, Dynamics and Accretion Models of SMBHs. (arXiv:1607.02151v4 [astro-ph.GA] UPDATED)
› Implications of the Occurrence of Glitches in Pulsar Free Precession Candidates. (arXiv:1610.03509v3 [astro-ph.HE] UPDATED)
› A New Measurement of the Spectral Lag of Gamma-Ray Bursts and its Implications for Spectral Evolution Behaviors. (arXiv:1610.07191v2 [astro-ph.HE] UPDATED)
› Detecting pulsars in the Galactic centre. (arXiv:1611.06977v2 [astro-ph.HE] UPDATED)
› Hints against the cold and collisionless nature of dark matter from the galaxy velocity function. (arXiv:1611.09362v3 [astro-ph.CO] UPDATED)
› Searching for Primordial Black Holes in the radio and X-ray sky. (arXiv:1612.00457v2 [astro-ph.HE] UPDATED)
› Forming short-period Wolf-Rayet X-ray binaries and double black holes through stable mass transfer. (arXiv:1701.02355v3 [astro-ph.SR] UPDATED)
› Observational evidence for high neutronization in supernova remnants: implications for Type Ia supernova progenitors. (arXiv:1701.07073v2 [astro-ph.HE] UPDATED)
› Enhanced interplanetary panspermia in the TRAPPIST-1 system. (arXiv:1703.00878v3 [astro-ph.EP] UPDATED)
› Higher Derivative Field Theories: Degeneracy Conditions and Classes. (arXiv:1703.01623v2 [hep-th] UPDATED)
› An algorithm for the reconstruction of high-energy neutrino-induced particle showers and its application to the ANTARES neutrino telescope. (arXiv:1703.02432v2 [astro-ph.HE] UPDATED)
› The first supermassive black holes. (arXiv:1703.03083v2 [astro-ph.GA] UPDATED)
› The GAPS Programme with HARPS-N@TNG XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets. (arXiv:1704.00373v2 [astro-ph.EP] UPDATED)
› Magnetic field line random walk in two-dimensional dynamical turbulence. (arXiv:1704.05059v2 [astro-ph.HE] UPDATED)
› Plasma Constraints on the Cosmological Abundance of Magnetic Monopoles and the Origin of Cosmic Magnetic Fields. (arXiv:1704.05094v2 [astro-ph.CO] UPDATED)
› Observational consequences of optical band milliarcsecond-scale structure in active galactic nuclei discovered by Gaia. (arXiv:1704.07365v2 [astro-ph.HE] UPDATED)
› Evolution of coexisting long and short period stellar activity cycles. (arXiv:1704.09009v2 [astro-ph.SR] UPDATED)
› Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I: Survey Description. (arXiv:1705.01606v3 [astro-ph.GA] UPDATED)
› 3D Relativistic MHD numerical simulations of X-shaped radio sources. (arXiv:1705.07799v2 [astro-ph.GA] UPDATED)
› Does information entropy play a role in the expansion and acceleration of the Universe?. (arXiv:1705.08945v2 [gr-qc] UPDATED)
› Understanding `galaxy groups' as a unique structure in the universe. (arXiv:1706.01916v2 [astro-ph.CO] UPDATED)
› Radiative Transfer for Exoplanet Atmospheres. (arXiv:1706.03188v2 [astro-ph.EP] UPDATED)
› The effect of stellar and AGN feedback on the low redshift Lyman-$\alpha$ forest in the Sherwood simulation suite. (arXiv:1706.04790v2 [astro-ph.CO] UPDATED)
› Inferring probabilistic stellar rotation periods using Gaussian processes. (arXiv:1706.05459v2 [astro-ph.SR] UPDATED)
› Microflare Heating of a Solar Active Region Observed with NuSTAR, Hinode/XRT, and SDO/AIA. (arXiv:1706.06108v2 [astro-ph.SR] UPDATED)
› Pulsations of a black hole in loop quantum gravity. (arXiv:1706.08009v2 [gr-qc] UPDATED)
› The Galaxy in circular polarization: all-sky radio prediction, detection strategy, and the charge of the leptonic cosmic rays. (arXiv:1706.08539v2 [astro-ph.HE] UPDATED)
› A solution of the dark energy and its coincidence problem based on local antigravity sources without fine-tuning or new scales. (arXiv:1706.08779v1 [gr-qc] CROSS LISTED)
› Compton Edge probing basic physics at Jefferson Laboratory: light speed isotropy and Lorentz invariance. (arXiv:1706.08907v1 [physics.acc-ph] CROSS LISTED)

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