Najnowsze prace na astro-ph:

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› Internal Structure and CO$_2$ Reservoirs of Habitable Water-Worlds. (arXiv:1904.10458v1 [astro-ph.EP])
› Ionization bias and the ghost proximity effect near $z\gtrsim6$ quasars in the shadow of proximate absorption systems. (arXiv:1904.10459v1 [astro-ph.CO])
› The effect of tides on the Sculptor dwarf spheroidal galaxy. (arXiv:1904.10461v1 [astro-ph.GA])
› The stellar host in star-forming low-mass galaxies: Evidence for two classes. (arXiv:1904.10462v1 [astro-ph.GA])
› $\mathtt{bimEX}$: A Mathematica package for exact computations in 3$+$1 bimetric relativity. (arXiv:1904.10464v1 [cs.SC])
› Survey of Gravitationally-lensed Objects in HSC Imaging (SuGOHI). III. Statistical strong lensing constraints on the stellar IMF of CMASS galaxies. (arXiv:1904.10465v1 [astro-ph.GA])
› JINGLE, a JCMT legacy survey of dust and gas for galaxy evolution studies: II. SCUBA-2 850 {\mu}m data reduction and dust flux density catalogues. (arXiv:1904.10466v1 [astro-ph.GA])
› The Boundary Between Gas-rich and Gas-poor Planets. (arXiv:1904.10470v1 [astro-ph.EP])
› MIND THE GAP: The Too Big To Fail Problem Resolved. (arXiv:1904.10471v1 [astro-ph.GA])
› Atmospheres and UV Environments of Earth-like Planets Throughout Post-Main Sequence Evolution. (arXiv:1904.10474v1 [astro-ph.EP])
› Gravitational waves from fermion production during axion inflation. (arXiv:1904.10483v1 [astro-ph.CO])
› TurbuStat: Turbulence Statistics in Python. (arXiv:1904.10484v1 [astro-ph.IM])
› Gamma-Ray Bursts: Theoretical Issues and Developments. (arXiv:1904.10488v1 [astro-ph.HE])
› The Masses of Supernova Remnant Progenitors in M83. (arXiv:1904.10490v1 [astro-ph.GA])
› Modelling the radiation pattern of a dual circular polarization system. (arXiv:1904.10496v1 [astro-ph.IM])
› Large Scale Structure in CHILES. (arXiv:1904.10511v1 [astro-ph.GA])
› Correlations between supermassive black holes, hot atmospheres, and the total masses of early type galaxies. (arXiv:1904.10513v1 [astro-ph.GA])
› A Fast and Accurate Algorithm for Spherical Harmonic Analysis of the Cosmic Microwave Background Radiation. (arXiv:1904.10514v1 [math.NA])
› Accounting for Correlations When Fitting Extra Cosmological Parameters. (arXiv:1904.10521v1 [astro-ph.CO])
› Upper Limits on Very-High-Energy Gamma-ray Emission from Core-Collapse Supernovae Observed with H.E.S.S. (arXiv:1904.10526v1 [astro-ph.HE])
› Six Years of Sustained Activity from Active Asteroid (6478) Gault. (arXiv:1904.10530v1 [astro-ph.EP])
› Diversity in density profiles of self-interacting dark matter satellite halos. (arXiv:1904.10539v1 [astro-ph.GA])
› Developments in Cosmic Growth and Gravitation. (arXiv:1904.10544v1 [astro-ph.CO])
› Chandra and Hubble Space Telescope observations of dark gamma-ray bursts and their host galaxies. (arXiv:1904.10549v1 [astro-ph.GA])
› Cold, old and metal-poor: New stellar substructures in the Milky Way's dwarf spheroidals. (arXiv:1904.10560v1 [astro-ph.GA])
› Rate of dark photon emission from electron positron annihilation in massive stars. (arXiv:1904.10567v1 [hep-ph])
› The tidal disruption event AT2017eqx: spectroscopic evolution from hydrogen rich to poor suggests an atmosphere and outflow. (arXiv:1904.10571v1 [astro-ph.HE])
› First Abundance Measurement of Organic Molecules in the Atmosphere of HH 212 Protostellar Disk. (arXiv:1904.10572v1 [astro-ph.GA])
› Is Gravity the Weakest Force?. (arXiv:1904.10577v1 [hep-th])
› Radial Velocities, Space Motions, and Nearby Young Moving Group Memberships of Eleven Candidate Young Brown Dwarfs. (arXiv:1904.10579v1 [astro-ph.SR])
› TRAO Survey of Nearby Filamentary Molecular clouds, the Universal Nursery of Stars (TRAO FUNS) I. Dynamics and Chemistry of L1478 in the California Molecular Cloud. (arXiv:1904.10594v1 [astro-ph.GA])
› No Evidence for Lunar Transit in New Analysis of HST Observations of the Kepler-1625 System. (arXiv:1904.10618v1 [astro-ph.EP])
› Electron and positron spectra in the three dimensional spatial-dependent propagation model. (arXiv:1904.10663v1 [astro-ph.HE])
› Volume uncertainty assessment method of asteroid models from disk-integrated visual photometry. (arXiv:1904.10676v1 [astro-ph.EP])
› Spectropolarimetric analysis of an active region filament. II. Evidence of the limitations of a single component model. (arXiv:1904.10688v1 [astro-ph.SR])
› Unveiling molecular clouds toward bipolar HII region G8.14+0.23. (arXiv:1904.10708v1 [astro-ph.GA])
› Self-consistent band calculation of slab phase in neutron-star crust. (arXiv:1904.10712v1 [nucl-th])
› Confronting expansion distances of planetary nebulae with Gaia DR2 measurements. (arXiv:1904.10721v1 [astro-ph.SR])
› Analysis and test of the central-blue-spot infall hallmark. (arXiv:1904.10737v1 [astro-ph.SR])
› High-resolution spectroscopic analysis of a large sample of Li-rich giants found by LAMOST. (arXiv:1904.10738v1 [astro-ph.SR])
› Structure and evolution of the photospheric magnetic field in 2010 - 2017: comparison of SOLIS/VSM vector field and $B_{LOS}$ potential field. (arXiv:1904.10740v1 [physics.space-ph])
› Exponentially Decaying Extended Emissions Following Short Gamma-Ray Bursts with Possible Luminosity -- E-folding Time Correlation. (arXiv:1904.10775v1 [astro-ph.HE])
› How do scalar-field dark matter haloes react to orbiting bodies?. (arXiv:1904.10777v1 [gr-qc])
› SDSS-IV/SPIDERS: A Catalogue of X-Ray Selected AGN Properties; Spectral Properties and Black Hole Mass Estimates for SPIDERS SDSS DR14 Type 1 AGN. (arXiv:1904.10780v1 [astro-ph.HE])
› CoRoT: The First Space-Based Transit Survey to Explore the Close-in Planet Population. (arXiv:1904.10793v1 [astro-ph.EP])
› Extracting the Global Signal from 21-cm Fluctuations: the Multi-Tracer Approach. (arXiv:1904.10857v1 [astro-ph.CO])
› Asymmetric distribution of weak photospheric magnetic field values. (arXiv:1904.10866v1 [astro-ph.SR])
› Episodic Jets from Black Hole Accretion Disks. (arXiv:1904.10870v1 [astro-ph.HE])
› Globular cluster candidates in the Galactic bulge: Gaia and VVV view of the latest discoveries. (arXiv:1904.10872v1 [astro-ph.GA])
› Accuracy Requirements for Empirically-Measured Selection Functions. (arXiv:1904.10879v1 [astro-ph.IM])
› Sulfur Chemistry in L1157-B1. (arXiv:1904.10895v1 [astro-ph.GA])
› Shallow Ultraviolet Transits of WD 1145+017. (arXiv:1904.10896v1 [astro-ph.EP])
› Spectral Variability of a Sample of Extreme Variability Quasars and Implications for the MgII Broad-line Region. (arXiv:1904.10912v1 [astro-ph.GA])
› Studying star-forming processes towards G29.862-0.044. (arXiv:1904.10914v1 [astro-ph.GA])
› $\gamma$-ray and $\nu$ searches for dark matter subhalos in the Milky Way with a baryonic potential. (arXiv:1904.10935v1 [astro-ph.HE])
› An extensive grid of DARWIN models for M-type AGB stars I. Mass-loss rates and other properties of dust-driven winds. (arXiv:1904.10943v1 [astro-ph.SR])
› Buried Black Hole Growth in IR-selected Mergers: New Results from Chandra. (arXiv:1904.10955v1 [astro-ph.GA])
› R-mode instability in compact stars. (arXiv:1904.10957v1 [astro-ph.HE])
› Resummed Photon Spectra for WIMP Annihilation. (arXiv:1712.07656v3 [hep-ph] UPDATED)
› X-ray properties of high-richness CAMIRA clusters in the Hyper Suprime-Cam Subaru Strategic Program field. (arXiv:1802.08692v2 [astro-ph.CO] UPDATED)
› Precision Photon Spectra for Wino Annihilation. (arXiv:1808.08956v2 [hep-ph] UPDATED)
› Photometric Redshift Calibration Requirements for WFIRST Weak Lensing Cosmology: Predictions from CANDELS. (arXiv:1808.10458v2 [astro-ph.GA] UPDATED)
› Ultrahigh energy cosmic rays and neutrinos from light nuclei composition. (arXiv:1809.05321v3 [astro-ph.HE] UPDATED)
› Analytical Black-Hole Binary Merger Waveforms. (arXiv:1810.00040v2 [gr-qc] UPDATED)
› CLOUDY view of the warm corona. (arXiv:1901.02962v2 [astro-ph.HE] UPDATED)
› On the Elevation and Suppression of Star Formation within Galaxies. (arXiv:1901.10276v2 [astro-ph.GA] UPDATED)
› Probing the Fundamental Nature of Dark Matter with the Large Synoptic Survey Telescope. (arXiv:1902.01055v2 [astro-ph.CO] UPDATED)
› On the Orbital Decay of Globular Clusters in NGC1052-DF2: Testing a Baryon-Only Mass Model. (arXiv:1902.05959v2 [astro-ph.GA] UPDATED)
› Isocurvature bounds on axion-like particle dark matter in the post-inflationary scenario. (arXiv:1903.06194v2 [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:1904.04575v2 [astro-ph.GA] UPDATED)
› Imprint of a scalar era on the primordial spectrum of gravitational waves. (arXiv:1904.07870v2 [hep-ph] UPDATED)
› Confirming interstellar C$_{60}^+$ using the Hubble Space Telescope. (arXiv:1904.08821v2 [astro-ph.GA] UPDATED)
› Search for sub-solar mass ultracompact binaries in Advanced LIGO's second observing run. (arXiv:1904.08976v2 [astro-ph.CO] UPDATED)
› Analytic computation of the secular effects of encounters on a binary: features arising from second-order perturbation theory. (arXiv:1904.09624v2 [astro-ph.SR] UPDATED)
› The Scalar Hexaquark $uuddss$: a Candidate for Dark Matter?. (arXiv:1904.09913v2 [hep-ph] UPDATED)

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