output
19922026
most citedSciPy 1.0--Fundamental Algorithms for Scientific Computing in Python

40.2k citations

Showing 2019 · astro-ph.EPShow all

7 papers · 2 filters

astro-ph.EP2019★ 160 cited

Accretion of a giant planet onto a white dwarf

Boris T. Gaensicke, Matthias R. Schreiber, Odette Toloza +3

The detection of a dust disc around G29-38 and transits from debris orbiting WD1145+017 confirmed that the photospheric trace metals found in many white dwarfs arise from the accre…

astro-ph.EP2019★ 17 cited

Revisiting the cosmic-ray induced Venusian radiation dose in the context of habitability

Konstantin Herbst, Saša Banjac, Dimitra Atri +1

The Atmospheric Radiation Interaction Simulator (AtRIS) was used to model the altitude-dependent Venusian absorbed dose and the Venusian dose equivalent. For the first time, we mod…

astro-ph.EP2019★ 34 cited

A New Model Suite to Determine the Influence of Cosmic Rays on (Exo)planetary Atmospheric Biosignatures -- Validation based on Modern Earth

Konstantin Herbst, John Lee Grenfell, Miriam Sinnhuber +8

The first opportunity to detect indications for life outside the Solar System may be provided already within the next decade with upcoming missions such as the James Webb Space Tel…

astro-ph.EP2019★ 80 cited

Interpretation and diversity of exoplanetary material orbiting white dwarfs

Andrew Swan, Jay Farihi, Detlev Koester +5

Nine metal-polluted white dwarfs are observed with medium-resolution optical spectroscopy,where photospheric abundances are determined and interpreted through comparison against so…

astro-ph.EP2019★ 18 cited

Constraining the detectability of water ice in debris disks

Minjae Kim, Sebastian Wolf, Alexey Potapov +2

Water ice is important for the evolution and preservation of life. Identifying the distribution of water ice in debris disks is therefore of great interest in the field of astrobio…

astro-ph.EP2019★ 155 cited

The CARMENES search for exoplanets around M dwarfs. Two temperate Earth-mass planet candidates around Teegarden's Star

M. Zechmeister, S. Dreizler, I. Ribas +182

Context. Teegarden's Star is the brightest and one of the nearest ultra-cool dwarfs in the solar neighbourhood. For its late spectral type (M7.0V), the star shows relatively little…