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

40.2k citations

Showing 2015 · astro-ph.EPShow all

18 papers · 2 filters

astro-ph.EP2015★ 22 cited

Inferring heat recirculation and albedo for exoplanetary atmospheres: Comparing optical phase curves and secondary eclipse data

P. von Paris, P. Gratier, P. Bordé +1

Basic atmospheric properties such as albedo and heat redistribution between day and nightside have been inferred for a number of planets using observations of secondary eclipses an…

astro-ph.EP2015★ 21 cited

2D photochemical modeling of Saturn's stratosphere. Part II: Feedback between composition and temperature

V. Hue, T. K. Greathouse, T. Cavalié +2

Saturn's axial tilt produces seasons in a similar way as on Earth. Both the stratospheric temperature and composition are affected by this latitudinally varying insolation along th…

astro-ph.EP2015

Ethyl alcohol and sugar in comet C/2014Q2 (Lovejoy)

Nicolas Biver, Dominique Bockelée-Morvan, Raphaël Moreno +7

The presence of numerous complex organic molecules (COMs; defined as those containing six or more atoms) around protostars shows that star formation is accompanied by an increase o…

astro-ph.EP2015★ 23 cited

Radar scattering of linear dunes and mega-yardangs: Application to Titan

Philippe Paillou, Benoît Seignovert, Jani Radebaugh +1

The Ku-band (13.8 GHz - 2.2 cm) RADAR instrument onboard the Cassini-Huygens spacecraft has revealed the richness of the surface of Titan, as numerous seas, lakes, rivers, cryo-vol…

astro-ph.EP2015★ 42 cited

Fast migration of low-mass planets in radiative discs

Arnaud Pierens

Low-mass planets are known to undergo Type I migration and this process must have played a key role during the evolution of planetary systems. Analytical formulae for the disc torq…

astro-ph.EP2015★ 98 cited

Terrestrial Planet Formation Constrained by Mars and the Structure of the Asteroid Belt

André Izidoro, Sean N. Raymond, Alessandro Morbidelli +1

Reproducing the large Earth/Mars mass ratio requires a strong mass depletion in solids within the protoplanetary disk between 1 and 3 AU. The Grand Tack model invokes a specific mi…