activity
20112025
most citedSOPHIE velocimetry of Kepler transit candidates XVII. The physical properties of giant exoplanets within 400 days of period

273 citations · 1.3k across the 36 of their papers we have counts for

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Showing 2013Show all

6 papers · 1 filter

astro-ph.SR2013

High Resolution Spectroscopy of M subdwarfs

A. S. Rajpurohit, C. Reyle, M. Schultheis +1

M subdwarfs are metal poor and cool stars. They are important probes of the old galactic populations. However, they remain elusive due to their low luminosity. Observational and mo…

astro-ph.SR2013★ 4 cited

CFBDS J111807-064016: A new L/T transition brown dwarf in a binary system

C. Reylé, P. Delorme, É. Artigau +7

Stellar-substellar binary systems are quite rare, and provide interesting benchmarks. They constrain the complex physics of substellar atmospheres, because several physical paramet…

astro-ph.SR2013★ 43 cited

The SDSS-III APOGEE Radial Velocity Survey of M dwarfs I: Description of Survey and Science Goals

R. Deshpande, C. H. Blake, C. F. Bender +28

We are carrying out a large ancillary program with the SDSS-III, using the fiber-fed multi-object NIR APOGEE spectrograph, to obtain high-resolution H-band spectra of more than 120…

astro-ph.IM2013★ 57 cited

Instrumental Methods for Professional and Amateur Collaborations in Planetary Astronomy

O. Mousis, R. Hueso, J. -P. Beaulieu +57

Amateur contributions to professional publications have increased exponentially over the last decades in the field of Planetary Astronomy. Here we review the different domains of t…

astro-ph.SR2013★ 231 cited

The Effective Temperature Scale of M dwarfs

A. S. Rajpurohit, C. Reylé, F. Allard +4

Despite their large number in the Galaxy, M dwarfs remain elusive objects and the modeling of their photospheres has long remained a challenge (molecular opacities, dust cloud form…

astro-ph.SR2013★ 51 cited

Progress in Modeling Very Low Mass Stars, Brown Dwarfs, and Planetary Mass Objects

F. Allard, D. Homeier, B. Freytag +2

We review recent advancements in modeling the stellar to substellar transition. The revised molecular opacities, solar oxygen abundances and cloud models allow to reproduce the pho…