activity
20002020
most citedThe Taurus Spitzer Survey: New Candidate Taurus Members Selected Using Sensitive Mid-Infrared Photometry

293 citations · 1.1k across the 13 of their papers we have counts for

collaborators

12 papers

astro-ph.SR2020★ 90 cited

Rotation of Low-Mass Stars in Taurus with K2

L. M. Rebull, J. R. Stauffer, A. M. Cody +4

We present an analysis of K2 light curves (LCs) from Campaigns 4 and 13 for members of the young (3 Myr) Taurus association, in addition to an older (30 Myr) population…

astro-ph.SR2016★ 3 cited

Fundamental stellar parameters for selected T-Tauri stars in the Chamaeleon and Rho Ophiuchus star-forming regions

David James, Alicia Aarnio, Alexander Richert +4

We present the results of an optical photometry and high-resolution spectroscopy campaign for a modest sample of X-ray selected stars in the Chamaeleon and Rho Ophiuchus star formi…

astro-ph.GA2010★ 54 cited

The low-mass population of the Rho Ophiuchi molecular cloud

C. Alves de Oliveira, E. Moraux, J. Bouvier +3

Star formation theories are currently divergent regarding the fundamental physical processes that dominate the substellar regime. Observations of nearby young open clusters allow t…

astro-ph.SR2009★ 293 cited

The Taurus Spitzer Survey: New Candidate Taurus Members Selected Using Sensitive Mid-Infrared Photometry

L. M. Rebull, D. L. Padgett, C. -E. McCabe +31

We report on the properties of pre-main-sequence objects in the Taurus molecular clouds as observed in 7 mid- and far-infrared bands with the Spitzer Space Telescope. There are 215…

astro-ph.SR2009★ 57 cited

Young T-Dwarf Candidates in IC 348

A. S. M. Burgess, E. Moraux, J. Bouvier +3

The determination of the lower-end of the initial mass function (IMF) provides strong constraints on star formation theories. We report here on a search for isolated planetary-mass…

astro-ph.SR2009★ 71 cited

A spectroscopic survey of the youngest field stars in the solar neighbourhood. I. The optically bright sample

P. Guillout, A. Klutsch, A. Frasca +8

We present the first results of a ground-based programme conducted on 1-4m class telescopes. Our sample consists of 1097 active and presumably young stars, all of them being optica…