activity
20142016
most citedThe Kepler Follow-Up Observation Program. I. A Catalog of Companions to Kepler Stars from High-Resolution Imaging

257 citations · 658 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.SR2016257 cited

The Kepler Follow-Up Observation Program. I. A Catalog of Companions to Kepler Stars from High-Resolution Imaging

E. Furlan, D. R. Ciardi, M. E. Everett +16

We present results from high-resolution, optical to near-IR imaging of host stars of Kepler Objects of Interest (KOIs), identified in the original Kepler field. Part of the data we…

astro-ph.EP201610 cited

Spectroscopic characterisation of microlensing events Towards a new interpretation of OGLE-2011-BLG-0417

A. Santerne, J. -P. Beaulieu, B. Rojas Ayala +14

The microlensing event OGLE-2011-BLG-0417 is an exceptionally bright lens binary that was predicted to present radial velocity variation at the level of several km/s. Pioneer radia…

astro-ph.EP201612 cited

Detection of the secondary eclipse of Qatar-1b in the Ks band

Patricia Cruz, David Barrado, Jorge Lillo-Box +4

Qatar-1b is a close-orbiting hot Jupiter ( , ) around a metal-rich K-dwarf, with orbital separation and period of 0.023 AU and 1.42 days.…

astro-ph.SR2016

An upper limit to the mass of a close companion candidate to σ Ori E

José A. Caballero, Hervé Bouy, Jorge Lillo-Box

The famous, very young, helium rich, magnetically-active, radio and X-ray emitter, short-period rotationally variable, spectroscopically peculiar star σ Ori E may have a close late…

astro-ph.SR201625 cited

The seven sisters DANCe.II. Proper motions and the lithium-rotation-activity connection for G and K Pleiads

D. Barrado, H. Bouy, J. Bouvier +7

Stellar clusters are open windows to understand stellar evolution. Specifically, the change with time and the dependence on mass of different stellar properties. As such, they are…

astro-ph.SR20151 cited

Spectro-astrometry of LkCa 15 with X-Shooter: Searching for emission from LkCa 15b

E. T. Whelan, N. Huelamo, J. M. Alcala +5

Planet formation is one explanation for the partial clearing of dust observed in the disks of some T Tauri stars. Indeed studies using state-of-the-art high angular resolution tech…