Millimagnitude photometry for transiting extrasolar planetary candidates IV Solution to the puzzle of the extremely red OGLE TR 82 primary

We measured a pseudo-equivalent width (pEW) of 18±4 Å (1σ), consistent with the compilation of field L5 dwarfs ex- hibiting lithium in absorption We derived the error bars from

The proposed observations are a critical component of a broader study comprising existing and future ground- and space- based observations that will produce a

We detected the transit light-curve signature in the course of the TrES multi-site transiting planet survey, and confirmed the planetary nature of the companion via

We cross-matched the 2MASS and AllWISE public catalogues and measured proper motions to identify low-mass stars and brown dwarf candidates in an area of radius eight degrees around

Spectral profiles of Rb i (top) and Cs i (bottom) atomic lines of Luhman 16AB. The relative fluxes of the two objects have been normal- ized to the mean pseudo-continuum around Rb i

2, but the spectrum of GCS 0845 is compared to those of other field dwarfs with known spectral types taken from the literature and not observed with GTC/OSIRIS: the 2M 0251 +2521

- Can affect age by ~0.5 Gyr.. Initial Mass Function.. 2010). - Larger characteristic mass at

We show that the very young brown dwarf candidate ISO 217 (M6.25) is driving an intrinsically asymmetric bipolar outflow with a stronger and slightly faster red-shifted component