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BVR light curves of KR Com
We present the detailed analysis of triple system KR Com with different observational techniques - photometry, interferometry, and period variation. The use of BVR photometry of... -
1318 new variable stars in Galactic plane
We have conducted a deep photometric survey of a 0.5deg*0.5deg area of the Galactic Plane using the WFI instrument on the 2.2-m ESO telescope on La Silla, Chile. The dataset... -
Transits of HD40307b by Spitzer
We used Spitzer and its IRAC camera to search for the transit of the super-Earth HD 40307b. The hypothesis that the planet transits could not be firmly discarded from our first... -
Spectral lines of BK Peg and BW Aqr
Double-lined, detached eclipsing binaries are our main source for accurate stellar masses and radii. In this paper we focus on the 1.15-1.70M_{sun}_ interval where convective... -
H-band thermal emission of exoplanet WASP-19b
We present the first ground-based detection of thermal emission from an exoplanet in the H-band. Using HAWK-I on the VLT, we observed an occultation of WASP-19b by its G8V-type... -
Light curves of CoRoT-2 in z-band, 4.5um and 8um
We report measurements of the thermal emission of the young and massive planet CoRoT-2b at 4.5 and 8um with the Spitzer Infrared Array Camera (IRAC). Our measured occultation... -
EW Ori differential uvby light curves
Recent studies of inactive and active solar-type binaries suggest that chromospheric activity, and its effect on envelope convection, is likely to cause significant radius and... -
V1130 Tau differential uvby light curves
Double-lined, detached eclipsing binaries are our main source for accurate stellar masses and radii. This paper is the first in a series with focus on the upper half of the... -
Stellar Limb-Darkening Coefficients
Transiting exoplanets provide unparalleled access to the fundamental parameters of both extrasolar planets and their host stars. We present limb-darkening coefficients (LDCs)... -
Four new SDSS eclipsing systems
We present photometry of nine cataclysmic variable stars identified by the Sloan Digital Sky Survey, aimed at measuring the orbital periods of these systems. Four of these... -
Study of an eclipsing binary in M31
The cosmic distance scale largely depends on distance determinations to galaxies of the Local Group. In this sense, the Andromeda galaxy (M31) is a key rung to better constrain... -
Transits of 12 new exoplanet candidates
We used VLT/VIMOS images in the V band to obtain light curves of extrasolar planetary transits OGLE-TR-111 and OGLE-TR-113, and candidate planetary transits: OGLE-TR-82,... -
BEST-II periodic variables in CoRoT LRa02 field
The Berlin Exoplanet Search Telescope II (BEST II) is a small wide field-of-view photometric survey telescope system located at the Observatorio Cerro Armazones, Chile. The high... -
Eclipsing binaries in CoRoT-LRc01 field
We present here the list of planetary transit candidates detected in the first long run observed by CoRoT: LRc01, towards the galactic center in the direction of Aquila, which... -
Eclipsing binary candidates in Corot-IRa01 field
CoRoT is a pioneering space mission devoted to the analysis of stellar variability and the photometric detection of extrasolar planets. We present the list of planetary transit... -
FORS2 and HAWKI photometry of CoRoT-1
We present VLT eclipse photometry for the giant planet CoRoT-1b. We observed a transit in the R-band filter and an occultation in a narrow filter centered on 2.09{mu}m. Our... -
Variable stars in a VLT/VIMOS field in Carina
We have searched for variable stars in deep V-band images of a field towards the Galactic plane in Carina. The images were taken with VIMOS instrument at ESO VLT during 4... -
HD 17156 transit photometry & radial velocities
To improve the parameters of the HD17156 system (peculiar due to the eccentric and long orbital period of its transiting planet) and constrain the presence of stellar... -
WASP-13b photometry and radial velocities
We report the discovery of WASP-13b, a low-mass M_p_=0.46^+0.06^-0.05 M_J_ transiting exoplanet with an orbital period of 4.35298+/-0.00004days. The transit has a depth of... -
V636 Cen radial velocities curves
The influence of stellar activity on the fundamental properties of stars around and below 1M_{sun}_ is not well understood. Accurate mass, radius, and abundance determinations...