OGLE-TR-132b transits a very metal-rich F dwarf about 2000 pc from the Sun, in the Galactic disc towards Carina. It orbits very close to its host star (a = 0.03 AU) and has an equilibrium temperature of nearly 2000 K. Using rapid-cadence transit photometry from the FORS2 camera on the VLT and SUSI2 on the NTT, and high-resolution spectroscopy with UVES on the VLT, we refine the shape of the transit light curve and the parameters of the system. In particular, we improve the planetary radius estimate, R = 1.18 ± 0.07 R[SUB]J[/SUB] and provide very precise ephemeris, T_tr = 2 453 142.59123 ± 0.0003 BJD and P = 1.689868 ± 0.000003 days. The obtained planetary mass is 1.14 ± 0.12 M_J. Our results give a slightly smaller and lighter star, and big...
We present I and B photometry of five distinct transits of the exoplanet OGLE-TR-10b. By modeling th...
We present accurate V-band photometry for a planetary transit of OGLE-TR-111 acquired with VIMOS at ...
Transiting planets are essential to study the structure and evolution of extra-solar planets. For th...
OGLE-TR-132b transits a very metal-rich F dwarf about 2000 pc from the Sun, in the Galactic disc tow...
Transiting planets are essential to study the structure and evolution of extra-solar planets. For th...
A high accuracy photometry algorithm is needed to take full advantage of the potential of the transi...
The exoplanet OGLE-TR-132b belongs to the new class of very hot giant planets, together with OGLE-T...
accepted in A&A lettersThe exoplanet OGLE-TR-132b belongs to the new class of very hot giant planets...
By re-processing the data of the second season of the OGLE survey for planetary transits and adding ...
We present results of the photometric campaign for planetary and low-luminosity object transits cond...
Transiting planets are essential to study the structure and evolution of extra-solar planets. For th...
We present I and B photometry of five distinct transits of the exoplanet OGLE-TR-10b. By modeling th...
We present accurate V-band photometry for a planetary transit of OGLE-TR-111 acquired with VIMOS at ...
Transiting planets are essential to study the structure and evolution of extra-solar planets. For th...
OGLE-TR-132b transits a very metal-rich F dwarf about 2000 pc from the Sun, in the Galactic disc tow...
Transiting planets are essential to study the structure and evolution of extra-solar planets. For th...
A high accuracy photometry algorithm is needed to take full advantage of the potential of the transi...
The exoplanet OGLE-TR-132b belongs to the new class of very hot giant planets, together with OGLE-T...
accepted in A&A lettersThe exoplanet OGLE-TR-132b belongs to the new class of very hot giant planets...
By re-processing the data of the second season of the OGLE survey for planetary transits and adding ...
We present results of the photometric campaign for planetary and low-luminosity object transits cond...
Transiting planets are essential to study the structure and evolution of extra-solar planets. For th...
We present I and B photometry of five distinct transits of the exoplanet OGLE-TR-10b. By modeling th...
We present accurate V-band photometry for a planetary transit of OGLE-TR-111 acquired with VIMOS at ...
Transiting planets are essential to study the structure and evolution of extra-solar planets. For th...