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Related papers: New Data and Improved Parameters for the Transitin…

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We report five new transit epochs of the extrasolar planet OGLE-TR-111b, observed in the v-HIGH and Bessell I bands with the FORS1 and FORS2 at the ESO Very Large Telescope, between April and May 2008. The new transits have been combined…

Earth and Planetary Astrophysics · Physics 2015-05-27 Sergio Hoyer , Patricio Rojo , Mercedes López-Morales , Rodrigo Díaz , John E. Chambers , Dante Minniti

We present six new transits of the exoplanet OGLE-TR-111b observed with the Magellan Telescopes in Chile between April 2008 and March 2009. We combine these new transits with five previously published transit epochs for this planet between…

Earth and Planetary Astrophysics · Physics 2010-12-16 E. R. Adams , M. Lopez-Morales , J. L. Elliot , S. Seager , D. J. Osip

We report the results of the first transit timing variation (TTV) analysis of the very hot Jupiter OGLE-TR-132b, using ten transits collected over a seven-year period. Our analysis combines three previously published transit light curves…

Earth and Planetary Astrophysics · Physics 2011-08-24 Elisabeth R. Adams , Mercedes Lopez-Morales , James L. Elliot , Sara Seager , David J. Osip

The search for double transit planetary systems opens new possibilities for the transit searches and for studies of orbital stability, stellar irradiation, and migration scenarios, among others. We explore the OGLE lightcurves of stars with…

Astrophysics · Physics 2007-05-23 Dante Minniti

We present high precision K-band photometry of the transit and secondary eclipse of extrasolar planet OGLE-TR-113, using the SOFI near-infrared instrument on ESO's NTT. Data were taken in 5 second exposures over two periods of 3-4 hours,…

Astrophysics · Physics 2008-11-26 I. A. G. Snellen , E. Covino

We have computed evolutionary models for extrasolar planets which range in mass from 0.1 to 3.0 Jovian Masses, and which range in equilibrium temperature from 113 K to 2000 K. We present four sequences of models, designed to show the…

Astrophysics · Physics 2010-04-06 P. Bodenheimer , G. Laughlin , D. N. C. Lin

We present results of the photometric campaign for planetary and low-luminosity object transits conducted by the OGLE survey in 2005 season (Campaign #5). About twenty most promising candidates discovered in these data were subsequently…

Context: During the past years photometric surveys, later complemented by follow-up radial-velocity measurements, have revealed the presence of several new extra-solar transiting planets, in very short period orbits. Many of the host stars…

Astrophysics · Physics 2009-11-11 N. C Santos , F. Pont , C. Melo , G. Israelian , F. Bouchy , M. Mayor , C. Moutou , D. Queloz , S. Udry , T. Guillot

We report on the detection of the secondary eclipse of the very-hot Jupiter OGLE-TR-56b from combined z-band time series photometry obtained with the VLT and Magellan telescopes. We measure a flux decrement of 0.0363+/-0.0091 percent from…

Earth and Planetary Astrophysics · Physics 2009-11-13 David K. Sing , Mercedes Lopez-Morales

The photometric data collected during 2001 season OGLE-III planetary/low luminosity object transit campaign were reanalyzed with the new transit search technique -- the BLS method by Kovacs, Zucker and Mazeh. In addition to all presented in…

The initial task that confronted extrasolar-planet transit surveys was to monitor enough stars with sufficient photometric precision and complete phase coverage. Numerous searches have been pursued over the last few years. Among these…

Astrophysics · Physics 2009-09-29 David Charbonneau

We report the discovery of a transiting hot Jupiter around OGLE-TR-111, from our radial velocity follow-up of OGLE transiting candidates in Carina. The planet has a mass of 0.53 +- 0.11 M_J and a radius of 1.0 +0.13-0.06 R_J. Three…

While the vast majority of multiple-planet systems have their orbital angular momentum axes aligned with the spin axis of their host star, Kepler-56 is an exception: its two transiting planets are coplanar yet misaligned by at least 40…

Two years ago, the OGLE-III survey (Optical Gravitational Lensing Experiment) announced the detection of 54 short period multi-transiting objects in the Galactic bulge (Udalski et al., 2002a, 2002b). Some of these objects were considered to…

Astrophysics · Physics 2011-03-28 Francois Bouchy , F. Pont , C. Melo , N. C. Santos , M. Mayor , D. Queloz , S. Udry

We present a second paper of fully characterization of a sample of stars whose low-depth transits were discovered by the OGLE-III campaign in order to select the most promising candidates for spectroscopic confirmation, following the same…

Earth and Planetary Astrophysics · Physics 2010-04-28 J. Gallardo , S. Silva , S. Ramirez Alegria , D. Minniti , P. Pietrukowicz

The detection of transits is an efficient technique to uncover faint companions around stars. The full characterisation of the companions (M-type stars, brown dwarfs or exoplanets) requires high-resolution spectroscopy to measure properly…

Astrophysics · Physics 2008-12-18 J. Gallardo , D. Minniti , D. Valls-Gabaud , M. Rejkuba

As a result of a radial velocity follow-up of OGLE planetary transit candidates in Carina, we report the discovery of two new transiting planets with very short orbital periods: OGLE-TR-113 with m=1.35+-0.22 M_{Jup}, r=1.08 {+0.07}{-0.05}…

Astrophysics · Physics 2009-11-10 F. Bouchy , F. Pont , N. C. Santos , C. Melo , M. Mayor , D. Queloz , S. Udry

We present RIz photometry of four consecutive transits of the newly discovered exoplanet XO-1b. We improve upon the estimates of the transit parameters, finding the planetary radius to be R_P = 1.184 +0.028/-0.018 R_Jupiter and the stellar…

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, OGLE-TR-86, OGLE-TR-91, OGLE-TR-106, OGLE-TR-109, OGLE-TR-110,…

Earth and Planetary Astrophysics · Physics 2015-05-14 P. Pietrukowicz , D. Minniti , R. F. Diaz , J. M. Fernandez , M. Zoccali , W. Gieren , G. Pietrzynski , M. T. Ruiz , A. Udalski , T. Szeifert , M. Hempel

Context: Repeated observations of exoplanet transits allow us to refine the planetary parameters and probe them for any time dependent variations. In particular deviations of the period from a strictly linear ephemeris, transit timing…

Earth and Planetary Astrophysics · Physics 2010-11-05 M. Lendl , C. Afonso , J. Koppenhoefer , N. Nikolov , Th. Henning , M. Swain , J. Greiner