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The Optical Gravitational Lensing Experiment project has recently provided the OGLE III list of low-luminosity object transits from campaigns #3 and #4, reporting 40 new objects exhibiting the low-amplitude photometric eclipses expected for…

天体物理学 · 物理学 2009-11-13 S. Dreizler , S. Schuh , D. Homeier

Recently, 59 low-luminosity object transits were reported from the Optical Gravitational Lensing Experiment (OGLE). Our follow-up low-resolution spectroscopy of 16 candidates provided two objects, OGLE-TR-3 and OGLE-TR-10, which have…

天体物理学 · 物理学 2009-11-07 S. Dreizler , P. Hauschildt , W. Kley , T. Rauch , S. L. Schuh , K. Werner , B. Wolff

We present results of an extensive photometric search for planetary and low-luminosity object transits in the Galactic disk stars commencing the third phase of the Optical Gravitational Lensing Experiment -- OGLE-III. Photometric…

We propose a method to distinguish between planetary and stellar companions to stars which present a periodic decrease in brightness, interpreted as a transit. Light curves from a total of 177 stars from the OGLE project were fitted by the…

天体物理学 · 物理学 2009-11-11 Adriana V. R. Silva , Patricia C. Cruz

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…

天体物理学 · 物理学 2011-03-28 Francois Bouchy , F. Pont , C. Melo , N. C. Santos , M. Mayor , D. Queloz , S. Udry

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…

天体物理学 · 物理学 2007-05-23 A. Udalski , K. Zebrun , M. Szymanski , M. Kubiak , I. Soszynski , O. Szewczyk , L. Wyrzykowski , G. Pietrzynski

We present results of the second planetary and low-luminosity object transit campaign conducted by the OGLE-III survey. Three fields (35'x35' each) located in the Carina regions of the Galactic disk (l~290) were monitored continuously in…

天体物理学 · 物理学 2008-11-26 A. Udalski , O. Szewczyk , K. Zebrun , G. Pietrzynski , M. Szymanski , M. Kubiak , I. Soszynski , L. Wyrzykowski

The photometric data collected by OGLE-III during the 2001 and 2002 observational campaigns aiming at detection of planetary or low-luminosity object transits were corrected for small scale systematic effects using the data pipeline by…

天体物理学 · 物理学 2007-05-23 A. Udalski , G. Pietrzynski , M. Szymanski , M. Kubiak , K. Zebrun , I. Soszynski , O. Szewczyk , L. Wyrzykowski

We report the results of our campaign to follow-up spectroscopically several candidate extrasolar transiting planets from the OGLE-III survey in the direction of the Galactic center, announced in 2001 (Udalski et al 2002a,b). All of these…

天体物理学 · 物理学 2009-11-10 Maciej Konacki , Guillermo Torres , Dimitar D. Sasselov , Saurabh Jha

We present results of two observing campaigns conducted by the OGLE-III survey in the 2003 observing season aiming at the detection of new objects with planetary transiting companions. Six fields of 35'x35' each located in the Galactic disk…

天体物理学 · 物理学 2008-11-26 A. Udalski , M. K. Szymanski , M. Kubiak , G. Pietrzynski , I. Soszynski , K. Zebrun , O. Szewczyk , L. Wyrzykowski

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…

天体物理学 · 物理学 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 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…

地球与行星天体物理 · 物理学 2010-04-28 J. Gallardo , S. Silva , S. Ramirez Alegria , D. Minniti , P. Pietrukowicz

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…

天体物理学 · 物理学 2007-05-23 Dante Minniti

We analyze the photometry of 117 OGLE stars with periodic transit events for the presence of ellipsoidal light variations, which indicate the presence of massive companions. We find that ~50% of objects may have stellar companions, mostly…

天体物理学 · 物理学 2009-11-07 E. Sirko , B. Paczynski

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…

天体物理学 · 物理学 2008-12-18 J. Gallardo , D. Minniti , D. Valls-Gabaud , M. Rejkuba

We present I and B photometry of five distinct transits of the exoplanet OGLE-TR-10b. By modeling the light curves, we find the planetary radius to be R_P = 1.06 +/- 0.08 R_Jup and the stellar radius to be R_S = 1.10 +/- 0.07 R_sun. The…

We recently used near-infrared spectroscopy to improve the characterization of 76 low-mass stars around which K2 had detected 79 candidate transiting planets. Thirty of these worlds were new discoveries that have not previously been…

We present the results of our high-resolution spectroscopic follow-up of 42 planetary transit candidates in Carina from the OGLE survey. This follow-up has already allowed the discovery of three new transiting exoplanets, OGLE-TR-111, 113…

天体物理学 · 物理学 2009-11-10 F. Pont , F. Bouchy , C. Melo , N. C. Santos , M. Mayor , D. Queloz , S. Udry

We present results of a search for transiting exoplanets in 10-yr long photometry with thousands of epochs taken in the direction of the Galactic bulge. This photometry was collected in the fourth phase of the Optical Gravitational Lensing…

We present precise V-band photometry for the low-amplitude transit candidate star OGLE-TR-109. This is an extreme case among the transiting candidates found by the OGLE group because of the early spectral type of the star (F0V), of the low…

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