Context: CoRoT is a pioneering space mission devoted to the analysis of stellar variability and the photometric detection of extrasolar planets. Aims: We present the list of planetary transit candidates detected in the first field observed by CoRoT, IRa01, the initial run toward the Galactic anticenter, which lasted for 60 days. Methods: We
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Planetary transit candidates in Corot-IRa01 fieldCarpano, S. et al.102009
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Planetary transit candidates in CoRoT-LRc01 field
Aims: 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 lasted from May to October 2007. Methods: we analyzed 3719 (33%) sources in the chromatic bands and 7689 in the monochromatic band. Instrumental noise and the stellar
Cabrera, J. et al.Advertised on:
102009 -
Planetary transit candidates in the CoRoT initial run: resolving their nature
With the release of CoRoT lightcurves of the Initial Run IRa01, 50 transiting planetary candidates have been published in a companion paper. About twenty of them were identified as binary stars from the CoRoT lightcurve itself. Complementary observations were conducted for 29 candidates, including ground-based photometry and radial-velocity
Moutou, C. et al.Advertised on:
102009 -
Planetary transit of TrES-1 and TrES-2 (Rabus+, 2009)
We observed several transits of TrES-1 and TrES-2 with the IAC 80cm telescope. (2 data files).
Rabus, M. et al.Advertised on:
102009 -
Polarized Mid-infrared Synchrotron Emission in the Core of Cygnus A
We present high-angular (~0.''4) resolution mid-infrared (MIR) polarimetric observations in the 8.7 μm and 11.6 μm filters of Cygnus A using CanariCam on the 10.4 m Gran Telescopio CANARIAS. A highly polarized nucleus is observed with a degree of polarization of 11% ± 3% and 12% ± 3% and a position angle of polarization of 27° ± 8° and 35° ± 8° in
Lopez-Rodriguez, E. et al.Advertised on:
102014 -
Position and Variability of {2A 1704+241}
We present results of analyses of observations of the X-ray source 2A 1704+241 with the ROSAT Position Sensitive Proportional Counter (PSPC) and the High Resolution Imager (HRI). 2A 1704+241 was first associated with the M-giant star HD 154791 based upon observations with the HEAO 1 SMC and the {Einstein} IPC and analysis of a spectrum of HD 154791
Morgan, W. A., Jr. et al.Advertised on:
102000