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J/A+A/506/491 Planetary transit candidates in Corot-IRa01 field (Carpano+, 2009)
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tablea1.dat
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Beginning of ReadMe :J/A+A/506/491 Eclipsing binary candidates in Corot-IRa01 field (Carpano+, 2009)
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Planetary transit candidates in Corot-IRa01 field.
Carpano S., Cabrera J., Alonso R., Barge P., Aigrain S., Almenara J.-M.,
Borde P., Bouchy F., Carone L., Deeg H.J., De La Reza R., Deleuil M.,
Dvorak R., Erikson A., Fressin F., Fridlund M., Gondoin P., Guillot T.,
Hatzes A., Jorda L., Lammer H., Leger A., Llebaria A., Magain P.,
Moutou C., Ofir A., Ollivier M., Janot-Pacheco E., Paetzold M., Pont F.,
Queloz D., Rauer H., Regulo C., Renner S., Rouan D., Samuel B.,
Schneider J., Wuchterl G.
<Astron. Astrophys., 506, 491-500 (2009)>
=2009A&A...506..491C
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ADC_Keywords: Stars, double and multiple ; Binaries, eclipsing ; Planets
Keywords: stars: planetary systems - techniques: photometric -
binaries: eclipsing - planetary systems
Abstract:
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 candidates detected in the
first field observed by CoRoT, IRa01, the initial run toward the
Galactic anticenter, which lasted for 60 days.
We analysed 3898 sources in the coloured bands and 5974 in the
monochromatic band. Instrumental noise and stellar variability were
taken into account using detrending tools before applying various
transit search algorithms.
Description:
CoRoT observed its first field from early February 2008 until early
April, for approximatively 60 days. The run code "IRa01" is explained
as following. The "IR" means "initial run" in contrast to the
subsequent "long runs" (LR) and "short runs" (SR). The third letter
refers to the direction with respect to the Galactic center ("a", as
in this case, anticenter or "c" Galactic center). The last two digits
are the sequence for this type of observation (01 being the first
one).