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J/A+A/506/491  Eclipsing binary candidates in Corot-IRa01 field (Carpano+, 2009)

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
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). File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file tablea1.dat 97 145 Eclipsing binary candidates found in IRa01
See also: B/corot : CoRoT observation log Release 5 (CoRoT, 2010) J/A+A/506/501 : Eclipsing binaries in CoRoT-LRc01 field (Cabrera+, 2009) Byte-by-byte Description of file: tablea1.dat
Bytes Format Units Label Explanations
1- 3 I3 --- Seq [1/145] Sequential number 4 A1 --- n_Seq [*] * Note on sources 39 and 40 (1) 6- 14 I9 --- CoRoT CoRoT identification number (Cat. B/corot) 16- 22 A7 --- WIN WIN designation (EN NNNN) 24- 30 F7.3 deg RAdeg Right ascension (J2000) 32- 40 F9.6 deg DEdeg Declination (J2000) 42- 46 F5.2 mag Vmag V magnitude 48- 55 F8.5 d Per ?=- Period (2) 57- 64 E8.3 d e_Per ? rms uncertainty on Per 66- 74 F9.5 d Epoch Epoch (JD-2454000) 76- 83 E8.3 d e_Epoch rms uncertainty on Epoch 85- 90 F6.3 h Dur Transit duration 92- 97 F6.3 % Depth Transit depth
Note (1): Sources labeled 39 and 40 are two binaries in the same mask of CoRoT, so there is a single CoRoT identifier for both. Note (2): Sources 140 to 145 are eclipsing binaries where only one eclipse has been found, so their period could not be determined (these are the so-called mono-transit events).
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 27-May-2010
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