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J/A+A/538/A112 Planetary transit candidates in CoRoT LRa01 field (Carone+, 2012)

Planetary transit candidates in the CoRoT LRa01 field. Carone L., Gandolfi D., Cabrera J., Hatzes A.P., Deeg H.J., Csizmadia SZ., Paetzold M., Weingrill J., Aigrain S., Alonso R., Alapini A., Almenara J.-M., Auvergne M., Baglin A., Barge P., Bonomo A.S., Borde P., Bouchy F., Bruntt H., Carpano S., Cochran W.D., Deleuil M., Diaz R.F., Dreizler S., Dvorak R., Eisloeffel J., Eigmueller P., Endl M., Erikson A., Ferraz-Mello S., Fridlund M., Gazzano J.-C., Gibson N., Gillon M., Gondoin P., Grziwa S., Guenther E.W., Guillot T., Hartmann M., Havel M., Hebrard G., Jorda L., Kabath P., Leger A., Llebaria A., Lammer H., Lovis C., MacQueen P.J., Mayor M., Mazeh T., Moutou C., Nortmann L., Ofir A., Ollivier M., Parviainen H., Pepe F., Pont F., Queloz D., Rabus M., Rauer H., Regulo C., Renner S., de La Reza R., Rouan D., Santerne A., Samuel B., Schneider J., Shporer A., Stecklum B., Tal-Or L., Tingley B., Udry S., Wuchterl G. <Astron. Astrophys., 538, A112 (2012)> =2012A&A...538A.112C
ADC_Keywords: Binaries, eclipsing ; Planets Keywords: techniques: spectroscopic - techniques: photometric - binaries: eclipsing - techniques: radial velocities - planetary systems Abstract: CoRoT is a pioneering space mission whose primary goals are stellar seismology and extrasolar planets search. Its surveys of large stellar fields generate numerous planetary candidates whose lightcurves have transit-like features. An extensive analytical and observational follow-up effort is undertaken to classify these candidates. Description: We present the list of planetary transit candidates from the CoRoT LRa01 star field in the Monoceros constellation toward the Galactic anti-center direction. The CoRoT observations of LRa01 lasted from 24 October 2007 to 3 March 2008. We acquired and analyzed 7470 chromatic and 3938 monochromatic lightcurves. Instrumental noise and stellar variability were treated with several filtering tools by different teams from the CoRoT community. Different transit search algorithms were applied to the lightcurves. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table5.dat 98 56 CoRoT LRa01 planetary candidates: coordinates and transit parameters table6.dat 124 56 CoRoT LRa01 planetary candidates: follow-up results notes.dat 80 185 Individual notes for table6 table7.dat 98 190 CoRoT eclipsing binary candidates in LRa01
See also: B/corot : CoRoT observation log Release 8 (CoRoT, 2012) J/AJ/136/654 : BEST periodic variable stars in LRa1 field (Kabath+, 2008) J/A+A/539/A14 : Planetary transit candidates in CoRoT SRc01 (Erikson+, 2012) Byte-by-byte Description of file: table[57].dat
Bytes Format Units Label Explanations
1 A1 --- St [CNGLFXM] Status of candidate (G1) 3- 11 I9 --- CoRoT CoRoT identification number 13- 14 A2 --- CCD [E1 E2] Window designation (G2) 16- 19 I4 --- wId Window designation (G2) 21- 29 F9.5 deg RAdeg Right ascension in decimal degrees (J2000) 31- 38 F8.5 deg DEdeg Declination in decimal degrees (J2000) 40- 45 F6.3 mag Vmag ? V magnitude (only in table7) 47- 56 F10.7 d Per ?=- Period 58- 65 F8.6 d e_Per ?=- rms uncertainty in Per 67- 76 F10.6 d Epoch Epoch of transit or eclipse (HJD-2454000) 78- 85 F8.6 d e_Epoch rms uncertainty in Epoch 87- 91 F5.2 h Dur Transit or Eclipse duration 93- 98 F6.3 % Depth [0/100] Transit or Eclipse depth
Byte-by-byte Description of file: table6.dat
Bytes Format Units Label Explanations
1 A1 --- St [CNGLFXM] Status of candidate (G1) 3- 4 A2 --- CCD [E1 E2] Window designation (G2) 6- 9 I4 --- wId Window designation (G2) 11- 16 F6.3 mag Bmag B magnitude 18- 23 F6.3 mag Vmag V magnitude 25- 30 F6.3 mag r'mag r' magnitude 32- 37 F6.3 mag i'mag i' magnitude 39- 49 A11 --- Cand Candidate nature (3) 51- 85 A35 --- FUP Follow-up facilities, photometry 88-124 A37 --- FUS Follow-up facilities, spectroscopy
Note (3): Abbreviations used: CEB = Spatially resolved contaminating eclipsing binary system whose light is diluted by the main CoRoT target SB1 = Binary system with one spectroscopically visible stellar component SB2 = Binary system with two spectroscopically visible stellar components SB3 = Triple system with three spectroscopically visible stellar components Blend = spatially unresolved eclipsing binary system whose light is diluted by the main CoRoT target
Byte-by-byte Description of file: notes.dat
Bytes Format Units Label Explanations
1- 2 A2 --- CCD [E1 E2] Window designation (G2) 4- 7 I4 --- wId Window designation (G2) 9- 80 A72 --- Com Comments
Global notes: Note (G1): Flags as follows: C = Confirmed planets N = Settled cases: non-planetary objects G = Unsettled good planetary candidates L = Unsettled low-priority planetary candidates F = False alarms X = X-case candidates M = Mono-transits Note (G2): contains the identifier E1 or E2, which identifies the CCD 1 or 2 of the exoplanet channel, respectively, followed by a 4-digit number. This number represents the assigned CoRoT mask.
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 17-Apr-2012
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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