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 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:
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FileName Lrecl Records Explanations
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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 97 190 CoRoT eclipsing binary candidates in LRa01
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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
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Bytes Format Units Label Explanations
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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
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Byte-by-byte Description of file: table6.dat
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Bytes Format Units Label Explanations
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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
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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
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Byte-by-byte Description of file: notes.dat
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Bytes Format Units Label Explanations
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1- 2 A2 --- CCD [E1 E2] Window designation (G2)
4- 7 I4 --- wId Window designation (G2)
9- 80 A72 --- Com Comments
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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.
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History:
From electronic version of the journal
(End) Patricia Vannier [CDS] 17-Apr-2012