III/282 CoRoT Bright Stars Catalogue with variability classes (Baglin+, 2015)
CoRoT Bright Stars Catalogue including variability classes.
Baglin A., Michel E.
<CoRoT Symposium 3, Kepler KASC-7 Joint Meeting, Toulouse, France (2015)>
=2019yCat.3282....0B 2019yCat.3282....0B
=2015EPJWC.10106002B 2015EPJWC.10106002B
ADC_Keywords: Stars, variable ; MK spectral classification
Mission_Name: CoRoT
Abstract:
The CoRoT bright stars catalogue describes the 143 different objects
observed during the mission, in the "bright star" field of CoRoT, and
their major properties. The almost continuous observations lasted
between 20 and 156 days, with a regular 32s sampling time.
Description:
Among the 143 different stars observed with CoRoT, 15 have been
observed twice and one has been observed three times. They have
spectral types from O to G, and luminosity classes from V to III.
The star types characterise the object. It has been used during the
selection or results from the light-curve inspection; it is often
complemented by indications on the variability class. Each star can
have several star-types related to its spectral type and to its
variability.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
catalog.dat 180 160 CoRoT Bright Stars Catalogue including
variability classes
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See also:
B/corot : CoRoT observation log (N2-4.4) (CoRoT 2016)
Byte-by-byte Description of file: catalog.dat
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Bytes Format Units Label Explanations
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1- 14 A14 --- Name Star name
16- 20 I5 --- CoRoT CoRoT identification number
22- 28 A7 --- Run Run
30- 37 A8 "DD/MM/YY" Obs.date Start observation date
39- 43 A5 "h:m" Obs.time Start observation time
45- 47 I3 d Length ? Length of observation
49- 58 A10 "h:m:s" Obs.timeE End observation time
60- 87 A28 --- Type Star type (1)
89- 99 A11 --- SpType Spectral type
101-105 F5.2 mag Vmag V magnitude
107-180 A74 --- Rem Remarks (2)
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Note (1): Star types as follows:
O = O type stars
B = B type stars
Be = B type stars with emission lines
CP = Chemically peculiar stars
A/early F = A and early F type stars
late F/G = Late F and G stars
KM = K or M type stars
Giant = Red giants (occasionally yellow)
Sol-like = showing solar-like pulsations
B Ceph = Beta Cephei stars
D Scut = Delta Scuti stars
G Dor = Gamma doradus stars
SPB = Slowly pulsating variables
FGK = FGK stars
Note (2): EB (eclipsing binary) and cluster member, run of another observation
if it has been observed several times, interruptions larger than one day
associated with partial change of the targets.
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Acknowledgements:
The CoRoT space mission, launched on 2006 December 27, was developed
and operated by Centre National d'Etudes Spatiales (CNES, France)
with the participation of the Science Program of the European Space
Agency (ESA), the ESA Research and Scientific Support Department
(RSSD), Austria, Belgium, Brazil, Germany and Spain
Annie Baglin, annie.baglin(at)obspm.fr
Eric Michel, eric.michel(at)obspm.fr
Reference:
Baglin and Michel (2015) : The Space Photometry Revolution - CoRoT
Symposium 3, Kepler KASC-7 Joint Meeting, Toulouse, France, Edited by
R.A. Garcia; J. Ballot; EPJ Web of Conferences, Volume 101, id.06002
(End) Patricia Vannier [CDS] 14-Jan-2019