==========================================================================
III/282 CoRoT Bright Stars Catalogue with variability classes (Baglin+, 2015)
The following files can be converted to FITS (extension .fit or fit.gz)
catalog.dat
==========================================================================
Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=III/282
==========================================================================
drwxr-xr-x 259 cats archive 8192 Dec 5 19:00 [Up]
drwxr-xr-x 3 cats archive 275 Jan 12 2023 [TAR file]
-rw-r--r-- 1 cats archive 463 Dec 19 2022 .message
-r--r--r-- 1 cats archive 4554 Jan 16 2019 ReadMe
-rw-r--r-- 1 cats archive 337 Jan 16 2019 +footg5.gif
-rw-r--r-- 1 cats archive 2532 Jan 16 2019 +footg8.gif
-r--r--r-- 1 cats archive 18251 Jan 14 2019 catalog.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe :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
=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.