Table 1:

Instruments and methods used in the complementary observations of the IRa01 candidates.
Instrument Diam Tel Nb Nightsa Method Measurementb
INT/WFC 2.5 5 photometry pre-launch spectral typing, astrometry
IAC80 0.8 0.5 photometry on-target transit confirmation
EulerCam 1.2 3 photometry on-target transit confirmation
Wise/0.46 0.46 3 photometry on-target transit confirmation
Wise/1.0 1.0 3 photometry on-target transit confirmation
CFHT/Megacam 3.6 1.5 photometry on-target transit confirmation
CORALIE 1.2 1 radial velocity SB identification
SOPHIE 1.93 7 radial velocity SB identification,
        mass characterization
HARPS 3.6 5 radial velocity SB identification, stellar parameters
        mass characterization
UVES 8.0 0.5 spectroscopy stellar parameters
a The approximate number of nights per instrument is given as an indication of the observational effort needed for the follow-up of a single CoRoT field. b SB stands for spectroscopic binary.

Source LaTeX | All tables | In the text

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