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Table 1
Instruments used for the ground-based CoRoT follow-up observations.
Instrument | Observatory |
|
|
Photometry | |
CAMELOT on the IAC 80 cm telescope; SD camera on the ESA Optical ground-station (ESA-OGS); FastCam at the Carlos Sanchez Telescope (CST) | Observatorio del Teide, Tenerife, Spain |
CCD cameras on the 0.46 m and 1 m Wise telescopes | Wise Observatory, Israel |
EulerCam on the Euler 1.2 m telescope | La Silla observatory, Chile |
MegaCam on the 3.6 m Canada-France-Hawaii telescope (CFHT) | CFH observatory, Hawaii, USA |
CCD camera on the 1.2 m MONET-North telescope | McDonald Observatory, Texas, USA |
NACO on the ESO-VLT | Paranal Observatory, Chile |
BEST on the DLR 20 cm telescope | Observatoire de Haute-Provence (OHP), France |
BEST II on the DLR 25 cm telescope | Observatorio Cerro Armazones, Chile |
|
|
Spectroscopy | |
AAOmega on the 3.9 m AAO telescope | Astronomical Australian Observatory (AAO), Australia |
FLAMES-GIRAFFE and UVES on ESO’s VLT | Paranal Observatory, Chile |
CRIRES on ESO’s VLT | Paranal Observatory, Chile |
CORALIE on the 1.2 m Euler telescope, HARPS on the ESO 3.6 m telescope | La Silla observatory, Chile |
Sandiford on the 2.1 m Otto Struve telescope | McDonald Observatory, Texas, USA |
Coudé spectrograph on the 2 m TLS telescope | Thüringer Landessternwarte (TLS), Tautenburg, Germany |
SOPHIE on the 1.93 m telescope | Observatoire de Haute-Provence (OHP), France |
HIRES on the 10 m Keck I telescope | Keck observatory, Hawaii,USA |
FIES on the 2.56 m NOT telescope | Roque de los Muchachos Observatory, La Palma, Spain |
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