Free Access

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

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.