Free Access
| Instrument | Observatory |
| BEST 0.2-ma | Observatoire de Haute Provence, France |
| BESTII 0.25-ma | Cerro Armazones, Chile |
| TEST 0.3-m | Thüringer Landessternwarte, Germany |
| Vienna 0.8-m | Vienna Observatory, Austria |
| IAC 80-cm | Observatorio del Teide, Canary Islands, Spain |
| WISE 0.46-m, 1-m | WISE Observatory, Israel |
| OHP 1.2-m | Observatoire de Haute Provence, France |
| Euler 1.2-m telescope | La Silla, Chile |
| Tautenburg 2-m | Thüringer Landessternwarte, Germany |
| CFHT/Megacam 3.6-m | Mauna Kea, Hawaii |
| a The small BEST and BEST II telescopes are not used in the follow-up as decribed here. They obtained previous timeseries of CoRoT's sample fields (Rauer et al. 2009; Kabath et al. 2009b; Karoff et al. 2007; Kabath et al. 2008,2009a,2007) which are routinely checked against the detections from CoRoT. They will also be used for future surveying of CoRoT-short run fields. |
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