Abstract
We report on the ground-based follow-up program of spectroscopic and photometric observations of solar-like asteroseismic targets for the Kepler space mission. These stars constitute a large group of more than a thousand objects which are the subject of an intensive study by the Kepler Asteroseismic Science Consortium Working Group 1 (KASC WG-1). In the current work we will discuss the methods we use to determine the fundamental stellar atmospheric parameters using high-quality stellar spectra. These provide essential constraints for the asteroseismic modelling and make it possible to verify the parameters in the Kepler Input Catalogue (KIC).
| Original language | English |
|---|---|
| Pages (from-to) | 981-984 |
| Number of pages | 4 |
| Journal | Astronomische Nachrichten |
| Volume | 331 |
| Issue number | 9-10 |
| DOIs | |
| Publication status | Published - Dec 2010 |
| Externally published | Yes |
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