Bibcode
Bloemen, S.; Marsh, T. R.; Degroote, P.; Ostensen, R. H.; Papics, P. I.; Aerts, C.; Koester, D.; Gansicke, B. T.; Breedt, E.; Lombaert, R.; Pyrzas, S.; Copperwheat, C. M.; Exter, K.; Raskin, G.; van Winckel, H.; Prins, S.; Pessemier, W.; Fremat, Y.; Hensberge, H.; Jorissen, A.; van Eck, S.
Bibliographical reference
VizieR On-line Data Catalog: J/MNRAS/422/2600. Originally published in: 2012MNRAS.422.2600B
Advertised on:
1
2013
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0
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0
Description
To determine the spectral type, the rotational velocity and the radial
velocity amplitude of the primary, we obtained 46 high-resolution
(R~85000) echelle spectra using the HERMES spectrograph at the 1.2-m
Mercator telescope (La Palma, Canary Islands). These were reduced using
the standard instrument-specific data reduction pipeline. Additionally,
we obtained 29 spectra with the ISIS spectrograph mounted on the 4.2-m
William Herschel Telescope (La Palma, Canary Islands).
The Kepler data from Q0 (quarter 0), Q1, Q2 and Q3 were retrieved from
the public archive (http://archive.stsci.edu/kepler/). The data span
229-d, resulting in a data set of 212-d of observations excluding the
gaps.
(6 data files).