Absolute dimensions of eclipsing binaries - XXVIII. BK Pegasi and other F-type binaries: Prospects for calibration of convective core overshoot

J. V. Clausen; S. Frandsen; H. Bruntt; E. H. Olsen; B. E. Helt; K. Gregersen; D. Juncher; P. Krogstrup

doi:10.1051/0004-6361/201014266

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Volume 516 (June-July 2010)

A&A, 516 (2010) A42

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Table 3:

Log of the FIES observations of BK Peg.
HJD-2 400 000^a	phase	$t_{\rm exp}$ ^b	S/N^c
54333.45954	0.6647	300	60
54333.46395	0.6655	300	55
54334.42028	0.8397	300	20
54335.52799	0.0414	300	70
54335.53872	0.0434	600	85
54335.62203	0.0586	600	85
54335.72881	0.0780	600	100
54336.41869	0.2037	600	55
54336.43503	0.2067	600	60
54336.52436	0.2229	600	75
54336.74168	0.2625	600	80
54337.44772	0.3911	600	65
54337.58944	0.4169	600	75

Notes. ^(a) Refers to mid-exposure. ^(b) Exposure time in seconds. ^(c) Signal-to-noise ratio measured around 6070 Å.

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