Absolute dimensions of eclipsing binaries - XXVII. V1130 Tauri: a metal-weak F-type system, perhaps with preference for Y = 0.23–0.24

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Table 5:

Log of the FEROS observations of V1130 Tau.
HJD-2400000^a	Phase	$t_{\rm exp}$ ^b	S/N^c
51188.6379	0.1675	600	223
51207.5446	0.8344	600	171
51207.5662	0.8615	600	170
51208.5852	0.1370	600	162
51209.5918	0.3971	600	200
51211.5630	0.8645	600	84
51212.6064	0.1706	600	176
51385.9274	0.1288	600	142
51386.9327	0.3872	600	170
51390.8696	0.3154	600	241
51391.9171	0.6266	600	225
51392.8746	0.8252	720	237
51562.5335	0.1992	600	243
51562.5962	0.2777	600	281
51562.6289	0.3187	600	244
51977.4958	0.6371	630	181
51978.4897	0.8812	600	179
51981.4927	0.6402	600	166

Notes. ^(a) Refers to mid-exposure. ^(b) Exposure time in seconds. ^(c) Signal-to-noise ratio measured around 6070 Å. At the shorter wavelengths used for the radial velocity measurements it is somewhat lower.

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