Discovery of non-radial pulsations in the spectroscopic binary Herbig Ae star RS Chamaeleontis

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Table 2:

Log of the observations at Mt John Observatory, NZ, in Jan. 2006.
Date	JD $_{\rm first}$	JD $_{\rm last}$	$N_{\rm spec}$	S/N $_{\rm Range}$
(1)	(2)	(3)	(4)	(5)
Jan. 09	3745.0101		1	120
Jan. 10	3745.9544	3745.9733	2	80-100
Jan. 12	3747.9537	3748.1779	28	70-90
Jan. 13	3749.0013	3749.1930	23	100-120
Jan. 14	3749.8911	3749.9911	12	70-90
Jan. 15	3750.8921	3751.1919	31	150
Jan. 16	3751.8958	3752.1970	29	90-120
Jan. 19	3754.9015	3755.2006	33	100-130
Jan. 20	3755.9245	3756.1993	25	90-120
Jan. 21	3756.9068	3757.0386	14	60-150
Jan. 22	3757.9004	3758.1621	32	120-170

(1) Date of the observation; (2) Julian date (mean observation, 2 450 000+) of the first and (3) last stellar spectrum of the night, respectively; (4) Number of spectra; (5) typical range of S/N (pixel^-1) at 550 nm.

Source LaTeX | All tables | In the text

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