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

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Table 4:

Data subset used for the frequency analysis.
Date	JD $_{\rm first}$	JD $_{\rm last}$	N $_{\rm spec}$	Duration
(1)	(2)	(3)	(4)	(5)
Jan. 12	3747.9537	3748.1607	26	4.97
Jan. 13	3749.0013	3749.1099	13	2.60
Jan. 14	3749.8911	3749.9411	6	1.20
Jan. 15	3751.0417	3751.1838	16	3.41
Jan. 16	3751.8958	3752.1861	28	6.97
Jan. 18	3753.9037	3754.1257	16	5.33
Jan. 19	3754.9015	3754.9259	8	1.32
Jan. 20	3756.0609	3756.1912	16	3.13
Jan. 22	3757.9004	3758.1621	32	6.28
Total			161	35.2

(1) Date (2006); (2) Julian date (2 450 000+) of the first; and (3) last observation of the night;
(4) number of spectra; and (5) summed exposure time (hrs) of the night.

Source LaTeX | All tables | In the text

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