Evaluating the stability of atmospheric lines with HARPS

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Table 1:

The summary of the data set properties for the stars used in this paper. Note that the S/N is calculated at the center of order 60.
Target	$\char93$ of observations	$\char93$ of days with observations	$\overline{{\rm\char93 observations/day}}$	Time span [d]	$\overline{{\rm S/N}}$
Tau Ceti	5270	110	47.9	2308	260
$\mu$ Ara	2868	117	24.5	2303	176
e Eri	1527	104	14.7	2217	316

Source LaTeX | All tables | In the text

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