Table 4: Orbital solutions for two slightly overlapping subsets of older and more recent primary RVs to test the possibility of a secular change of the orbital period.

Time interval	No. of	P
(HJD-2 400 000)	RVs	(d)
13 743-34 975	104	137.9449 0.0075
29 500-53 674	124	137.9257 0.0060

Source LaTeX | All tables | In the text