Table 2: Observation log of NGC 3960. One star is common to configurations A and B; we consider only clump objects here (7 stars in total). The remaining fibers were assigned to sky and to MS stars.
Date UT $_{\rm {beginning}}$ Exposure time Configuration Grating No. of stars

(s) (clump)

2004-04-03 02 57 39.980 2595 A CD4 4

2004-04-03 03 52 16.186 2595 A CD4 4

2004-04-03 04 47 31.818 2595 A CD3 4

2004-04-20 03 37 39.635 2595 B CD3 4

2004-05-02 00 12 31.740 2595 B CD4 4

2004-05-02 00 57 37.007 2595 B CD4 4

2004-05-02 01 43 13.805 2595 B CD3 4

2004-05-02 02 39 18.200 2595 A CD3 4

**Table 2:** Observation log of NGC 3960. One star is common to configurations A and B; we consider only clump objects here (7 stars in total). The remaining fibers were assigned to sky and to MS stars.
Date	UT $_{\rm {beginning}}$	Exposure time	Configuration	Grating	No. of stars
		(s)			(clump)
2004-04-03	02 57 39.980	2595	A	CD4	4
2004-04-03	03 52 16.186	2595	A	CD4	4
2004-04-03	04 47 31.818	2595	A	CD3	4
2004-04-20	03 37 39.635	2595	B	CD3	4
2004-05-02	00 12 31.740	2595	B	CD4	4
2004-05-02	00 57 37.007	2595	B	CD4	4
2004-05-02	01 43 13.805	2595	B	CD3	4
2004-05-02	02 39 18.200	2595	A	CD3	4

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