Table 3: Data for NGC 3960. ID $_{\rm {phot}}$ and BVI photometry (non corrected for differential reddening) are from Prisinzano et al. (2004). The number of exposures for each star is intended as the number of pointings with the same cross-disperser.
Star Star RA Dec B V I $J_{\rm {2MASS}}$ $K_{\rm {2MASS}}$ No. exp. RV S/N Notes
ID $_{\rm {fla}}$ ID $_{\rm {phot}}$                 (km s-1)    
c1 310753 11 50 06.330 -55 44 13.00 15.866 14.262 12.496 11.213 10.238 2 +1.83 60-80 NM
c3 310755 11 50 33.149 -55 42 36.13 14.799 13.514 12.088 11.079 10.357 2 -24.16 120-130 M
c4 310756 11 50 28.184 -55 41 36.66 14.366 13.194 11.907 10.989 10.304 2 -22.39 95-115 M
c5 310757 11 50 36.050 -55 42 05.40 14.323 13.062 11.679 10.671 9.959 2 -21.94 110-130 M
c6 310758 11 50 26.750 -55 40 28.20 14.084 12.945 11.697 10.815 10.133 4 -21.86 115-160 M
c8 310760 11 50 37.621 -55 40 15.19 14.224 13.060 11.758 10.820 10.162 2 -32.87 120-190 bin, M
c9 310761 11 50 38.100 -55 39 44.50 14.309 13.100 11.787 10.839 10.151 2 -22.58 100-110 M


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