Table 1: FLAMES heliocentic radial velocities $\varv $ of globular clusters in Leo I: for each of the 42 confirmed GCs, $\varv $ and its error estimated by fxcor are the median values over the ÉLODIE templates (ordered by projected distance to NGC 3379, R in arcsec; the position angle $\theta $ is counted in degrees from 0 to 90, N to E). Numbering is from Rhode & Zepf (2004) as well as the $\varV $ magnitudes, $\varB -\varV $ and $\varV -\varR $ colours. Equatorial J2000.0 coordinates should be accurate to $\lesssim $0 $.\!\!^{\prime\prime}$2 with respect to the GSC2.2. The Tonry & Davis (1979) cross-correlation coefficient  $\mathcal{R}_{_{\rm CCF}}$ is the median value over the ÉLODIE templates. Class B objects are commented, as well as the 10 GCs in common with Puzia et al. (2004) with their velocity estimate. Full tables of all MEDUSA targets - including stars and galaxies/unclassified objects - are available online.
Id $_{\rm {RZ04}}$ $\alpha~$(J2000.0) $\delta\ $(J2000.0) $R~\hbox{$^{\prime\prime}$ }$ $\theta~\hbox{$^\circ$ }$ $\varV $ $\varB -\varV $ $\varV -\varR $ $\mathcal{R}_{_{\rm CCF}}$ $\varv\pm\delta\varv$  (km s-1) Comments
gc771 10$^{\rm h}$47$^{\rm m}$50 $.\!\!^{\rm s}$62 12 $\hbox{$^\circ$ }$35$^\prime$31 $.\!\!^{\prime\prime}$9 39 20 21.26 0.68 0.52 6.0 758 $\pm $ 9 Puzia23 at 791 km s-1
gc830 10$^{\rm h}$47$^{\rm m}$47 $.\!\!^{\rm s}$71 12 $\hbox{$^\circ$ }$34$^\prime$14 $.\!\!^{\prime\prime}$5 49 217 21.11 0.85 0.59 16.4 926 $\pm $ 5  
gc820 10$^{\rm h}$47$^{\rm m}$48 $.\!\!^{\rm s}$18 12 $\hbox{$^\circ$ }$35$^\prime$44 $.\!\!^{\prime\prime}$9 55 336 20.94 0.75 0.49 9.9 889 $\pm $ 6 Puzia27 at 911 km s-1
gc764 10$^{\rm h}$47$^{\rm m}$51 $.\!\!^{\rm s}$07 12 $\hbox{$^\circ$ }$35$^\prime$49 $.\!\!^{\prime\prime}$1 58 21 20.00 0.72 0.52 18.7 776 $\pm $ 4 Puzia24 at 801 km s-1
gc839 10$^{\rm h}$47$^{\rm m}$47 $.\!\!^{\rm s}$19 12 $\hbox{$^\circ$ }$34$^\prime$04 $.\!\!^{\prime\prime}$6 62 217 21.98 0.69 0.46 6.7 1064 $\pm $ 13  
gc774 10$^{\rm h}$47$^{\rm m}$50 $.\!\!^{\rm s}$40 12 $\hbox{$^\circ$ }$33$^\prime$47 $.\!\!^{\prime\prime}$7 67 171 21.36 0.68 0.50 5.3 656 $\pm $ 9 Puzia14 at 645 km s-1
gc728 10$^{\rm h}$47$^{\rm m}$53 $.\!\!^{\rm s}$42 12 $\hbox{$^\circ$ }$34$^\prime$12 $.\!\!^{\prime\prime}$2 69 127 21.83 0.81 0.44 5.2 978 $\pm $ 15 Puzia13 at 941 km s-1
gc741 10$^{\rm h}$47$^{\rm m}$52 $.\!\!^{\rm s}$60 12 $\hbox{$^\circ$ }$35$^\prime$59 $.\!\!^{\prime\prime}$6 78 34 21.27 0.97 0.59 9.6 1188 $\pm $ 6  
gc740 10$^{\rm h}$47$^{\rm m}$52 $.\!\!^{\rm s}$65 12 $\hbox{$^\circ$ }$33$^\prime$37 $.\!\!^{\prime\prime}$9 88 150 21.85 1.07 0.52 6.2 889 $\pm $ 7 Puzia12 at 867 km s-1
gc719 10$^{\rm h}$47$^{\rm m}$53 $.\!\!^{\rm s}$83 12 $\hbox{$^\circ$ }$33$^\prime$46 $.\!\!^{\prime\prime}$2 92 138 21.51 0.65 0.52 4.4 740 $\pm $ 10 Puzia11 at 705 km s-1; class B
gc709 10$^{\rm h}$47$^{\rm m}$54 $.\!\!^{\rm s}$19 12 $\hbox{$^\circ$ }$36$^\prime$31 $.\!\!^{\prime\prime}$5 118 35 20.97 0.72 0.50 13.0 954 $\pm $ 4  
gc682 10$^{\rm h}$47$^{\rm m}$56 $.\!\!^{\rm s}$72 12 $\hbox{$^\circ$ }$33$^\prime$26 $.\!\!^{\prime\prime}$4 137 130 20.47 0.63 0.48 8.1 1137 $\pm $ 6 Puzia09 at 1130 km s-1
gc923 10$^{\rm h}$47$^{\rm m}$41 $.\!\!^{\rm s}$91 12 $\hbox{$^\circ$ }$36$^\prime$11 $.\!\!^{\prime\prime}$2 139 303 21.97 0.75 0.57 4.0 999 $\pm $ 14 Class B
gc925 10$^{\rm h}$47$^{\rm m}$41 $.\!\!^{\rm s}$87 12 $\hbox{$^\circ$ }$33$^\prime$31 $.\!\!^{\prime\prime}$0 144 235 21.18 0.99 0.56 13.2 1048 $\pm $ 4  
gc948 10$^{\rm h}$47$^{\rm m}$40 $.\!\!^{\rm s}$34 12 $\hbox{$^\circ$ }$35$^\prime$54 $.\!\!^{\prime\prime}$9 152 293 20.25 0.66 0.38 6.8 1264 $\pm $ 9 Puzia33 at 1310 km s-1
gc958 10$^{\rm h}$47$^{\rm m}$39 $.\!\!^{\rm s}$34 12 $\hbox{$^\circ$ }$33$^\prime$59 $.\!\!^{\prime\prime}$1 164 250 21.57 0.74 0.42 4.4 951 $\pm $ 8 Class B
gc634 10$^{\rm h}$48$^{\rm m}$02 $.\!\!^{\rm s}$13 12 $\hbox{$^\circ$ }$35$^\prime$57 $.\!\!^{\prime\prime}$3 196 71 20.97 0.77 0.46 7.0 950 $\pm $ 6  
gc971 10$^{\rm h}$47$^{\rm m}$38 $.\!\!^{\rm s}$75 12 $\hbox{$^\circ$ }$36$^\prime$47 $.\!\!^{\prime\prime}$8 199 305 21.78 0.83 0.47 4.4 1027 $\pm $ 13 Class B
gc949 10$^{\rm h}$47$^{\rm m}$40 $.\!\!^{\rm s}$33 12 $\hbox{$^\circ$ }$37$^\prime$24 $.\!\!^{\prime\prime}$1 205 317 21.81 0.69 0.43 3.0 933 $\pm $ 27 Class B
gc645 10$^{\rm h}$48$^{\rm m}$00 $.\!\!^{\rm s}$52 12 $\hbox{$^\circ$ }$32$^\prime$46 $.\!\!^{\prime\prime}$9 206 128 21.02 0.78 0.48 7.5 654 $\pm $ 6 Puzia05 at 632 km s-1
gc960 10$^{\rm h}$47$^{\rm m}$39 $.\!\!^{\rm s}$25 12 $\hbox{$^\circ$ }$32$^\prime$25 $.\!\!^{\prime\prime}$6 216 226 20.06 0.81 0.49 14.9 899 $\pm $ 5  
gc946 10$^{\rm h}$47$^{\rm m}$40 $.\!\!^{\rm s}$46 12 $\hbox{$^\circ$ }$31$^\prime$36 $.\!\!^{\prime\prime}$4 241 215 21.67 0.65 0.36 4.3 739 $\pm $ 6 Class B
gc984 10$^{\rm h}$47$^{\rm m}$37 $.\!\!^{\rm s}$80 12 $\hbox{$^\circ$ }$31$^\prime$52 $.\!\!^{\prime\prime}$7 254 224 20.86 0.82 0.49 7.8 1130 $\pm $ 5  
gc573 10$^{\rm h}$48$^{\rm m}$07 $.\!\!^{\rm s}$19 12 $\hbox{$^\circ$ }$37$^\prime$55 $.\!\!^{\prime\prime}$1 318 55 20.94 0.95 0.57 13.0 752 $\pm $ 4 NGC 3384 cluster?
gc581 10$^{\rm h}$48$^{\rm m}$06 $.\!\!^{\rm s}$60 12 $\hbox{$^\circ$ }$30$^\prime$58 $.\!\!^{\prime\prime}$5 346 133 21.82 0.98 0.58 3.9 1064 $\pm $ 11 Class B
gc571 10$^{\rm h}$48$^{\rm m}$07 $.\!\!^{\rm s}$40 12 $\hbox{$^\circ$ }$39$^\prime$24 $.\!\!^{\prime\prime}$1 378 45 21.25 0.73 0.50 5.9 792 $\pm $ 9 NGC 3384 cluster?
gc482a 10$^{\rm h}$48$^{\rm m}$13 $.\!\!^{\rm s}$88 12 $\hbox{$^\circ$ }$37$^\prime$14 $.\!\!^{\prime\prime}$1 388 69 21.59 1.00 0.63 17.6 908 $\pm $ 6 NGC 3384 cluster
gc454 10$^{\rm h}$48$^{\rm m}$15 $.\!\!^{\rm s}$73 12 $\hbox{$^\circ$ }$35$^\prime$54 $.\!\!^{\prime\prime}$2 394 81 21.89 1.06 0.62 6.1 874 $\pm $ 8 NGC 3384 cluster
gc461 10$^{\rm h}$48$^{\rm m}$15 $.\!\!^{\rm s}$36 12 $\hbox{$^\circ$ }$36$^\prime$58 $.\!\!^{\prime\prime}$0 404 72 21.87 0.71 0.45 9.4 847 $\pm $ 17 NGC 3384 cluster
gc670 10$^{\rm h}$47$^{\rm m}$58 $.\!\!^{\rm s}$08 12 $\hbox{$^\circ$ }$28$^\prime$11 $.\!\!^{\prime\prime}$2 422 163 20.37 0.72 0.44 7.4 921 $\pm $ 6  
gc442 10$^{\rm h}$48$^{\rm m}$16 $.\!\!^{\rm s}$81 12 $\hbox{$^\circ$ }$37$^\prime$04 $.\!\!^{\prime\prime}$0 426 72 21.15 0.74 0.51 7.7 878 $\pm $ 11 NGC 3384 cluster
gc449 10$^{\rm h}$48$^{\rm m}$16 $.\!\!^{\rm s}$20 12 $\hbox{$^\circ$ }$38$^\prime$30 $.\!\!^{\prime\prime}$6 452 61 20.97 0.80 0.54 15.8 672 $\pm $ 4 NGC 3384 cluster
gc387 10$^{\rm h}$48$^{\rm m}$20 $.\!\!^{\rm s}$06 12 $\hbox{$^\circ$ }$37$^\prime$15 $.\!\!^{\prime\prime}$5 476 73 21.98 0.83 0.44 5.4 704 $\pm $ 11 NGC 3384 cluster
ad1102 10$^{\rm h}$48$^{\rm m}$10 $.\!\!^{\rm s}$29 12 $\hbox{$^\circ$ }$40$^\prime$57 $.\!\!^{\prime\prime}$9 476 40 19.28 0.75 0.50 23.8 920 $\pm $ 3 NGC 3384 cluster?
gc683 10$^{\rm h}$47$^{\rm m}$56 $.\!\!^{\rm s}$61 12 $\hbox{$^\circ$ }$26$^\prime$30 $.\!\!^{\prime\prime}$2 514 168 21.14 0.70 0.39 4.4 1087 $\pm $ 14  
gc351 10$^{\rm h}$48$^{\rm m}$23 $.\!\!^{\rm s}$34 12 $\hbox{$^\circ$ }$36$^\prime$57 $.\!\!^{\prime\prime}$7 519 76 21.60 1.02 0.49 3.9 739 $\pm $ 17 NGC 3384 cluster
gc358 10$^{\rm h}$48$^{\rm m}$22 $.\!\!^{\rm s}$79 12 $\hbox{$^\circ$ }$38$^\prime$44 $.\!\!^{\prime\prime}$2 546 65 21.35 0.59 0.46 5.6 577 $\pm $ 13 NGC 3384 cluster
ad1021 10$^{\rm h}$48$^{\rm m}$13 $.\!\!^{\rm s}$33 12 $\hbox{$^\circ$ }$42$^\prime$24 $.\!\!^{\prime\prime}$8 573 38 21.71 0.99 0.52 5.3 752 $\pm $ 7 NGC 3384 cluster?
gc756 10$^{\rm h}$47$^{\rm m}$51 $.\!\!^{\rm s}$58 12 $\hbox{$^\circ$ }$45$^\prime$40 $.\!\!^{\prime\prime}$2 646 2 20.87 0.58 0.47 3.7 725 $\pm $ 19 Class B
gc368 10$^{\rm h}$48$^{\rm m}$22 $.\!\!^{\rm s}$19 12 $\hbox{$^\circ$ }$44$^\prime$00 $.\!\!^{\prime\prime}$3 731 42 21.15 0.82 0.44 4.6 1098 $\pm $ 10  
ad1481 10$^{\rm h}$47$^{\rm m}$52 $.\!\!^{\rm s}$08 12 $\hbox{$^\circ$ }$21$^\prime$45 $.\!\!^{\prime\prime}$2 790 177 19.39 0.52 0.43 7.0 1105 $\pm $ 6  
gc185 10$^{\rm h}$48$^{\rm m}$38 $.\!\!^{\rm s}$75 12 $\hbox{$^\circ$ }$27$^\prime$09 $.\!\!^{\prime\prime}$3 870 122 21.09 0.64 0.37 4.8 964 $\pm $ 10  

a $\equiv$ Brodie & Larsen (2002) N3384-FF-7 "fuzzy'' cluster. They found $\varv = 905\pm 23$ km s-1 (red channel value) using Keck / LRIS.

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