Canis Major 49 20.0 3.0 ... ... ... ... ... ... ... ... (1) H I measurements complex due to location! Sagittarius dSph 21 11.4 0.7 N/A N/A N/A^b N/A N/A N/A N/A 190 (2) (3) (4) (5) Segue (I) 0.00034 3.9^c 0.8 N/A N/A N/A N/A N/A N/A N/A 0.26 (6) (5) Stellar velocity gradient constrained to <5 km s^-1 at 90% confidence Ursa Major II 0.0041 6.7 1.4 N/A N/A N/A N/A N/A N/A N/A 3.9 (7) (5) Velocity difference of 8.4 +or- 1.4 km s^-1 between stars in the east and west Bootes II 0.0010 10.5 7.4 ... ... N/A N/A N/A N/A N/A 3.3 (8) (5) Segue II 0.00086 3.4 ^+2.5 ... ... ... ... ... ... ... 0.23 (9) Willman 1 0.0010 4.3 ^+2.3 ... ... N/A N/A N/A N/A N/A 0.27 (10) (5) Coma Berenices 0.0037 4.6 0.8 N/A N/A N/A N/A N/A N/A N/A 0.94 (7) (5) Stellar velocity gradient of 5.5 +or- 1.2 km s^-1 deg^-1 Bootes III 0.017 14.0 3.2 ... ... ... ... ... ... ... ... (11) LMC 1500 20.2 0.5 49.8 15.9 460 15.8 0.2 63.0 3.0 (12) (13) (14) Stellar velocities based on carbon stars; H I boundaries between LMC, SMC, bridge, and interface regions not clearly defined SMC 460 27.6 0.5 N/A N/A 460 22.0^d 2.0 60.0 5.0 (15) (16) (14) Stellar velocities based on red giant branch stars; stellar velocity gradient of 8.3 km s^-1 deg^-1; H I boundaries between LMC, SMC, bridge, and interface regions not clearly defined Bootes (I) 0.029 2.4 ^+0.9 ... ... N/A N/A N/A N/A N/A 0.81 (17) (5) Stellar velocity dispersion corresponds to dominant component, and there is evidence for a hotter component with sigma* ~ 9 km s^-1 Draco 0.29 9.1 1.2 N/A N/A N/A N/A N/A N/A N/A 11 (18) (19) (5) Ursa Minor 0.29 9.5 1.2 N/A N/A N/A N/A N/A N/A N/A 9.5 (20) (19) (5) Sculptor 2.3 9.2 1.4 N/A N/A 0.22^e N/A N/A N/A N/A 14 (21) (22) (23) (5) Stellar velocity gradient of 5.5 +or- 0.5 km s^-1 deg^-1 Sextans (I) 0.44 7.9 1.3 N/A N/A N/A N/A N/A N/A N/A 25 (21) (22) (5) Ursa Major (I) 0.014 7.6 1.0 ... ... N/A N/A N/A N/A N/A 11 (7) (5) Carina 0.38 6.6 1.2 N/A N/A N/A N/A N/A N/A N/A 6.3 (21) (22) (5) Stellar velocity gradient of 2.5 +or- 0.8 km s^-1 deg^-1 Hercules 0.037 3.7 0.9 ... ... N/A N/A N/A N/A N/A 2.6 (24) (5) Fornax 20 11.7 0.9 N/A N/A 0.17^f N/A N/A N/A N/A 56 (21) (22) (25) (5) Stellar velocity gradient of 6.3 +or- 0.2 km s^-1 deg^-1 Leo IV 0.019 3.3 1.7 ... ... N/A N/A N/A N/A N/A 1.3 (7) (5) Canes Venatici II 0.0079 4.6 1.0 ... ... N/A N/A N/A N/A N/A 0.91 (7) (5) Leo V 0.011 3.7 ^+2.3 ... ... N/A N/A N/A N/A N/A 1.1 (26) (27) (5) Pisces II 0.0086 ... ... ... ... ... ... ... ... ... ... Canes Venatici (I) 0.23 7.6 0.4 ... ... N/A N/A N/A N/A N/A 19 (7) (5) Leo II 0.74 6.6 0.7 ... ... N/A N/A N/A N/A N/A 4.6 (18) (5) Leo I 5.5 9.2 1.4 N/A N/A N/A N/A N/A N/A N/A 12 (28) (5) M32 320 92.0 5.0 55.0 3.0 N/A N/A N/A N/A N/A 540 (29) (5) Stellar velocity dispersion rises rapidly toward center and presents strong evidence for a supermassive black hole (e.g., see also van der Marel et al. 1997) Andromeda IX 0.15 4.5 3.6 ... ... N/A N/A N/A N/A N/A 6.5 (30) (5) NGC 205 330 35.0 5.0 11.0 5.0 0.40 16.1^g N/A N/A 420 (31) (32) H I velocity gradient of ~42 km s^-1 measured over ~3 arcmin Andromeda XVII 0.26 ... ... ... ... N/A N/A N/A N/A N/A ... (5) Andromeda I 3.9 10.6 1.1 ... ... N/A N/A N/A N/A N/A 44 (33) (5) Andromeda XXVII 0.12 ... ... ... ... ... ... ... ... ... ... Andromeda III 0.83 4.7 1.8 ... ... N/A N/A N/A N/A N/A 6.1 (33) (34)^h; (5) Andromeda XXV 0.68 ... ... ... ... ... ... ... ... ... ... Andromeda XXVI 0.060 ... ... ... ... ... ... ... ... ... ... Andromeda XI 0.049 100 AGB stars. Cetus 2.6 17.0^j 2.0 7.7 1.2 N/A N/A N/A N/A N/A 120 (47) (5) Tentative stellar velocity gradient across minor axis of 7.7 +or- 1.2 km s^-1; unassociated with nearby H I cloud Pegasus dIrr 6.61 ... ... ... ... 5.9 <9.0 21.0: ... (48) (49) Leo T 0.14 7.5 1.6 ... ... 0.28 6.9 1.0 N/A N/A 3.9 (7) (50) WLM 43 17.5 2.0 20.8 2.0 61 4.5 1.0 30.0 3.0 380 (51) (52) Leo A 6.0 9.3 1.3 N/A N/A 11 9.3 1.4 N/A N/A 25 (53) (54) Stellar kinematics derived using 10 young B supergiants + H II regions; H I gradient of ~1.3 km s^-1 arcmin^-1 Andromeda XVIII 0.63 ... ... ... ... ... ... ... ... ... ... Aquarius 1.6 ... ... ... ... 4.1 5.8 0.1 N/A N/A ... (48) H I velocity gradient of 6 km s^-1 arcmin^-1. Tucana 0.56 15.8 ^+4.1 N/A N/A N/A N/A N/A N/A N/A 41 (55) (5) Stellar velocity gradient of ~16 km s^-1 over ~2 x r_h; unlikely associated with nearby H I cloud Sagittarius dIrr 3.5 ... ... ... ... 8.8 10.0 1.0 N/A N/A ... (41) UGC 4879 8.3 ... ... ... ... 0.95 11.0 1.1 N/A N/A ... (56) NGC 3109 76 ... ... ... ... 450 10.0: 72.4 0.5 ... (57) (58) (59) Sextans B 52 ... ... ... ... 51 <18.0 71: (60) (49) Antlia 1.3 ... ... ... ... 0.73 6.4 0.7 N/A N/A ... (58) Sextans A 44 ... ... ... ... 77 8.0 1.0 20.0 2.0 ... (61) HIZSS 3(A) ... ... ... ... ... 14 ... ... 42.0 4.0 ... (62) HIZSS 3B ... ... ... ... ... 2.6 ... ... N/A N/A ... (62) H I velocity gradient of ~2.5 km s^-1 arcmin^-1 KKR 25 1.4 ... ... ... ... ... ... ... ... ... ... See Huchtmeier et al. (2000) for attempted H I observations ESO 410- G 005 3.5 ... ... ... ... 0.73 14.2 0.6 ... ... ... (63) NGC 55 2200 ... ... ... ... 1300 ... ... 86.0 6.0 ... (64) Castro et al. (2008) obtain stellar velocities for ~200 massive blue stars and find that their kinematics closely trace the H I rotation curve ESO 294- G 010 2.7 ... ... ... ... 0.34 9.7 0.9 ... ... ... (63) NGC 300 2100 ... ... ... ... 1800 13.0 5.0 98.8 3.1 ... (65) (66) H I velocity dispersion shows significant spatial variation IC 5152 270 ... ... ... ... 87 ... ... ... ... ... (45) H I line widths available in Koribalski et al. (2004) KKH 98 4.5 ... ... ... ... 6.6 ... ... ... ... ... (67) H I line widths available in Begum et al. (2008b) and Huchtmeier et al. (2003) UKS 2323-326 17 ... ... ... ... 17: ... ... ... ... ... (68) See also Huchtmeier & Richter (1986); H I line widths available in Longmore et al. (1982) and Huchtmeier & Richter (1986) KKR 3 0.54 ... ... ... ... 2.5 7.5 0.5 N/A N/A ... (69) H I velocity gradient of ~3.3 km s^-1 arcmin^-1 GR 8 6.4 ... ... ... ... 11 7.0 0.2 N/A N/A ... (48) Lumpy H I velocity distribution, with some evidence of an overall velocity gradient UGC 9128 7.8 ... ... ... ... 18 <15.0 56.0: ... (49) See also Begum et al. (2008b) UGC 8508 19 ... ... ... ... 29 ... ... 31.2 2.3 ... (67) (70) IC 3104 62 ... ... ... ... 13 ... ... ... ... ... (45) H I line widths available in Koribalski et al. (2004) DDO 125 47 ... ... ... ... 35 7.3 1.5 11.2 2.7 ... (71) (72) H I rotational velocity measured at r = 2 arcmin; see also Huchtmeier et al. (2003), Begum et al. (2008b), and Swaters et al. (2009) UGCA 86 16 ... ... ... ... 860 8.8 1.0 122.0 5.0 ... (73) H I structure consists of a rotating disk and a kinematically distinct, elongated "spur" DDO 99 16 ... ... ... ... 52 ... ... ... ... ... (67) H I line widths available in Begum et al. (2008b) IC 4662 190 ... ... ... ... 180 ... ... ... ... ... (45) H I line widths available in Koribalski et al. (2004) DDO 190 51 ... ... ... ... 43 10.0 2.4 24.7 2.5 ... (71) (72) H I rotational velocity measured at r = 1.5 arcmin KKH 86 0.82 ... ... ... ... 0.88 ... ... ... ... ... (74) H I line widths available in Karachentsev et al. (2001a) NGC 4163 37 ... ... ... ... 7.9 <7.4 8.7: ... (75) DDO 113 2.1 ... ... ... ... 48^k ... ... ... ... ... (76) H I line widths available in Huchtmeier & Richter (1986)