| Galaxy | Other Name | α2000 | δ2000 | l | b | Type | Notes |
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
| WLM | DDO 221 | 00 01 58 | -15 27.8 | 75.9 | -73.6 | IrrIV-V | |
| NGC 55 | 00 15 08 | -39 13.2 | 332.7 | -75.7 | IrrIV | ||
| IC 10 | UGC 192 | 00 20 25 | +59 17.5 | 119.0 | -3.3 | dIrr | |
| NGC 147 | DDO 3 | 00 33 12 | +48 30.5 | 119.8 | -14.3 | dSph/dE5 | |
| And III | 00 35 17 | +36 30.5 | 119.3 | -26.2 | dSph | ||
| NGC 185 | UGC 396 | 00 38 58 | +48 20.2 | 120.8 | -14.5 | dSph/dE3p | |
| NGC 205 | M110 | 00 40 22 | +41 41.4 | 120.7 | -21.1 | E5p/dSph-N | E |
| M32 | NGC 221 | 00 42 42 | +40 51.9 | 121.2 | -22.0 | E2 | |
| M31 | NGC 224 | 00 42 44 | +41 16.1 | 121.2 | -21.6 | SbI-II | |
| And I | 00 45 43 | +38 00.4 | 121.7 | -24.9 | dSph | ||
| SMC | NGC 292 | 00 52 44 | -72 49.7 | 302.8 | -44.3 | IrrIV-V | |
| Sculptor | 01 00 09 | -33 42.5 | 287.5 | -83.2 | dSph | ||
| LGS 3 | Pisces | 01 03 53 | +21 53.1 | 126.8 | -40.9 | dIrr/dSph | |
| IC 1613 | DDO 8 | 01 04 54 | +02 08.0 | 129.8 | -60.6 | IrrV | |
| And II | 01 16 27 | +33 25.7 | 128.9 | -29.2 | dSph | A | |
| M33 | NGC 598 | 01 33 51 | +30 39.6 | 133.6 | -31.3 | ScII-III | |
| Phoenix | 01 51 06 | -44 26.7 | 272.2 | -68.9 | dIrr/dSph | ||
| Fornax | 02 39 59 | -34 27.0 | 237.1 | -65.7 | dSph | ||
| EGB 0427+63 | UGCA 92 | 04 32 01 | +63 36.4 | 144.7 | +10.5 | dIrr | |
| LMC | 05 23 34 | -69 45.4 | 280.5 | -32.9 | IrrIII-IV | ||
| Carina | 06 41 37 | -50 58.0 | 260.1 | -22.2 | dSph | ||
| Leo A | DDO 69 | 09 59 24 | +30 44.7 | 196.9 | +52.4 | dIrr | |
| Sextans B | DDO 70 | 10 00 00 | +05 19.7 | 233.2 | +43.8 | dIrr | |
| NGC 3109 | DDO 236 | 10 03 07 | -26 09.5 | 262.1 | +23.1 | IrrIV-V | |
| Antlia | 10 04 04 | -27 19.8 | 263.1 | +22.3 | dIrr/dSph | B | |
| Leo I | DDO 74 | 10 08 27 | +12 18.5 | 226.0 | +49.1 | dSph | |
| Sextans A | DDO 75 | 10 11 06 | -04 42.5 | 246.2 | +39.9 | dIrr | |
| Sextans | 10 13 03 | -01 36.9 | 243.5 | +42.3 | dSph | ||
| Leo II | DDO 93 | 11 13 29 | +22 09.2 | 220.2 | +67.2 | dSph | |
| GR 8 | DDO 155 | 12 58 40 | +14 13.0 | 310.7 | +77.0 | dIrr | |
| Ursa Minor | DDO 199 | 15 09 11 | +67 12.9 | 105.0 | +44.8 | dSph | |
| Draco | DDO 208 | 17 20 19 | +57 54.8 | 86.4 | +34.7 | dSph | |
| Milky Way | 17 45 40 | -29 00.5 | 0.0 | 0.0 | Sbc | ||
| Sagittarius | 18 55 03 | -30 28.7 | 5.6 | -14.1 | dSph-N | E | |
| SagDIG | UKS 1927-177 | 19 29 59 | -17 40.7 | 21.1 | -16.3 | dIrr | |
| NGC 6822 | DDO 209 | 19 44 56 | -14 48.1 | 25.3 | -18.4 | IrrIV-V | |
| DDO 210 | Aquarius | 20 46 46 | -12 51.0 | 34.0 | -31.3 | dIrr/dSph | C |
| IC 5152 | 22 02 42 | -51 17.7 | 343.9 | -50.2 | dIrr | ||
| Tucana | 22 41 50 | -64 25.2 | 322.9 | -47.4 | dSph | D | |
| UKS 2323-326 | UGCA 438 | 23 26 27 | -32 23.3 | 11.9 | -70.9 | dIrr | |
| Pegasus | DDO 216 | 23 28 34 | +14 44.8 | 94.8 | -43.5 | dIrr/dSph | |
EXPLANATION OF COLUMNS OF TABLE 1:
Column 1: Galaxy name. Entries denoted in italics refer to the five giant Local Group galaxies that are not discussed in this review in any detail; Columns 2: A common alternative name; Columns 3 and 4: Right ascension and declination for epoch J2000.0, respectively; Columns 5 and 6: Galactic longitude and latitude, respectively; Column 7: Galaxy type following van den Bergh (1994a); Column 10: Special notes.
NOTES FOR TABLE 1:
A. The position listed here is based on an independent measurement by Paul Hodge (private communication).
B. Also known as PGC 29194 (Fouqué et al 1990) before it was re-discovered as a probable Local Group member by Whiting et al (1997). A thorough discussion of `pre-discovery' observations of Antlia is provided by Aparicio et al (1997a).
C. Marconi et al (1990) claimed that the original position of DDO 210 (Fisher and Tully 1975) was significantly in error. However, Lo et al (1993) noted that the original position seemed to be correct, and Marconi et al (1995) subsequently agreed. The position listed here corresponds to the original one from Fisher and Tully (1975).
D. Tucana was known prior to its re-discovery by Lavery and Mighell (1992) who thoroughly document all listings of the galaxy in earlier catalogs. Lavery and Mighell (1992) did first claim Tucana to be a possible Local Group member.
E. The `N' suffix has been added to indicate that these systems may be nucleated dwarfs.
REFERENCES FOR TABLE 1: [1] Sandage & Carlson (1985b); [2] Lautsen et al (1977); [3] Hummel et al (1986); [4] Puche et al (1991); [5] de Vaucouleurs & Ables (1965); [6] Shostak & Skillman (1989); [7] Young & Lo (1997a); [8] Caldwell et al (1992); [9] Kent (1987); [10] Hodge (1981); [11] de Vaucouleurs & Freeman (1972); [12] Mathewson & Ford (1984); [13] Carignan et al (1998); [14] Young & Lo (1997b); [15] Ables (1971); [16] Lake & Skillman (1989); [17] Sandage (1961); [18] Corbelli et al (1989); [19] van de Rydt et al (1991); [20] Carignan et al (1991); [21] Hodge (1971); [22] Saha & Hoessel (1991); [23] Hoessel et al (1988); [24] Smecker-Hane et al (1994); [25] Sandage (1986b); [26] Young & Lo (1996a); [27] Sandage & Carlson (1985a); [28] Skillman et al (1988); [29] Sandage & Carlson (1988); [30] Jobin & Carignan (1990); [31] Whiting et al (1997); [32] Hodge (1963a); [33] Sandage & Carlson (1982); [34] Mateo et al (1995a); [35] Deleted; [36] Fisher & Tully (1979); [37] Carignan et al (1990); [38] van Agt (1967); [39] Baade & Swope (1961); [40] Ibata et al (1997); [41] Longmore et al (1978); [42] Hodge (1978); [43] Gottesman & Weliachew (1977); [44] Lo et al (1993); [45] Deleted; [46] Deleted; [47] Lavery & Mighell (1992); [48] Oosterloo et al (1996); [49] van Agt (1978); [50] Hodge (1992a); [51] Sandage & Bedke (1994); [52] Vogt et al (1995); [53] Cesarsky et al (1977); [54] Hopp & Schulte-Ladbeck (1995).