This is The Southern Galaxy Catalogue, version 1.21, dated November 1993. The distribution includes seven files: sgc12.01 -- SGC, 00 hr to 07 hr 43 min sgc12.02 -- SGC, 07 hr 43 min to 18 hr 29 min sgc12.03 -- SGC, 18 hr 29 min to 23 hr 59 min sgc12.xmp -- a short example file for SGC. bugs.sgc -- Errata (all errors listed have been corrected in this version) sgc12.txt -- SGC, complete sgcdoc.txt -- This file. All are available as 7-bit ASCII files with UNIX line endings. MS-DOS versions of the first five files are in the zipped archive sgc.zip. Both versions contain identical data. Here is the format, identical to that in the printed version. RA (1950.0) Dec l N/I/A Type T n_T L n_L logD logR nD (2000.0) b ESO w_T w_L w_D w_R 18 28 57 -56 46.2 338.53 I4719 .SAS8P. 8.0 2 6.0 1 1.38 0.12 2 33 12 -56 43.9 -20.03 183- G 2 2.0 1.0 2.0 2.0 18 28 58 -58 0.7 337.28 I4717 .S..3?/ 3.0 3 1.43 0.51 3 33 18 -57 58.4 -20.44 140- G 24 0.75 3.0 3.0 18 29 11 -58 26.6 336.86 I4720 .SBT7.. 7.0 1 6.0 1 1.66 0.35 1 33 32 -58 24.3 -20.61 140- G 25 1.0 1.0 1.0 1.0 18 29 14 -41 32.9 353.33 A1829-41 .SXT5*. 5.0 1 3.0 1 1.60 0.15 1 32 46 -41 30.6 -14.36 336- G 3 0.5 0.5 1.0 1.0 18 29 21 -60 10.0 335.12 I4718 .S..3*. 3.0 1 5.0 1 1.58 0.30 1 33 50 -60 7.7 -21.19 140- G 26 0.5 0.5 0.5 0.5 A brief explanation of the columns: Columns 1, 2, and 3, lines 1 and 2: Position, usually from ESO, sometimes not. The positions from Spellman, Madore, and Helou (PASP 101, 360, 1989) have been entered. All most all galaxies have Notes in the printed version. Column 4, lines 1 and 2: Names from NGC, IC, and RC2 (line 1); from ESO (line 2). If the galaxy is not in ESO, the Southern Sky Survey Field number alone is listed on line 2. This, or the ESO name, is followed by an "r" if there is a Remark in the printed version about the field containing the galaxy. Columns 5 and 6, line 1: Coded revised Hubble type (column 5) using the coding conventions of RC2 and RC3; and the corresponding numerical Hubble stage code, followed by the number of plates on which the type was estimated (column 6). Column 6, Line 2 contains the weight of the numerical type on an arbitrary scale from 0 (no type) to 4 or 5 (type estimated on 4 or 5 plates, with no uncertainty noted). Column 7, lines 1 and 2: Coded numerical luminosity class, followed by the number of plates on which the class was estimated (line 1), and the weight of the luminosity class (same scale as the type weight). Columns 8, 9, and 10, lines 1 and 2: Base 10 logarithm of the major axis diameter (D in units 0.1 arcmin as in RC1, 2, and 3) and its weight (column 8); the base 10 logarithm of the axis ratio (D/d) and its weight (column 9); and the number of plates on which the diameters were measured (column 10). The measured isophote is approximately 27.0 B-mag arcsec^-2. Formulae to reduce these data to the standard isophote at 25.0 B-mag arcsec^-2 are given in RC3. See the printed version (University of Texas Astronomy Department Monograph in Astronomy No. 4, 1985, by Harold G. Corwin, Jr., Antoinette de Vaucouleurs, and Gerard de Vaucouleurs) for more information and details. Latest update: 2 Dec 2012.