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VII/112             RC2 Catalogue  (de Vaucouleurs+ 1976)

The Second Reference Catalogue of bright galaxies (RC2) de Vaucouleurs G., de Vaucouleurs A., Corwin H.G. <University of Texas Press, Austin (1976)> =1976RC2...C......0D
ADC_Keywords: Galaxy catalogs Description: This standardized documentation file does not contain a complete description of the electronic version of the RC2 catalogue; please refer to the "doc.tex" file prepared by Theresa A. Nagy and Robert S. Hill. See also: VII/155 : "Third Reference Catalogue of bright galaxies" (RC3) by de Vaucouleurs G., de Vaucouleurs A., Corwin H.G., Buta R.J., Paturel G. and Fouque P. (1991), with 23022 galaxies File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file catalog 298 4364 The RC2 catalogue doc.tex 81 1301 Complete LaTeX documentation (needs adc.sty) adc.sty 78 68 Style file to process doc.tex
Byte-by-byte Description of file: catalog
Bytes Format Units Label Explanations
1- 8 A8 --- Name RC2 identification (NGC, IC, or anonymous) 9 A1 --- m_Name Component identification (A, B, C, etc.) (1) 10- 11 I2 h RAh Hours RA, 1950.0 12- 16 F5.2 min RAm Minutes RA, 1950.0 17 A1 --- DE- Sign Dec, 1950.0 18- 19 I2 deg DEd Degrees Dec, 1950.0 20- 23 F4.1 arcmin DEm Minutes Dec, 1950.0 24- 29 F6.2 deg GLON Galactic longitude 30- 34 F5.1 deg SGLON Supergalactic longitude 35- 41 A7 --- MType Revised morphological Type (Table 2)(9) 42- 43 A2 --- Hubble Numerical Hubble Sequence Index T (Table 3)(9) 44 A1 --- n_Hubble [*RP$] Remark on Hubble Sequence Index (8) 45- 48 A4 --- Plate Source of plate (Table 4)(9) 49 A1 --- r_MType Morphological type author code (Table 5)(9) 50- 56 A7 --- Yerkes_1 Yerkes list 1 type and color classes (6) 57 I1 --- Byurkan [1/5]? Nuclear type in Byurkan system (2) 58 A1 --- n_Byurkan [*$S2-5] Note on Byurkan nucleus type (2) 59- 62 F4.2 [0.1arcmin] logD25 ? Major isophotal diameter, log(D_25) 63- 66 F4.2 --- logR25 ? Ratio major to minor diameter, log(R_25) 67- 70 F4.2 [0.1arcmin] logD(0)25 ? Face-on major isophotal diameter 71- 74 F4.2 [0.1arcmin] logAe ? Effective aperture diameter, log(Ae) 75 A1 --- u_logAe [*$] '*'=uncertain, '$'=doubtful 77- 81 A5 --- ID Object identifications (9) 82- 88 F7.2 0.01min/yr precRAm Centennial precession in RA, minutes 89- 93 F5.1 0.01arcmin/yr precDEm Centennial precession in DE, arcminutes 94- 99 F6.2 deg GLAT Galactic latitude 100-104 F5.1 deg SGLAT Supergalactic latitude 105-112 A8 --- DDOType David Dunlap Obs. (van den Bergh) type (7) 113 I1 --- DDOClass ? David Dunlap Obs. luminosity class (7) 114 A1 --- u_DDOClass [*$] '*'=uncertain, '$'=doubtful 115-117 F3.1 --- Weight ]0/5]? Plate material weight (9) 118-124 A7 --- Yerkes_2 Yerkes list 2 type and nuclear class (6) 125-128 A4 --- RC1 RC1 nuclear class (9) 129-132 F4.3 [0.1arcmin] e_logD25 ? Mean error of logD25 133-136 F4.3 --- e_logR25 ? Mean error of logR25 137-140 F4.2 [0.1arcmin] D0 ? Corrected log(D(0)25) for galactic extinc. 141-143 F3.2 [0.1arcmin] e_logAe ? Mean error of log(Ae) 145-148 F4.1 mag Hmag ? Harvard photographic magnitude, mH 149 A1 --- u_Hmag [*] if Hmag uncertain 150-154 F5.2 mag BT ? Total asymptotic B magnitude (BT) 155 A1 --- n_BT [*S] Flag on BT, see note (3) 156-159 F4.1 mag/arcsec2 SuBr ? Mean B surface brightness within Ae (9) 160-163 F4.2 mag Extinct ? Galactic extinction in B system (A_B) (9) 164-167 F4.2 mag (B-V)T ? Asymptotic color index (9) 168 A1 --- n_(B-V)T [*] Flag on (B-V)T, see comment (3) 169-172 F4.2 mag (U-B)T ? Asymptotic color index (9) 173 A1 --- n_(U-B)T [*] Flag on (U-B)T, see comment (3) 174-177 F4.2 mag (B-V)Ae ? Effective aperture color index (9) 178 A1 --- n_(B-V)Ae [*] Flag on (B-V)Ae, see comment (3) 179-182 F4.2 mag (U-B)Ae ? Effective aperture color index (9) 183 A1 --- n_(U-B)Ae [*] Flag on (U-B)Ae, see comment (3) 184-187 F4.2 mag B-V ? Total B-V color index, corrected (9) 188-191 F4.2 [10mJy] logS_R ? Radio continuum flux near 1.4GHz (21cm) 192 A1 --- nlogSR [$+*] Conditional code for logS_R (4) 193-196 F4.2 --- SpIndex1 ? Spectral index, α- for ν < ν_R 197 A1 --- u_SpIndex1 [$*] '*'=uncertain, '$'=very uncertain 198-201 F4.2 [10-22W/m2] logS_H ? Integrated HI flux density 202 A1 --- nlogSH [$+*] Conditional code for logS_H (4) 203-207 F5.2 mag RIndex ? Corrected radio index (RI) (9) 208 A1 --- u_RIndex [$] '$' for doubtful RIndex value 209-213 I5 km/s RadVel ? Observed Radial velocity (cz) 214 A1 --- u_RadVel [*] '*' if discrepant RadVel values 215-219 I5 km/s RadVel0 ? Radial velocity corrected for solar motion 220-222 A3 --- Appendix [PST ] Appendices codes, see comment (5) 225-234 A10 --- Zwicky Zwicky identifications 235-239 F5.2 mag HmagCorr ? Corrected Harvard photog. magnitude (9) 240-242 F3.2 mag e_BT ? Estimated mean error of BT (9) 243-246 F4.1 mag/arcsec2 SuBrAv ? Average surface brightness (9) 247-251 F5.2 mag BT0 ? Corrected face-on magnitude (9) 252-254 F3.2 mag e_(B-V)T ? Mean error of asymptotic color (9) 255-257 F3.2 mag e_(U-B)T ? Mean error of asymptotic color (9) 258-260 F3.2 mag e_(B-V)Ae ? Mean error of effective color (9) 261-263 F3.2 mag e_(U-B)Ae ? Mean error of effective color (9) 264-267 F4.2 --- (U-B)T0 ? Total corrected U-B color index (9) 268-269 I2 --- o_SpIndex1 ? Number of radio continuum measurements 270-271 I2 --- ologSR ? Number of radio measurements for logS_R 272-273 I2 --- o_SpIndex2 ? Number of radio continuum measurements 274-277 F4.2 --- SpIndex2 ? Spectral index, α+ for ν > ν_R 278 A1 --- u_SpIndex2 [$*] '*'=uncertain, '$'=very uncertain 279 I1 --- ologSH ? Number of 21cm emission line observations 280-282 F3.2 0.4mag A21 ? Self-absorption at 21 cm (1.4GHz) 283-287 F5.2 mag HI ? Neutral hydrogen index (9) 288 A1 --- u_HI [$] '$' if HI is doubtful 289 I1 --- o_RadVelR ? Number of radio observations for RadVel 290-291 I2 --- o_RadVelO ? Number of optical observations for RadVel 292-294 I3 km/s e_RadVel ? Radial velocity mean error 295-298 I4 km/s DVelSun Solar motion correction, delta V
Note (1): A '.' indicates double or multiple objects where the data refers to the combined objects, but the classification is the brightest component. Note (2): See details in doc.tex; nuclear type has the values 1 = no central condensation 2 = weak central condensation 3 = strong central condensation but no star-like image 4 = star-like nuclear image at short exposure but nebulous at long exposure 5 = star-like nuclear image even at long exposures. The additional n_Byurkan flag may also contain a second Byurkan type when two independent classifications are given. Otherwise, this flag contains the symbols: S = small nucleus * = uncertain $ = doubtful Note (3): The flag on BT or asymptotic colors has the following meaning: '*' if no total magnitude could be derived with single aperture observations requiring corrections in excess of 0.5 mag. 'S' if magnitude or color is a weighted mean. Note (4): the flag on logS has the approximate meaning (see doc.tex for details): '$' indicates discrepancies '*' indicates uncertainty '+' if a close pair was in the beam Note (5): indicates objects that have entries in the special appendices of the published catalogue: 'P': source of photographs in 18 atlases and major surveys; 'S': galaxies with supernovae; 'T': Hubble-Sandage and Hubble-Holmberg types. Note (6): see details about Yerkes color and class on doc.tex, Table 6 Note (7): see details about van den Bergh type and classes in doc.tex, Table 7. Note (8): The flag concerning the numerical Hubble type is 'P'=peculiar 'R'=note '$'=doubtful '*'=uncertain Note (9): See documentation file doc.tex
Historical Notes: * See section 3 in "doc.tex" * available on the NASA "Selected Astronomical Catalogs" Vol. 1 CD-ROM, directory /nonstell/galaxies/rc2 * 13-Sep-1995 (CDS): compared to the CD-ROM version: - the decimal point was inserted when declination is given to the arcmin accuracy in file "catalog" - the document file "doc.tex" was corrected according to Harold Corwin's comments (except for units of radio fluxes) - the standardized "ReadMe" file was created
(End) Francois Ochsenbein [CDS] 13-Sep-1995
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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