Table name: RC3 Records: 23024 Spectral Band: Uband,Bband,Vband,OPT,Colour Index Kind of Object: BrightGalaxy Mode: 2DPhotometry PreView: Coordinates: J2000
Name Meaning ra right ascension for the equinox 2000.0 processed from the 1950.0 position (see down) given to 0.1 second of time when available, and to 0.1 minute of time otherwise. dec right ascension for the equinox 2000.0 processed from the 1950.0 position (see down) given to 1 arcsec when available, and to 1 arcmin otherwise. lii Galactic longitude computed from ra and dec bii Galactic longitude computed from ra and dec The precision of lii and bii(though depending on the precision of ra and dec) is better than that in l and b l Galactic longitude in the IAU 1958 system, to deg 0.01 b Galactic latitude in the IAU 1958 system, to deg 0.01 sl Supergalactic longitude, to deg 0.01 sb Supergalactic latitude, to deg 0.01 ra_ori Right ascension for the equinox 1950.0 dec_ori Declination for the equinox 1950.0 Names = commonly used designations for the galaxies name1 Names (e.g. LMC, SMC) or NGC and IC designations name2 UGC (Nilson `73), ESO (Lauberts `82), MCG (Vorontsov-Veljaminov et al. `62-`74), UGCA (Nilson `74), CGCG (Zwicky et al. `61-`68) designations, given in that order of preference. MCG designations not listed here are given in UGC and ESO. name3 Other common designations. PGC Paturel et al. `89a,b designation. Types and Luminosity Classes type Mean revised morphological type in the RC2 system, coded as in RC2 sT_nL Sources of revised type estimates and number of luminosity class estimates T Mean numerical index of stage along the Hubble sequence in RC2 system T_u T mean error L Mean numerical luminosity class in RC2 system. L_u L mean error Optical Diameters and Axis Ratios logD25 mean decimal logarithm of the ratio of the major isophotal diameter, D25, to the minor isophotal diameter, d25, measured at or reduced to the surface brightness level (mu )_(bet) = 25.0 B-m/ss , as explained in Section 3.4.a logD25_u Mean error on logD25 logR25 Mean decimal logarithm of the ratio D25/d25 measured at or reduced to the surface brightness level (mu)_(bet) = 25.0 B-m/ss, as explained in Section 3.4.b logR25_u Mean error on logR25 logAe Decimal logarithm of the apparent diameter (in 0.1 arcmin) of the "effective aperture", the circle centered on the nucleus within which one-half of the total B-band flux if emitted logAe_u logAe mean error logD0 Decimal logarithm of the isophotal major diameter corrected to face-on (i=0 deg.), and corrected for galactic extinction to Ag = 0, but not for redshift. Major Axis Position Angle, Galactic and Internal Extinctions posan Position angle, measured in degrees from north through east (all <180 deg.), taken available from UGC,ESO and ESGC (and in few cases from HI data). Ag Galactic extinction in B-band magnitudes, calculated following Burstein and Heiles (1978a,1982,1984) Ai Internal extinction in B-band magnitudes (for correction to face-on), calculated from logR and T. A21 HI line self-absorption in magnitudes (for correction to face-on), calculated from logR and T>=1 Optical and Infrared Magnitudes btot Total (asymptotic) magnitude in the B systemderived by extrapolation from photoelectric aperture-magnitude data and from surface photometry with photoelectric zero point. btot_u btot mean error mb Photographic magnitude mb_u mb mean error mfir far-infrared magnitude calculated from mfir=-20.0-2.5*log(FIR) where FIR is the far infrared continuum flux measured at 60 and 100 microns as listed in the IRAS_PSC (Point Source Catalog) (1987) b0t Total "face-on" magnitude corrected for galactic and internal extinction, and for redshift Total Color Indices bmv_t Total color index in the Johnson B-V system bmv_tu bmv mean error umb_t Total color index in the Johnson U-B system umb_tu umb mean error bmv_0t Total (B-V) color index corrected for galactic and internal extinction, and for redshift umb_0t Total (U-B) color index corrected for galactic and internal extinction, and for redshift Effective Color Indices and B-band Surface Brightness bmv_e Mean (B-V) color index within the effective aperture Ae bmv_eu bmv_e mean error umb_e Mean (U-B) color index within the effective aperture Ae umb_eu umb_e mean error m_e Mean B-band surface brightness in magnitudes per square arcmin (B-m)/sm within the effective aperture Ae, calculated from the relation m_e = btot + 0.75 + 5*logAe - 5.26. this m_e is statistically related to the effective mean surface brightness with which it coincides when logR=0 (i = 0 deg.) m_eu Mean error of m_e m_25 Mean surface brightness in magnitudes per square arcmin within the (mu)_(bet) = 25.0 B-m/ss elliptical isophote of major axis logD25 and axis ratio logR25, defined as in RC2 by: m_25 = btot + (DEL)m25 + 5 logD25 -2.5 logR25 -5.26 where (DEL)m25 = 2.5 log (Lt/L25) = B25 - btot is the magnitude increment contributed by the outer regions of a galaxy fainter than (mu)_(bet) = 25.0 B-m/ss. m_25u Mean error on m_25 21-cm Magnitude and Linewidths, Hydrogen Index m21 21 cm emission line magnitude defined by m21 = 21.6 - 2.5 log S_H where S_H is the measured neutral hydrogen flux density in units of 10^-24 Wm^-2 m21_u m21 mean error w20 Neutral hydrogen line full width (in km/s) measured at the 20 % level (I_20/I_max) w20_u Mean error on w20 w50 Neutral hydrogen line full width (in km/s) measured at the 50 % level (I_50/I_max) w50_u Mean error on w50 HI Corrected neutral hydrogen index, which is the difference (m21 - btot)_0 between the corrected (face-on) 21cm emission line magnitude and the similarly corrected magnitude in the btot system. Radial Velocities v21 = cz is the mean heliocentric radial velocity in km/s derived from neutral hydrogen observations. v21_u Mean error on v21 vopt = cz is the mean heliocentric radial velocity in km/s derived from optical observations. vopt_u Mean error on vopt vgsr The weighted mean of the neutral hydrogen and optical velocities, corrected to the "Galactic standard of rest" v3K The weighted mean velocity corrected to the reference frame defined by the 3^oK microwave background radiation