J/ApJS/92/219 J/ApJS/92/219 Catalog of recent supernovae S Van den Bergh Astrophys. J. Suppl. Ser. 92 219 1994 1994ApJS...92..219V II/133 : Photoelectric UBV observations of supernovae II/159 : Asiago Supernova Catalogue 1988 II/189 : A catalogue of magnitude observations of type I supernovae II/201 : Sternberg SN Catalogue, 1994Sep. II/205 : GCVS, Vol. V.: Extragalactic Variable Stars Gomez G. & Lopez 1993, AJ 106, 245 (=1993AJ....106..245G) Lauberts, A., 1982 The ESO/Uppsala Survey of the ESO (B) Atlas (Garching: European Southern Observatory) (Catalogue<VII/34B>) Vorontsov-Velyaminov, B.A., et al. Morphological Catalogue of Galaxies I-IV MCG (Moscow: Moscow University) 1962-1974 (Catalogue<VII/62A>) Pennypacker et al. 1992, IAUC 5652 (=1992IAUC.5652....1P) Sandage, A., & Tammann, G.A. 1981 A Revised Shapley-Ames Catalog at Bright Galaxies (Washington: Carnegie Institution) (Catalogue<VII/51>) Schmidt B.P., et al. 1993 AJ 105, 2236 (=1993AJ....105.2236S) de Vaucouleurs, G., de Vaucouleurs, A., Corwin, H.G., Buta, R.J., Paturel, G., & Fouque, P. 1991 Third Reference Catalogue of Bright Galaxies (RC3) (Berlin: Springer) (Catalogue<VII/155>) Supernovae supernovae: general A listing is given of all supernovae discovered between 1989 January 1 and 1993 April 1. The data show no evidence for a significant dependence of the discovery probability of supernovae on parent galaxy inclination to the line of sight. If no inclination corrections need to be applied, then the supernova rates in spirals are only about half as large as previously believed. The mean linear separation of supernovae of type II (SNe II) from the center of their parent galaxy increases with increasing distance (Shaw effect). The Shaw effect appears less evident, or absent, for (more luminous) supernovae of type Ia. The data are consistent with, but do not prove, the hypothesis that (presumably reddened) SNe II are more likely to be discovered in the red than in the blue. Due to intensive surveillance, most bright SNe Ia tend to be found before maximum, whereas the majority of faint SNe Ia are discovered after maximum light.

SN Supernova name --- n_SN A 'N' indicates that it is not a supernova --- Gal Parent galaxy name number=1 N = NGC, I = IC, U = UGC. The letters E and M indicate that the galaxy is listed in the ESO (Lauberts 1982) or MCG (Vorontsov-Velyaminov et al. 1962-1974) Catalogs, respectively --- MType Parent galaxy classification types number=2 Galaxy classification types were, in order of preference, drawn from (a) Sandage and Tammann (1981) (Catalogue <VII/51>) (b) an unpublished catalog of DDO classifications by the present author (c) de Vaucouleurs et al. (1991) (RC3, Catalogue <VII/155>) (d) Lauberts (1982) (Catalogue <VII/34B>) --- RAh Right ascension 1950 h RAm Right ascension 1950 min RAs Right ascension 1950 s DE- Declination sign --- DEd Declination 1950 deg DEm Declination 1950 arcmin DEs Declination 1950 arcsec RV Radial velocity number=3 Galaxy radial velocity, preferentially drawn from the optical heliocentric listing of de Vaucouleurs et al. (1991) km/s Mag Discovered magnitude mag n_Mag Color of discovered magnitude number=4 Both mpg, blue and B are called B, MJ is designated J, mpv and V are both indicated by V, r and R are both called as R. For a few supernovae I or K discovery magnitudes are listed --- IAUC Number of IAU Circular giving discovery information --- Offsets Offsets from nucleus of galaxy --- Type Supernova type --- IAUC(SN) Number of IAU Circular from which SN type was drawn --- Notes Remarks on some individual supernovae number=5 individual notes: 1 Offset from nucleus given as 25" NE in IAU Circular 4758. 2 Offsets provided by Tsvetkov et al. 3 Offset from nucleus given as 5.8" SW in IAUC 5046. 4 According to IAUC 4959 this is a compact HII region, not a supernova 5 Type II-P supernova according to Schmidt et al. (1993). 6 IAUC 5111 gives type Ib, whereas IAUC 5129 assigns a type Ic. 7 Located between two galaxies. Quoted position is that of the supernova. 8 Not a supernova according to IAUC 5270. 9 Quasar according to IAUC 5328. 10 The "anonymous" galaxy in IAUC 5356 is, in fact, MCG 4-6-29. 11 It is not clear whether the position quoted in IAUC 5446 refers to the galaxy or to the supernovae. 12 According to IAUC 5468 possibly a subluminous SNIa like SN1991bg. 13 Foreground M star according to IAUC 5528. 14 Occurred 4"N of SN 1992R (Gomez & Lopez 1993). 15 Supernova located 45" from nucleus. 16 On the basis of photometry Pennypacker et al. (IAUC 5652) claim that this supernova was probably of type Ia. --- SN Supernova name --- Gal Parent galaxy name --- Type Type of the supernova --- Age Information on the spectral age --- l_T Limit flag on T --- T Evolutionary age at the time of the discovery d u_T Uncertainty flag on T --- e_T rms uncertainty on T d Patricia Bauer CDS 1996May14Sidney van den Bergh <vdb@dao.nrc.ca> J_ApJS_92_219.xml