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[vsnet-campaign-sn 592] SNe information from IAUC 8101



SN2003cj  20020414.21 <212:C  PAL
SN2003cj  20030212.51 <202:C  PAL
SN2003cj  20030316.36 <193:C  PAL
SN2003cj  20030321.64 <187:C  PAL
SN2003cj  20030322.47 <200:C  PAL
SN2003cj  20030326.28  202:C  PAL
SN2003cj  20030327.20  200:C  PAL

# SN 2003cj (12:15:51.90, +8:59:15.7 (J2000.0), offset = 1"W, 3"S) is
# hosted by a very dim (mag about 20) galaxy.

SN2003ck  20020413.2  <209:C  PAL
SN2003ck  20030203.61 <205:C  PAL
SN2003ck  20030217.45 <192:C  PAL
SN2003ck  20030326.39  193:C  PAL
SN2003ck  20030328.26  195:C  PAL

# SN 2003ck (13:06:21.72, +3:04:21.0 (J2000.0), offset = 3"W, 1"N) is
# hosted by MAPS-NGP O_557_1733751, also a dim (mag 18.5) galaxy. 

SN2003cl  20020721.17 <216:C  PAL
SN2003cl  20030216.39 <186:C  PAL
SN2003cl  20030306.54  200:C  PAL
SN2003cl  20030327.24  195:C  PAL

# SN 2003cl (12:38:50.11, -2:49:58.8 (J2000.0), offset = 2"E, 2"N) is
# hosted by 2dFGRS N186Z103, a distant (v_r = 50000 km/s) galaxy.  

SN2003cm  20020727.3  <200:C  KAI
SN2003cm  20030327.5   194:C  KAI
SN2003cm  20030328.5   194:C  KAI
SN2003cm  20030329.5   194:C  KAI

# SN 2003cm (16:50:55.02, +59:43:18.1 (J2000.0), offset = 9"W, 11"N)
# is hosted by UGC 10590, a face-on barred-spiral (SBcd?) galaxy.  The
# expected maximum for typical SN Ia is mag about 14.8, so it is very
# subluminous or reddened or old event.

SN2003cn  20030307.4  <195:C  KAI
SN2003cn  20030329.4   181:C  KAI
SN2003cn  20030330.4   181:C  KAI

# SN 2003cn (13:07:37.05, -0:56:49.9 (J2000.0), offset = 24"W, 16"S)
# is hosted by IC 849, a face-on spiral (SAB(rs)cd) galaxy.  The Las
# Campanas spectrum taken on Mar. 31.31 UT revealed that it is type II
# SN about 2-3 weeks after explosion (IAUC 8102).  The discovery
# magnitude is typical for the graviatational-collapse event.

SN2003cg  20030319.511 <160:C  YHr


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