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SN2003ia 20030602.0 <185C KIt SN2003ia 20030605.0 <180C KIt SN2003ia 20030915.422 172C KIt SN2003ia 20030916.411 173C KIt # SN 2003ia (16:17:41.17, +35:00:07.2 (J2000.0), offset = 8"E, 8"S) is # hosted by NGC 6109, a lenticular (E/S0) galaxy. The morphology of # the host galaxy suggest that it would be a type Ia SN, whose # expected maximum is consistent with the discovery magnitude. SN2003ib 20030815.3 <185:C KAI SN2003ib 20030901.2 190:C KAI SN2003ib 20030911.2 179:C KAI SN2003ib 20030916.2 176:C KAI SN2003ib 20030917.2 175:C KAI # SN 2003ib (20:33:30.98, -24:37:15.0 (J2000.0), offset = 1"E, 10"N) # is hosted by MCG -04-48-15, a spiral ((R)S(r?)b) galaxy. There are # several foreground stars around the host galaxy. It is probably a # member of a cluster Abell 3698. If it is the case, the expected # maximum for typical SN Ia is mag about 16.3. SN2003ic 20030902.4 <190:C KAI SN2003ic 20030916.4 176:C KAI SN2003ic 20030917.4 176:C KAI # SN 2003ic (0:41:50.23, -9:18:19.0 (J2000.0), offset = 2"W, 8"S) is # hosted by MCG -02-2-86, a giant elliptical (cD;SB(r)0^0^ pec?) # galaxy in a cluster Abell 85. It is likely a SN Ia near maximum. # There are many objects around the galaxy. SN2003id 20030907.5 <185:C KAI SN2003id 20030916.5 167:C KAI SN2003id 20030917.5 167:C KAI # SN 2003id (2:21:35.70, -5:31:51.0 (J2000.0), offset = 11"W, 35"S) is # hosted by NGC 895, a nearby spiral (SA(s)cd) galaxy. The expected # maximum for typical SN Ia is mag about 14.2, so it seems to be a # gravitational-collapsed event and/or absorbed SN. SN 2003hx: In [vsnet-campaign-sn 691] (Sep. 15) > The ANU group revealed that it is truely a type Ia SN, near maximum >on Sept. 13.78 UT. An ESO spectrum taken on Sept. 15.4 UT suggest that it is affected by significant dust extinction. Sincerely Yours, Hitoshi Yamaoka, Kyushu Univ., Japan yamaoka@rc.kyushu-u.ac.jp
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