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SN 2003gx: In [vsnet-campaign-sn 669] (Aug. 10!): >SN2003gx 20030219.0 <190C Bol >SN2003gx 20030803.038 186C Bol >SN2003gx 20030804.044 185C Bol > ># SN 2003gx (1:02:55.09, +37:40:10.3 (J2000.0), offset = 2"W, 13"S) is ># hosted by MCG +6-3-7, a faint spiral galaxy. The expected maximum ># for typical SN Ia is mag about 17.5. The CfA group obtained a spectrum of this SN on Sept. 18.42 UT, which revealed that it is type II SN. SN 2003hy: In [vsnet-campaign-sn 691] (Sept. 15): >SN2003hy 20030803.0 <195C ARM >SN2003hy 20030816.0 <195C Bol >SN2003hy 20030901.0 <195C Bol >SN2003hy 20030904.0 <185C ARM >SN2003hy 20030913.865 163C ARM >SN2003hy 20030914.007 166C Bol >SN2003hy 20030914.815 163C ARM >SN2003hy 20030914.837 166C Bol > ># SN 2003hy (21:54:22.72, +15:09:38.7 (J2000.0), offset = 6"W, 13"N) ># is hosted by IC 5145, a spiral (Sab) galaxy. IC 5145 also produced ># SN Ic 2002dn, which was caught at mag about 18.6 about a week after ># maximum. The expected maximum for typical SN Ia is consistent with ># the discovery magnitude of SN 2003hy. The CfA team also took a spectrum of SN 2003hy on Sept. 18.28 UT, which revealed that it is a type IIn SN without broad components. SN 2003ia: In [vsnet-campaign-sn 693] (Sept. 18) >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. The CfA team obtained a spectrum of SN 2003ia on Sept. 19.18 UT, which revealed that it is a type Ia SN about 2 weeks after maximum. SN 2003ib: In [vsnet-campaign-sn 693] (Sept. 18) >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. The Carnegie Observatories group took a spectrum of SN 2003ib on Sept. 18.17 UT, which revealed that it is a young type II SN. The host galaxy seems to be indeed a member of Abell 3698. SN 2003ic: In [vsnet-campaign-sn 693] (Sept. 18) >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. The Carnegie Observatories team also revealed that it is type Ia supernova about 5 days before maximum on Sept. 18.25 UT. SN 2003id: In [vsnet-campaign-sn 693] (Sept. 18) >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. The Carnegie Observatories team also revealed that it is type Ic supernova about 4 days before maximum on Sept. 18.33 UT.
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