SN2002kg 19981113.0 <195:C KAI SN2002kg 20021026.0 190:C KAI SN2002kg 20021030.0 190:C SCH SN2002kg 20021101.0 190:C KAI SN2002kg 20021114.0 190:C SCH SN2002kg 20021122.0 190:C SCH SN2002kg 20021124.0 190:C SCH SN2002kg 20021125.0 190:C SCH SN2002kg 20021202.0 190:C KAI SN2002kg 20021208.0 190:C SCH SN2002kg 20030101.0 190:C SCH # A host galaxy of SN 2002kg (7:37:01.83, +65:34:29.3 (J2000.0), # offset = 62"E, 96"S) is a nearby (about 3.5 Mpc) spiral (SAB(s)cd # HII) galaxy NGC 2403. This object is quite dim, so the # identification would be very difficult. The UCB team spectrum # reveals that it is type IIn supernova, resembling SNe 1997bs or # 2000ch, which have been suggested to be a superoutburst of the # luminous blue variables, like eta Car. The absolute magnitude of SN # 2002kg is now about -8, which is even lower than that of SN 2000ch # or resembling SN IIn (around -12 at its short-lived maximum). SN # 2000ch was caught in the "premaximum halt" during a few years until # its maximum (see IAUC 7415, 7417, 7419, and 7421), so possibly SN # 2002kg will become brighter. Interestingly, SN 1954J in the same # galaxy NGC 2403 (maximum B=16.5) was also very dim SN, and Smith et # al. 2001, PASP, 113, 692 suggest that SN 1954J is of this class. SN 2002hz: In [vsnet-campaign-sn 507] (02 Nov 18!): >SN2002hz 20021102.2 <190:C KAI >SN2002hz 20021112.2 184:C KAI >SN2002hz 20021116.2 178:C KAI > ># UGC 12044, a host galaxy of SN 2002hz (22:27:49.54, +38:35:09.5 ># (J2000.0), offset = 14"E, 3"S), is an edge-on spiral (Sab) galaxy ># with low galactic latitude (b=-16o). The expected maximum for ># typical SN Ia (without a reddening in the host galaxy) is mag about ># 16.3, but judged from the reports (0.6 mag rise in 4 days), it is ># possibly a reddened (or subluminous) SN Ia or a core-collapse event. A spectrum taken by the UCB team on Jan. 7 suggest that it is type Ib SN roughly 2 months after maximum light. Sincerely Yours, Hitoshi Yamaoka, Kyushu Univ., Japan yamaoka@rc.kyushu-u.ac.jp