SN2003F 20021211.0 <190:C KAI SN2003F 20030108.16 167C Puc SN2003F 20030108.3 163:C KAI SN2003F 20030109.6 161C BAO # A host galaxy of SN 2003F (5:11:33.03, +17:03:28.4 (J2000.0), offset # = 7"E, 6"N) is a disturbed spiral (Sdm:) galaxy UGC 3261. It is # near to the Galactic plain (b = -13o), so there are several # foreground stars superimposed on the host galaxy. A spectrum taken # with the Las Campanas Observatory Baade 6.5-m telescope on Jan 9.11 # revealed that it is type Ia SN a few days before maximum. Some # reddening within the host galaxy is suggested, as well as Galactic # one. The reported magnitude is thus considerably brighter than # expected maximum for typical SNe Ia (mag about 16.7) taking account # of the redshift and the Galactic extinction. Further magnitude # estimates are urged. SN2003G 20021212.0 <190:C KAI SN2003G 20030108.2 162:C KAI SN2003G 20030109.5 158C BAO # A host galaxy of SN 2003G (2:08:28.13, +6:23:51.9 (J2000.0), offset # = 6"E, 10"N) is a face-on spiral (SAbc) galaxy IC 208. A spectrum # taken with Baade telescope on Jan 9.05 revealed that it is a young # SN IIn. The reported magnitudes are consistent with that of ordinal # core-collapsed SNe. SN2003H 20030103.0 <190:C KAI SN2003H 20030108.3 178:C KAI SN2003H 20030109.6 180C BAO # A host galaxy of SN 2003H (6:16:25.68, -21:22:23.8 (J2000.0)) is an # interacting pair NGC 2207 (SAB(rc)bc pec) + IC 2163 (SB(rs)c pec). # An offset from IC 2163 = eastern component of the pair is reported # as 32"W, 10"N. An offset from NGC 2207 is derived as 51"E, 2"S. # The classification was not been reported on IAUC 8045. NGC 2207 had # produced SN Ia 1975A (B=14.7 at maximum) and SN Ib(?) 1999ec # (discovery mag about 17.9, past maximum). SN 2003E: In [vsnet-campaign-sn 531] (Jan. 9): >SN2003E 20021127.3 <185:C KAI >SN2003E 20030105.3 170:C KAI >SN2003E 20030107.3 170:C KAI > ># A host galaxy of SN 2003E (4:39:10.88, -24:10:36.5 (J2000.0), offset ># = 6"W, 9"N) is an edge-on spiral (Sbc) galaxy MCG -4-12-4, which ># makes a pair with MCG -4-12-3. The SN is superimposed on the disk, ># so notable extinction is possible. The expected maximum for typical ># unreddened (in the host galaxy) SN Ia is mag about 15.7. A spectrum taken with Baade telescope on Jan 9.15 shows that it is a young SN II. Sincerely Yours, Hitoshi Yamaoka, Kyushu Univ., Japan yamaoka@rc.kyushu-u.ac.jp