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# SN 2003bv was already reported in [vsnet-campaign-sn 582] (CBET 11). SN2003bv 20030201.0 <190C Bol SN2003bv 20030218.0 <195C Bol SN2003bv 20030311.995 177C Bol SN2003bv 20030313.918 168C Bol # SN 2003bv (7:22:11.92, +40:28:01.5 (J2000.0), offset = 4"E, 5"S) is # hosted by MCG +07-15-15, a barred-spiral galaxy with a ring # structure. The expected maximum (derived from NED recession # velocity) of typical SN Ia is well below (more than 1 mag) of the # reported magnitude on Mar. 13.918, so the timely follow-up # observations (spectroscopy, photometry) are extremely encouraged. SN2003bw 20020704.3 <190:C KAI SN2003bw 20030312.5 180:C KAI SN2003bw 20030313.5 180:C SCH # SN 2003bw (14:57:22.44, -19:12:45.9 (J2000.0), offset = 10"E, 4"N) # is hosted by IC 1077, a face-on spiral (SA(s)bc) galaxy. The new # object is superimposed on the western arm. It was also detected on # Mar. 3.5 in poor condition. The expected maximum of typical SN Ia # is mag about 15.2, though it seems not a case. # Faint SNe 2003bx-ca were discovered by Deep Lens Survey with 4-m # class telescopes. # Deep Lens Survey also discovered an optical transient without # apparent host galaxy at 9:22:38.29, +29:17:19.1 (J2000.0), which was # mag 22.9 on Mar. 10.3. Sincerely Yours, Hitoshi Yamaoka, Kyushu Univ., Japan yamaoka@rc.kyushu-u.ac.jp
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