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SN2003co 20020331.32 <209:C PAL SN2003co 20030221.46 <209:C PAL SN2003co 20030322.14 186:C PAL SN2003co 20030330.14 181:C PAL # SN2003co (10:49:39.91, +29:21:44.6 (J2000.0), offset = 7"W, 8"S) is # hosted by 2MASXi J1049404+292152, a distant (v_r = 25000 km/s) # spiral (Sb) galaxy. SN2003cp 20030314.0 <185:C ARM SN2003cp 20030330.86 162:C ARM SN2003cp 20030331.786 162:C ARM # SN 2003cp (8:09:11.13, +57:41:14.0 (J2000.0), offset = 3"W, 9"N) is # hosted by MCG +10-12-78, a spiral (Sb) galaxy. The expected maximum # for typical SN Ia is consistent with the discovery magnitude. A # bright (mag about 15) foreground star exists at about 17" ENE of the # nucleus of the host galaxy. SN2003cq 20030314.0 <174:C ARB SN2003cq 20030330.84 170:C ARB SN2003cq 20030331.816 179:C Bol SN2003cq 20030331.830 170:C ARB # SN 2003cq (11:56:14.17, +60:31:19.1 (J2000.0), offset = 32"E, 2"S) # is hosted by NGC 3978, a face-on spiral (SABbc:) galaxy making a # pair with 2' west NGC 3975. The expected maximum for typical SN Ia # is consistent with the discovery magnitude. SN2003cr 20030224.0 <190:C Bol SN2003cr 20030331.18 177:C Bol SN2003cr 20030331.894 175:C Bol # SN 2003cr (14:58:35.53, +44:53:06.4 (J2000.0), offset = 5"W, 5"N) is # hosted by UGC 9639, a spiral (Sab) galaxy. The expected maximum for # typical SN Ia is consistent with the discovery magnitude. There is # a foreground star (mag about 17) at NE of the nucleus of the host # galaxy. SN2003cs 20020418.14 <208:C PAL SN2003cs 20030203.49 179:C PAL SN2003cs 20030209.44 171:C PAL SN2003cs 20030327.19 194:C PAL SN2003cs 20030331.22 196:C PAL # SN 2003cs (11:20:37.52, -4:54:32.7 (J2000.0), offset = 6" due north) # is hosted by 2MASXi J1120375-045437, a dim galaxy. The discovery # (early February) magnitude is consistent with the expected maximum # for typical SN Ia. SN2003ct 20030209.44 <206:C PAL SN2003ct 20030325.20 191:C PAL SN2003ct 20030327.19 190:C PAL SN2003ct 20030331.22 191:C PAL # SN 2003ct (11:22:56.20, -2:56:59.9 (J2000.0), offset = 13"E, 3"S) is # hosted by CGCG 011-083, a distant spiral (SA(s)bc:) galaxy. The # expected maximum for typical SN Ia is mag about 18.2. SN 2003bw: In [vsnet-campaign-sn 583] (Mar. 16) >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. The Las Campanas spectrum taken on Mar 31.39 revealed that it is of type II, at least two months after explosion. Sincerely Yours, Hitoshi Yamaoka, Kyushu Univ., Japan yamaoka@rc.kyushu-u.ac.jp
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