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SN2003cx 20020517.29 <210C PAL SN2003cx 20030212.61 <203C PAL SN2003cx 20030323.44 194C PAL SN2003cx 20030331.42 191C PAL SN2003cx 20030331.46 191C PAL SN2003cx 20030331.48 191C PAL # SN 2003cx (13:57:06.46, -17:02:22.6 (J2000.0), offset = 1"W, 3"S) is # hosted by a dim (mag about 18) galaxy, which has stellar appearence # on DSS images. SN 2003cp: In [vsnet-campaign-sn 593] (Apr. 1): >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. The CfA team reported that the spectrum taken on Apr. 1.18 resembles that of SN Ia 2-3 weeks after maximum, but there are some unusuality. The spectrum can be seen at: http://cfa-www.harvard.edu/cfa/oir/Research/supernova/spectra/sn2003cp-20030401.flm.gif , from which I have an impression that it can be somewhat younger than they reported. Sincerely Yours, Hitoshi Yamaoka, Kyushu Univ., Japan yamaoka@rc.kyushu-u.ac.jp
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