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[vsnet-obs 43248] SN information from IAUC 8061
- Date: Thu, 30 Jan 2003 15:43:38 +0900 (JST)
- To: vsnet-obs@kusastro.kyoto-u.ac.jp,vsnet-campaign-sn@kusastro.kyoto-u.ac.jp, isnchat@yahoogroups.com
- From: Hitoshi YAMAOKA <yamaoka@rc.kyushu-u.ac.jp>
- Subject: [vsnet-obs 43248] SN information from IAUC 8061
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SN2003W 20030116.4 <190:C KAI
SN2003W 20030128.4 173:C KAI
SN2003W 20030129.4 169:C KAI
SN2003W 20030129.4 170:C SCH
# A host galaxy of SN 2003W (9:46:49.48, +16:02:37.6 (J2000.0), offset
# = 3" due north) is a spiral (S(r)c) galaxy UGC 5234. There is a
# very bright (mag about 11) foreground star about 20" due east of the
# nucleus of UGC 5234. The CfA team took a spectrum on Jan. 29.34,
# which revealed that it is type Ia supernova well (about 12 days)
# before maximum. The expected maximum for typical SN Ia is mag about
# 16.3, if an extinction within the host galaxy is small.
SN 2003U:
In [vsnet-campaign-sn 546] (Jan. 28):
>SN2003U 20020910.0 <190C Bol
>SN2003U 20030127.153 180C Bol
>SN2003U 20030128.069 180C Bol
>
># A host galaxy of SN 2003U (17:22:45.66, +62:09:50.4 (J2000.0),
># offset = 13"E, 7"S) is a face-on barred-spiral (SBcd) galaxy NGC
># 6365A, which is making a probably interacting pair NGC 6365 = Arp 30
># with a northern egde-on Sdm galaxy NGC 6365B. The expected maximum
># for typical SN Ia is mag about 17.0.
The CfA team also revealed that It is a type-Ia SN a few days before
maximum light on Jan 29.53.
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