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[vsnet-obs 39855] SN observation from IAUC 7901
- Date: Fri, 17 May 2002 10:21:42 +0900 (JST)
- To: vsnet-obs@kusastro.kyoto-u.ac.jp
- From: Hitoshi YAMAOKA <yamaoka@rc.kyushu-u.ac.jp>
- Subject: [vsnet-obs 39855] SN observation from IAUC 7901
- Delivered-To: vsnet-obs@kusastro.kyoto-u.ac.jp
- Sender: owner-vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
SN2002cv 20020328.0 <170I TNT
SN2002cv 20020429.0 <180J AZT
SN2002cv 20020505.0 <180J AZT
SN2002cv 20020506.0 <180J AZT
SN2002cv 20020509.0 180:J AZT
SN2002cv 20020513.8 157J AZT
SN2002cv 20020514.0 177I TNT
SN2002cv 20020514.0 <200V TNT
SN2002cv 20020515.2 190:R MMT
SN2002cv 20020515.2 166:I MMT
Observer:
AZT: 1.1-m AZT-24 telescope at Campo Imperatore (from IAUC)
TNT: 0.72-m Teramo TNT telescope (from IAUC)
MMT: MMT 6.5-m (from IAUC)
# SN 2002cv occurred in the same galaxy as a bright SN 2002bo = NGC
# 3190. The position of new SN is: R.A. = 10h18m03s.68, +21o50'06".2
# (2000.0), which is about 18" west and 10" north of the nucleus of
# the host galaxy. SN 2002cv is highly reddened, and the spectrum
# shows that it seems to be a core-collapse SN soon after burst.
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