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[vsnet-obs 42182] SN observations from IAUC 8008
- Date: Tue, 5 Nov 2002 14:09:02 +0900 (JST)
- To: vsnet-obs@kusastro.kyoto-u.ac.jp
- From: Hitoshi YAMAOKA <yamaoka@rc.kyushu-u.ac.jp>
- Subject: [vsnet-obs 42182] SN observations from IAUC 8008
- Cc: vsnet-campaign-sn@kusastro.kyoto-u.ac.jp
- Delivered-To: vsnet-obs@kusastro.kyoto-u.ac.jp
- Sender: owner-vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
SN2002hl 20020404.0 <185C Bol
SN2002hl 20021104.236 163C Bol
SN2002hl 20021105.083 165C Bol
# NGC 3665, a host galaxy of SN 2002hl (11:24:40.12, +38:46:03.0
# (J2000.0), offset = 42"W, 17"N), is a nearly lenticular (SA(s)0^0^)
# galaxy, which likely produce only SN Ia, whose expected maximum is
# mag about 13.9. If this is the case, it should be one (or mixed) of
# the followings: a) reddened by dust in the host galaxy, b) very
# subluminous, or c) several month old. The possibility that it is
# rising is unlikely because it remains almost constant for 1 day.
# The last negative observation by T. Boles was on June 1 (limiting
# magnitude was not reported).
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