Circular No. 8288
Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION Mailstop 18, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A. IAUSUBS@CFA.HARVARD.EDU or FAX 617-495-7231 (subscriptions) BMARSDEN@CFA.HARVARD.EDU or DGREEN@CFA.HARVARD.EDU (science) URL http://cfa-www.harvard.edu/iau/cbat.html Phone 617-495-7244/7440/7444 (for emergency use only)
SUPERNOVA 2004Y
Further to IAUC 8287, W. Li reports the LOSS discovery, on a
KAIT image taken on Feb. 12.5 UT, of a supernova (mag 18.5) located
at R.A. = 11h43m28s.26, Decl. = +21o40'30".3 (equinox 2000.0),
which is 0".5 east and 3".3 north of the center of the apparent
host galaxy. A. V. Filippenko, R. Chornock, and R. J. Foley report
that inspection of CCD spectra (range 400-1000 nm), obtained on
Feb. 14 UT with the Keck II 10-m telescope (+ ESI), shows that SN
2004Y is of type Ia, roughly 3-4 weeks past maximum brightness.
The redshift of the host galaxy, measured from narrow emission
lines from H II regions close to the supernova, is 0.0692.
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Host galaxy info: vel = 20760 km/s.
SN type info: Ia
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