> Date: Sat, 6 Jan 2001 17:05:32 -0500 (EST) > From: IAUC mailing list > To: uai@obs-azur.fr > Subject: IAUC 7557: 2001D; 2001E; 2000fo; Poss. N IN Pup > Circular No. 7557 > 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) > CBAT@CFA.HARVARD.EDU (science) > URL http://cfa-www.harvard.edu/iau/cbat.html ISSN 0081-0304 > Phone 617-495-7440/7244/7444 (for emergency use only) > > > SUPERNOVA 2001D IN IC 728 > M. Modjaz and W. D. Li, University of California at Berkeley, > on behalf of LOTOSS (cf. IAUC 7514), report the discovery with the > 0.8-m Katzman Automatic Imaging Telescope (KAIT) of an apparent > supernova on unfiltered images taken on Jan. 5.5 (mag about 17.6) > and 6.4 UT (mag about 17.5). The new object is located at R.A. = > 11h44m50s.97, Decl. = -1 36'18".4 (equinox 2000.0), which is 8".0 > east and 12".4 south of the nucleus of IC 728. A KAIT image of the > same field taken on 2000 Dec. 28.5 showed nothing at the position > of SN 2001D (limiting mag about 18.5). > > > SUPERNOVA 2001E IN NGC 3905 > Modjaz and Li also report the discovery with KAIT of another > apparent supernova on unfiltered images on Jan. 5.5 (mag about > 17.6) and 6.4 UT (mag about 17.2). SN 2001E is located at R.A. = > 11h49m05s.00, Decl. = -9 44'10".9 (equinox 2000.0), which is 0".6 > east and 23".2 south of the nucleus of NGC 3905. A KAIT image of > the same field taken on 2000 Dec. 30.5 showed nothing at the > position of the new object (limiting mag about 19.0). > > > SUPERNOVA 2000fo IN PGC 70148 > T. Matheson, S. Jha, P. Challis, and R. Kirshner, Harvard- > Smithsonian Center for Astrophysics, report that a spectrum of SN > 2000fo, obtained by M. Calkins on 2000 Dec. 23.08 UT with the F. L. > Whipple Observatory 1.5-m telescope (+ FAST spectrograph), shows it > to be a type-Ia supernova at maximum light. The spectrum exhibits > a possibly reddened continuum, with well-defined Si II, S II, Fe > II, Mg II, and Ca II features. Adopting the NASA/IPAC > Extragalactic Database recession velocity of 7152 km/s for the host > galaxy, the expansion velocity is 11 800 km/s for Si II (rest 635.5 > nm). The spectral-feature age of the supernova (Riess et al. 1997, > A.J. 114, 722) is 3 +/- 2 days before maximum light. > > > POSSIBLE NOVA IN PUPPIS > CCD photometry of the new variable star noted on IAUC 7552 and > 7556 (comparison stars from Tycho catalogue): 2000 Dec. 31.001 UT, > V = 9.24 +/- 0.05, B-V = +0.44 +/- 0.07 (D. Hanzl, Brno, Czech > Republic); 31.96, V = 9.14 +/- 0.06, B-V = +0.48 +/- 0.06 (Hanzl); > 2001 Jan. 1.020, V = 9.13 (M. Lehky, Hradec Kralove, Czech Republic). > > (C) Copyright 2001 CBAT > 2001 January 6 (7557) Daniel W. E. Green >
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