------------------------------------------------------------------- THE ASTRONOMER Electronic Circular No 1891 2003 Jun 19 18.48UT Ed:Guy M Hurst, 16,Westminster Close, Kempshott Rise, Basingstoke, Hants, RG22 4PP,England.Telephone/FAX(01256)471074Int:+441256471074 INTERNET: GUY@TAHQ.DEMON.CO.UK GMH at AST.STAR.RL.AC.UK WORLD WIDE WEB http://www.theastronomer.org ------------------------------------------------------------------- SUPERNOVA 2003gd IN M74 Rev Bob Evans has e-mailed TA to advise that he has found a possible supernova in Messier 74 in Pisces (= NGC 628). The object, of magnitude 13.2, was first detected visually on 2003 June 12.82UT and offsets were estimated to be 20"E and 150"S of the nucleus. Robert McNaught confirmed the presence of this object on images of June 13.84UT using the 1.0-m Siding Spring Observatory telescope. >From these he has measured a precise position of: RA 01h 36m 42.65s DEC +15 44' 20.9" (2000) and revises the offsets to: 13.2"E and 161"S of the centre of the host galaxy. He adds the object is not present on digitised sky survey images. Additionally Bob Evans has e-mailed that Tom Dobosz also confirmed the object on June 14 using an LX200 and three ten minute exposures co-added. This image has been submitted to us for possible publication in the July issue. According to IAUC 8150, P. Garnavich, University of Notre Dame; and E. Bass, Cornell University, obtained near-infrared spectra (range 850-2400 nm) in twilight on June 13.46 UT with the 1.8-m Vatican Advanced Technology Telescope. They indicate it is a type-II supernova. A further report, detailed on IAUC 8152, by R. Kotak and Peter Meikle, Imperial College, London, and S. J. Smartt, Institute of Astronomy, Cambridge report that a spectrum was obtained at the William Herschel Telescope by Chris Benn on June 14.2 UT. The analysis also confirms it to be of type II approximately two months after maximum. S. Smartt also reports that a progenitor for this supernova may have been detected at V=26.1 but it is planned to obtain HST override time to refine this further to establish if the identification is correct. This is the second supernova detected in this galaxy in consecutive years. The first was Supernova 2002ap found by Yoji Hirose on 2002 January 29 (see The Astronomer E-Circular 1738). Guy M Hurst