------------------------------------------------------------------- THE ASTRONOMER Electronic Circular No 2536 2009 Mar 25 10.16UT 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 Backup: gmh@wdcc1.bnsc.rl.ac.uk WORLD WIDE WEB http://www.theastronomer.org ------------------------------------------------------------------- SUPERNOVA 2009E IN NGC 4141 As a follow-up to the discovery of Supernova 2009E in NGC 4141 (CBET 1648, TA E-Circular 2517) by Tom Boles on 2009 Jan 3 at magnitude 17.8 (unfiltered), Guy Hurst reports that a brightening has been detected, some 78 days after discovery. Photometry using the Bradford Robotic Telescope (0.35-m Schmidt-Cassegrain + CCD) near discovery and in a more recent image of Mar. 22 yielded: Jan 28.138UT, mag 17.5 Mar 22.067UT, mag 16.7 Magnitudes are based on A2 values for multiple comparison and check stars converted to V. In response to a report to the Central Bureau Dan Green has issued the following on CBET 1734: E. Prosperi (Castelmartini, Italy) and G. M. Hurst (Basingstoke, Hants, England) have both noted that this object (cf. CBET 1648) appears to have brightened, as indicated by their unfiltered CCD magnitudes of 2009E obtained with 0.35-m reflectors: Jan. 16.944 UT, 17.4 (Prosperi); 28.138, 17.5 (Hurst); Mar. 8.053, 16.3 (Prosperi); 9.916 16.2 (Prosperi); 22.067, 16.7 (Hurst). No spectroscopy of this object has been reported to the Central Bureau, so the supernova type remains unknown. It is hoped this will persuade a group to obtain a spectrum and classify the object but in the meantime we would welcome further images and photometry. EDITOR'S ABSENCE The editor will be away from March 27 giving the opening lecture about IYA 2009 at the Wrexham Science Festival and would welcome meeting any TA subscribers who intend to visit this event this weekend. I shall return on Monday March 30 and during this period Nick James will issue any E-Circulars and deal with any potential discovery reports. His contact details are in the first page of each issue of TA. Guy M Hurst