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THE ASTRONOMER Electronic Circular No 2383      2007 Oct 06 10.10UT
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
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THE ASTRONOMER ANNUAL MEETING, 2007 OCTOBER 20
We are delighted to announce the addition of a further speaker for our 
annual meeting to be held on Saturday October 20 here in Basingstoke. 
Daniel Fischer, from Germany, will be talking on 'Unusual Effects in 
Annular Eclipses'.

On reviewing the press announcements this morning about the industrial 
action affecting Royal Mail, we understand no further post can be 
accepted until next Thursday and that subsequent planned action might 
mean delivery thereafter could be substantially delayed. This seems to 
suggest our usual method of sending programmes by post about 10 days 
before the event is not practical this year. We are exploring the 
alternative of e-mailing programmes within the next few days and will 
keep you informed.

SUPERNOVA 2007it IN NGC 5530
C. Contreras et. al., on behalf of the Carnegie Supernova Project, 
report on CBET 1068 that the probable bright supernova in NGC 5530 (see 
TA E-Circular 2376) has been confirmed as a supernova.
2007it is found at:
RA 14h 18m 25.627s DEC 43 22' 53.80" (2000), with B magnitude 13.1 +/- 
0.3, relative to 40 field stars in the USNO-B1 catalogue from Sept 
14.03. A spectrum of Sept 14.98UT indicates it to be a young type-II 
supernova.

SUPERNOVA 2007iu IN ANONYMOUS GALAXY
Discovery by ROTSE collaboration of a possible supernova (CBET 1069):
SN      2006 UT      R.A.  (2000.0)  Decl.    Mag.     Offset
2007iu  Sep  8.24   01 25 20.11  +08 54 12.7  19.0     -       -
It is blended with a nearby USNO-catalogue star of mag 16.2 in the ROTSE 
images. A spectrum of Sept.15.28 UT with the 9.2-m Hobby-Eberly 
Telescope shows it to be a type-II supernova.

VARIABLE STAR IN PERSEUS
Herman Mikuz, Crni Vrh Observatory, has reported to us that a new 
starlike variable (mag 17.9R) was detected on four unfiltered CCD images 
(limiting mag 19.0) taken around Sept. 16.078UT in the course of the 
PIKA project at the Crni Vrh Observatory using
the 0.60-m f/3.3 Cichocki telescope. A report has subsequently appeared 
in IAUC 8870.
The variable object is located at:
RA 03h 57m 28.01s DEC +35 37'16.3" (2000).  This position is consistent 
with USNO-B1-catalogue star 1256-0061977 with B
magnitude 21.5. Additional PIKA magnitudes for the new object show that 
it is brightening:  2003 Sept. 26, [19.0; 2004 Feb. 9, [19.0; 2005 Jan. 
11, [19.0; 2007 Sept. 16.955, B = 17.90, R = 17.65; Sept. 17.037, B = 
17.60, R = 17.39. Nothing is visible at this location on several Palomar 
Sky Survey and 2MASS images from the Aladin database.

Guy M Hurst