Dear SN watchers, In the course of UK Nova/SN patrol, Tom Boles has discovered a SN in a dim galaxy within the region of Abell 426 = "Perseus cluster". The magnitude at discovery (Oct. 9.133) was mag about 17 (unfiltered CCD), and has somewhat brightened in a following week. The position of the new object, measured by Mike Armstrong, is R.A. = 3h13m07s.46, Decl. = +42o26'14".9, which is about 5" due east of the nucleus of the anonymous spiral host galaxy. Tom has also reported the position of this object, but it seems to be consistent with the position of the nucleus of the host galaxy. Because of the low galactic latitude (b = 13o), there are several foreground stars around this galaxy. One star is located on about 11" east and 1" south of the nucleus of the host galaxy. The SN locates on the midway of this foreground star and the nucleus (slightly north of this line). The host galaxy is near to UGC 2590, which is a member of the "Perseus Cluster" Abell 426. If the host galaxy is also a member of this cluster, the expected maximum of typical SN Ia is mag around 16 (included the Galactic extinction but not of the host). It is also possible that it is the far behinder. The spectral confirmation and the continuous photometry is urged. Sincerely Yours, Hitoshi Yamaoka, Kyushu Univ., Japan yamaoka@rc.kyushu-u.ac.jp