Following suspected variable was found durning my scan of Amateur FITS Archive: AFASV_M31_256 AFASV_M31_256 amplitude=0.31 mag R. A. (2000) Decl. image 12.86 0 41 54.219 + 41 14 13.10 so1 12.55 0 41 54.409 + 41 14 14.15 ugm images: so1: Mauro Facchini, Obsservatorio di Cavezzo, 0.20- m reflector f2.8, CCD Starlight HX516 date: 26/06/00 time: 00:15:26 UT ugm: Mauro Facchini, Obsservatorio di Cavezzo, 0.13- m reflector f4, CCD Starlight HX516 date: 06/09/00 time: 00:40:00 UT IDS FROM VIZIER: GSC: dif: 0.0244 RA: 00 41 54.10 Decl: +41 14 13.5 GSCid: 0280102031 mag: 12.98+/-0.43 Brightest stars in the field of M31 (Berkhuijsen+ 1988): dif: 0.0255 RA: 00 41 54.15 Decl: +41 14 11.8 seq: 3747 Vmag: 13.81+/-0.20 BVRI CCD photometry in the field of M 31 (Magnier+ 1992) dif: 0.0273 RA: 00 41 54.08 Decl: +41 14 13.4 seq: 240123 Bmag: 13.968+/-0.016 Vmag: 12.900+/-0.034 2MASS: dif: 0.0102 RA: 00 41 54.17 Decl: +41 14 13.4 Jmag: 10.911+/-0.035 Hmag: 10.354+/-0.033 Kmag: 10.205+/-0.032 M 31 reference catalog (Shokin+ 1998): dif: 0.0166 RA: 00 41 54.13 Decl: +41 14 13.1 Bmag: 14.00 Maybe an Einstain X source (Harris+ 1994): dif: 0.405 RA: 00 41 52.2 Decl: +41 14 04 Catnum: 130 seq: 574 also possible ROSAT source: RX J0041.8+4114 dif: 0.740 RA: 00 41 51.9 Decl: +41 14 49