Following suspected variable was found durning my scan of Amateur FITS Archive: AFASV_M31_263 AFASV_M31_263 amplitude=0.30 mag R. A. (2000) Decl. image 14.90 0 42 01.833 + 40 50 58.98 so1 15.20 0 42 01.967 + 40 50 55.36 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: USNO A2.0: dif: 0.0559 RA: 00 42 02.028 Decl: +40 50 56.41 USNOid: 1275-00422209 Bmag: 16.7 Rmag: 15.9 epoch: 1953.773 Brightest stars in the field of M31 (Berkhuijsen+ 1988): dif: 0.0905 RA: 00 42 02.10 Decl: +40 50 54.4 seq: 3843 Vmag: 15.05+/-0.17 BVRI CCD photometry in the field of M 31 (Magnier+ 1992): dif: 0.0606 RA: 00 42 01.99 Decl: +40 50 55.8 seq: 121530 Bmag: 15.367+/-0.003 Vmag: 14.846+/-0.003 2MASS: dif: 0.0615 RA: 00 42 02.02 Decl: +40 50 55.9 Jmag: 13.534+/-0.032 Hmag: 13.209+/-0.035 Kmag: 13.136+/-0.036 Best regards, Maciej Reszelski