Following suspected variable was found durning my scan of Amateur FITS Archive: AFASV_M31_485 AFASV_M31_485 amplitude=0.35 mag RA (2000) Decl. image 13.58 0 45 21.002 + 41 17 17.76 ugm 14.33 0 45 21.045 + 41 17 01.33 so1 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: rad: 0.3047 RA: 00 45 21.08 Decl: +41 16 59.3 GSCid: 0280500126 mag: 13.84+/-0.40 USNO A2.0: rad: 0.2962 RA: 00 45 21.122 Decl: +41 16 59.88 USNOid: 1275-00453822 Bmag: 14.9 Rmag: 14.5 epoch: 1953.773 Brightest stars in the field of M31 (Berkhuijsen+ 1988): rad: 0.3817 RA: 00 45 21.31 Decl: +41 16 55.0 seq: 3943 Vmag: 14.34+/-0.16 2MASS: rad: 0.3041 RA: 00 45 21.11 Decl: +41 16 59.4 Jmag: 12.376+/-0.027 Hmag: 11.901+/-0.031 Kmag: 11.786+/-0.025 Best regards, Maciej Reszelski