Following suspected variable was found durning my scan of Amateur FITS Archive: AFASV_M31_510 AFASV_M31_510 amplitude=0.39 mag RA (2000) Decl. image 14.04 0 45 41.937 + 41 30 49.42 ugm 14.43 0 45 42.209 + 41 30 49.02 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: 0.0498 RA: 00 45 42.20 Decl: +41 30 48.4 GSCid: 0280500533 mag: 13.90+/-0.39 USNO A2.0: rad: 0.0528 RA: 00 45 42.217 Decl: +41 30 48.64 USNOid: 1275-00457095 Bmag: 14.9 Rmag: 14.1 epoch: 1953.773 Brightest stars in the field of M31 (Berkhuijsen+ 1988): rad: 0.1457 RA: 00 45 42.53 Decl: +41 30 43.6 seq: 4305 Vmag: 14.50+/-0.15 BVRI CCD photometry in the field of M 31 (Magnier+ 1992): rad: 0.0532 RA: 00 45 42.21 Decl: +41 30 48.3 seq: 327310 Bmag: 14.747+/-0.017 Rmag: 14.256+/-0.008 2MASS: rad: 0.0610 RA: 00 45 42.26 Decl: +41 30 48.5 Jmag: 12.920+/-0.024 Hmag: 12.581+/-0.026 Kmag: 12.585+/-0.028 Best regards, Maciej Reszelski