Following suspected variable was found durning my scan of Amateur FITS Archive: AFASV_M31_246 AFASV_M31_246 amplitude=0.53 mag R. A. (2000) Decl. image 14.79 0 41 44.128 + 40 47 28.84 ugm 15.32 0 41 44.209 + 40 47 30.90 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: USNO A2.0 dif: 0.0236 RA: 00 41 44.191 Decl: +40 47 30.00 USNOid: 1275-00419363 Bmag: 17.1 Rmag: 15.6 epoch: 1953.773 Brightest stars in the field of M31 (Berkhuijsen+ 1988): dif: 0.0330 RA: 00 41 44.29 Decl: +40 47 28.2 seq: 3598 Vmag: 15.37+/-0.16 BVRI CCD photometry in the field of M 31 (Magnier+ 1992): dif: 0.0200 RA: 00 41 44.21 Decl: +40 47 29.4 seq: 112038 Bmag: 15.595+/-0.019 Vmag: 14.968+/-0.001 2MASS: dif: 0.0292 RA: 00 41 44.25 Decl: +40 47 29.7 Jmag: 13.403+/-0.038 Hmag: 12.935+/-0.035 Kmag: 12.884+/-0.040 Possible also: Objective-prism survey of em. objects in M31 (Meyssonnier+ 1993): dif: 0.732 RA: 00 41 44.5 Decl: +40 48 13 Best regards, Maciej Reszelski