Following suspected variable was found durning my scan of Amateur FITS Archive: AFASV_M31_125 AFASV_M31_125 amplitude=0.66 mag R. A. (2000) Decl. image 15.65 0 39 56.752 + 40 47 18.24 so1 14.99 0 39 56.918 + 40 47 20.31 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 IDENTIFICATIONS FROM VIZIER: USNO A2.0: dif: 0.1071 RA: 00 39 56.211 Decl: +40 47 16.24 USNOno: 1275-00401606 Bmag: 17.6 Rmag: 16.2 epoch: 1953.773 M31 field foreground stars (Berghujisen 1988): dif: 0.1060 RA: 00 39 56.25 Decl: +40 47 15.3 seq: 1154 Vmag: 15.93+/-0.16 U-B: 0.08 2MASS: dif: 0.1052 RA: 00 39 56.25 Decl: +40 47 15.4 Jmag: 14.804+/-0.049 Hmag: 14.395+/-0.060 Kmag: 14.335+/-0.085 NOTE: Object is close to following ROSAT source: 1RXS J004014.5+404958 dif: 0.981 RA: 00 39 53.3 Decl: +40 48 02 Rank:128 sourceID: [SHP97] 049 Also near located object is V7832 from M31F eclipsing and Cepheids catalog (Mochejska et al.) but V7832 have a Vmag value 21.39. So I exclude this object.