Following suspected variable was found durning my scan of Amateur FITS Archive: AFASV_M31_330 AFASV_M31_330 amplitude=0.35 mag R. A. (2000) Decl. image 13.64 0 43 09.826 + 41 3 45.53 so1 13.99 0 43 09.913 + 41 3 43.42 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: 0.0203 RA: 00 43 09.765 Decl: +41 03 46.65 USNOid: 1275-00432839 Bmag: 14.4 Rmag: 13.7 epoch: 1953.773 Brightest stars in the field of M31 (Berkhuijsen+ 1988): dif: 0.0437 RA: 00 43 09.92 Decl: +41 03 43.2 seq: 4399 Vmag: 13.71+/-0.13 BVRI CCD photometry in the field of M 31 (Magnier+ 1992): dif: 0.0199 RA: 00 43 09.91 Decl: +41 03 45.6 seq: 179067 Bmag: 14.132+/-0.014 Vmag: 13.623+/-0.013 Rmag: 13.253 Imag: 12.976 2MASS: dif: 0.0319 RA: 00 43 09.97 Decl: +41 03 45.8 Jmag: 12.197+/-0.039 Hmag: 11.864+/-0.033 Kmag: 11.779+/-0.037 Best regards, Maciej Reszelski