Following suspected variable was found durning my scan of Amateur FITS Archive: AFASV_M31_237 AFASV_M31_237 amplitude=0.38 mag R. A. (2000) Decl. image 13.37 0 41 33.583 + 41 28 54.66 ugm 13.75 0 41 33.604 + 41 28 47.43 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: dif: 0.1276 RA: 00 41 33.89 Decl: +41 28 47.9 GSCid: 0280500210 mag: 13.57+/-0.34 USNO A2.0: dif: 0.1262 RA: 00 41 33.930 Decl: +41 28 48.22 USNOid: 1275-00417747 Bmag: 15.1 Rmag: 14.1 epoch: 1953.773 Brightest stars in the field of M31 (Berkhuijsen+ 1988) : dif: 0.1811 RA: 00 41 34.19 Decl: +41 28 46.3 41 seq: 209 Vmag: 13.37+/-0.15 U-B: 1.38 The WGACAT version of ROSAT sources (White+ 2000): 1WGA J0041.5+4129 dif: 0.327 RA: 00 41 33.7 Decl: +41 29 14 2MASS dif: 0.1257 RA: 00 41 33.92 Decl: +41 28 48.2 Jmag: 11.913+/-0.035 Hmag: 11.350+/-0.033 Kmag: 11.212+/-0.032 Best regards, Maciej Reszelski