Following suspected variable was found durning my scan of Amateur FITS Archive: AFASV_M31_436 AFASV_M31_436 amplitude=0.32 mag RA (2000) Decl. image 14.97 0 44 40.658 + 41 36 28.67 so1 14.65 0 44 40.866 + 41 36 27.64 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: rad: 0.0706 RA: 00 44 40.976 Decl: +41 36 28.24 USNOid: 1275-00447320 Bmag: 17.0 Rmag: 15.8 epoch: 1953.773 Brightest stars in the field of M31 (Berkhuijsen+ 1988): rad: 0.1573 RA: 00 44 41.34 Decl: +41 36 24.2 seq: 2976 Vmag: 15.08+/-0.17 BVRI CCD photometry in the field of M 31 (Magnier+ 1992): rad: 0.0694 RA: 00 44 40.97 Decl: +41 36 28.2 seq: 361731 Bmag: 15.287+/-0.014 Vmag: 14.764+/-0.033 Rmag: 14.380 Imag: 14.109 2MASS: rad: 0.0687 RA: 00 44 40.96 Decl: +41 36 28.1 Jmag: 13.487+/-0.030 Hmag: 13.191+/-0.036 Kmag: 13.139+/-0.043 Best regards, Maciej Reszelski