Following suspected variable was found durning my scan of Amateur FITS Archive: AFASV_M31_473 AFASV_M31_473 amplitude=0.52 mag RA (2000) Decl. image 14.30 0 45 08.784 + 41 26 10.01 ugm 14.82 0 45 09.040 + 41 26 05.88 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: rad: 0.0840 RA: 00 45 09.04 Decl: +41 26 05.7 GSCid: 0280500521 mag: 14.08+/-0.39 USNO A2.0: rad: 0.0826 RA: 00 45 09.102 Decl: +41 26 06.39 USNOid: 1275-00451937 Bmag: 16.1 Vmag: 14.1 epoch: 1953.773 Brightest stars in the field of M31 (Berkhuijsen+ 1988): rad: 0.1725 RA: 00 45 09.37 Decl: +41 26 01.9 seq: 3682 Vmag: 14.81+/-0.16 BVRI CCD photometry in the field of M 31 (Magnier+ 1992): rad: 0.0876 RA: 00 45 09.08 Decl: +41 26 05.8 seq: 300800 Bmag: 15.022+/-0.006 Vmag: 14.538+/-0.003 Imag: 13.848 2MASS: rad: 0.0858 RA: 00 45 09.08 Decl: +41 26 05.9 Jmag: 13.206+/-0.027 Hmag: 12.846+/-0.029 Kmag: 12.780+/-0.025 Best regards, Maciej Reszelski