Following suspected variable was found durning my scan of Amateur FITS Archive: AFASV_M31_388 AFASV_M31_388 amplitude=0.40 14.10 0 43 58.970 + 41 16 14.82 ugm 14.50 0 43 59.194 + 41 16 10.55 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: USNO A2.0: Uncertain USNO IDs. Two candidates, both are very faint: dif RA Decl USNOid Bmag Rmag epoch 0.1849 00 43 59.668 +41 16 22.62 1275-00440657 18.8 17.9 1953.773 0.1851 00 43 59.407 +41 16 04.85 1275-00440616 17.5 16.7 1953.773 BVRI CCD photometry in the field of M 31 (Magnier+ 1992): NOTE: uncertain ID dif: 0.1869 RA: 00 43 59.39 Decl: +41 16 04.6 seq: 252914 Bmag: 15.108+/-0.013 Vmag: 14.756+/-0.014 Brightest stars in the field of M31 (Berkhuijsen+ 1988): dif: 0.2546 RA: 00 43 59.60 Decl: +41 16 01.3 seq: 4733 Vmag: 15.31+/-0.17 2MASS (?): dif: 0.1290 RA: 00 43 59.66 Decl: +41 16 14.8 Jmag: 16.551+/-0.143 Hmag: 15.789+/-0.145 Kmag: 14.559 NOTE: Object may be identical with ROSAT source: 1RXS J004330.9+411452 = 1WGA J0043.9+4116 dif: 0.750 RA: 00 43 56.6 Decl: +41 15 39 rank: 307 Object is also not far form following M31 OB association (Magnier 1993): dif: 0.6659 RA: 00 44 02.35 Decl: +41 16 26.9 And Ionized nebula (Walterbos 1992): dif: 0.5272 RA: 00 43 58.36 Decl: +41 16 45.7 ID: 253 Best regards, Maciej Reszelski