Dear colleagues! I would like to send you observations of a new variable star (Brh V118), which I have discovered in a systematic CCD-based search for new variables. In each observing run typically 400 images are taken of several survey fields. The frames are processed automatically. Instruments: CCD-camera: Starlight Xpress SX (unfiltered) Telescope: Celestron-8 (20 cm Schmidt-Cassegrain) New variable star: New Brh V118 164243.4 -033401.1 (J2000) 12.4-12.6 (CCD) comments: Brh V118: GSC 5053 989 The comparison star is GSC 5053 935 (11.15 mag), which has been checked for constant brightness. The USNO A2.0 magnitudes (r:11.9, b: 14.7) and the following observations suggest a long period variable, type and period still unknown. object YYMMDD(UT) mag(CCD) code Brh V118 020626.9068 12.48 Brh.BAV Brh V118 020628.9068 12.50 Brh.BAV Brh V118 020629.8853 12.46 Brh.BAV Brh V118 020705.9026 12.41 Brh.BAV Brh V118 020707.8742 12.39 Brh.BAV Brh V118 020708.8651 12.42 Brh.BAV Brh V118 020712.8783 12.42 Brh.BAV Brh V118 020720.8631 12.56 Brh.BAV Brh V118 020722.8519 12.57 Brh.BAV Vizier investigations show that further photometry for this object can be found via the TASS Mk III tenxcat database at: http://a188-l009.rit.edu/cgi-bin/tass_curve2.cgi?250.6801_-03.5673 Regards, Klaus Bernhard Klaus Bernhard Kafkaweg 5 A-4030 LINZ AUSTRIA kl.bernhard@aon.at http://mitglied.lycos.de/klausbernhard/