Dear colleagues! I would like to send you observations of a new variable star (Brh V120), 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 V120 184705.5 -033145.3 (J2000) 12.7-12.9 (CCD) comments: Brh V120: GSC 5118 427 The comparison star is GSC 5122 294 (12.2 mag), which has been checked for constant brightness. The USNO A2.0 magnitudes (r:10.8, b: 14.6) and the following observations suggest a long period variable, type and period still unknown. object YYMMDD(UT) mag(CCD) code Brh V120 020626.9929 12.67 Brh.BAV Brh V120 020628.9929 12.73 Brh.BAV Brh V120 020705.9888 12.77 Brh.BAV Brh V120 020707.9603 12.79 Brh.BAV Brh V120 020708.9513 12.82 Brh.BAV Brh V120 020719.9485 12.83 Brh.BAV Brh V120 020814.8750 12.94 Brh.BAV Brh V120 020814.8757 12.85 Brh.BAV Brh V120 020814.8764 12.84 Brh.BAV Brh V120 020814.8771 12.85 Brh.BAV Brh V120 020814.8778 12.89 Brh.BAV Brh V120 020814.8785 12.88 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?281.7733_-03.5295 These observations (especially I-band) confirm the variability of GSC 5118 427. Regards, Klaus Bernhard Klaus Bernhard Kafkaweg 5 A-4030 LINZ AUSTRIA kl.bernhard@aon.at http://mitglied.lycos.de/klausbernhard/