285 V379 PEGASI (ZAND:) Range: 13.9-<16.2 Position: 23 53 52.47 +23 09 20.6 (J2000, from .dat file) Magnitude: V=18.589 B-V=0.159 (Henden, dat file) ID RA (2000) DEC X Y N V ERR B-V ERR a) Comparison star sequence 1 23 53 43.1 +23 14 18 -130 297 1 11.358 9.999 0.535 9.999 2 23 54 10.0 +23 11 56 242 155 1 11.640 9.999 1.175 9.999 3 23 54 15.4 +23 12 38 316 197 1 12.244 9.999 1.235 9.999 4 23 53 47.0 +23 09 04 -76 -17 1 13.242 9.999 1.216 9.999 5 23 53 52.1 +23 11 15 -5 114 1 13.413 9.999 0.773 9.999 6 23 54 02.1 +23 05 24 133 -237 2 14.208 0.006 0.732 0.001 7 23 53 59.1 +23 10 59 91 98 1 14.566 9.999 1.044 9.999 8 23 53 56.5 +23 08 10 55 -71 1 15.091 9.999 0.972 9.999 9 23 53 47.4 +23 06 38 -70 -163 1 15.641 9.999 0.843 9.999 10 23 53 36.2 +23 09 09 -225 -12 1 16.642 9.999 0.866 9.999 11 23 53 56.1 +23 09 19 49 -2 1 17.587 9.999 0.752 9.999 b) Wide-colour extension for CCD calibration 23 53 50.9 +23 09 19 -22 -2 1 15.161 9.999 1.537 9.999 Notes: 1. V379 Peg is classified as a ZAND variable in Namelist 76. However from the colours found during the determination of this sequence it almost definitely a cataclysmic variable, probably a unrecognised dwarf nova. 2. This single night sequence is expected to have errors of +/-0.02 mag. 3. This star was previously known as Peg 7, FBS2351, SVS 2550 and NSV26158. 4. The star identified by Downes, et.al, Atlas of Cataclysmic Variables, Living Edition as V379 Peg is not the variable. They identify the star here shown as the V=15.161 red wide colour extension red star as the variable. It is possible that this star is a symbiotic variable, but the faint star 22 arcsec due east of this red star is most likely the 'real' V379 Peg. Bruce Sumner 21 April 2002