CCD photometry of WX Ceti in quiescence and outburst

C. Sterken, N. Vogt, M. Uemura, T. Tuvikene, M. Knudsen and H. W. Duerbeck

WX Cet (Nova Cet 1963) - a SU UMa type dwarf nova - was observed in 2001 and in 2004-2005 during superoutburst and subsequent quiescence. This paper presents the complete light curve material in digital form, and provides a number of nightly-averaged BVR CCD frames of the WX Ceti field for calibration purposes.

 Table  Description  Band  Comparison star
 DAN_WX_B  WX Ceti light curve obtained at La Silla  B  Star 7
 DAN_WX_V  WX Ceti light curve obtained at La Silla  V  Star 7
 DAN_WX_R  WX Ceti light curve obtained at La Silla  R  Star 7
 LC1_WX_B  WX Ceti light curve, Las Campanas Observatory, July 2001  B  BD-18206
 LC1_WX_V  WX Ceti light curve, Las Campanas Observatory, July 2001  V  BD-18206
 LC1_WX_R  WX Ceti light curve, Las Campanas Observatory, July 2001  R  BD-18206
 LC2_WX_B  WX Ceti light curve, Las Campanas Observatory, August 2001  B  Star 10
 LC2_WX_V  WX Ceti light curve, Las Campanas Observatory, August 2001  V  Star 10
 OCA_WX_R  WX Ceti light curve, Observatorio Cerro Armazones  R  BD-18206
 CPC_WX  WX Ceti light curve obtained at Concepcion University  No filter  Star 7
       
 DAN_B  field stars, Danish Telescope La Silla  B  Star 7
 DAN_V  field stars, Danish Telescope La Silla  V  Star 7
 DAN_R   field stars, Danish Telescope La Silla  R  Star 7
  OCA_R  field stars, Observatorio Cerro Armazones  R  BD-18206