Walraven photometry of WX Hyi

The SU UMa-type dwarf nova WX Hyi was observed in the 5 passbands VBLUW (544, 430, 384, 362 and 324nm) during 15 nights on the 90cm telescope at ESO (La Silla), between July and...SU UMa型矮新星（SU UMa-type dwarf nova）WX Hyi于7月至[原文未完整给出的后续时段]间的15个观测夜中，借助位于欧洲南方天文台（ESO）拉西拉（La Silla）站点的90厘米口径望远镜，在VBLUW五个测光波段下完成观测，各波段中心波长分别为544 nm、430 nm、384 nm、362 nm及324 nm。