Secondary Photometric Standards for Northern Nova-Like Cataclysmic Variables

An average of 11 B, V secondary standards per field have been established for 58 cataclysmic variable stars, most of which are nova-like variables. The standards are within a few arc minutes of the variable and are therefore well suited for CCD photometry. The standards have brightnesses of V ~ 12-17 and have a typical accuracy per standard of +-0.02 mag. (SECTION: Stars)