The eclipsing dwarf nova EX Hydrae was monitored during 29 hours in Stromgren uvby, and, at the same occasion, during 45 hours in the $B$ band of the Johnson system. We present these data (more than 18,000 discrete magnitudes) in extenso, and scrutinize their quality in relation to their future employment in an analysis of flickering.
Journal of Astronomical Data
- Pub Date:
- STARS: VARIABLE;
- STARS: NOOVAE AND CATACLYSMIC VARIABLES;
- EX HYA