Light curves of 5 cataclysmic variables (Papadaki+, 2006)

Details Light curves of 5 cataclysmic variables (Papadaki+, 2006) Light curves of 5 cataclysmic variables (Papadaki+, 2006)

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ycat..34560599p&link_type=abstract

VizieR On-line Data Catalog: J/A+A/456/599. Originally published in: 2006A&A...456..599P

Computer Science

Stars: Variable, Photometry

Scientific paper

tablea1.dat describes the observing log. We have performed photometric observations of five relatively poorly-studied cataclysmic variables: V1193 Ori, LQ Peg, LD 317, V795 Her and MCT 2347-3144. For each target, we give the UT dates it was observed, the site where the observations took place, the Heliocentric Julian Date at the beginning of each observing night, the total duration of each run and which filter, if any, was used.
table1.dat shows (for V1193 Ori, LD 317 and MCT 2347-3144) the mean nightly magnitude of each CV along with the variation of the difference between two comparison stars.
figA2.dat-figA6.dat give the light curves of V1193 Ori, LQ Peg, LD 317, V795 Her and MCT 2347-3144, respectively. In figA3.dat, figA4.dat and figA5.dat the magnitude is in arbitrary units.
(7 data files).

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