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J/other/JAD/18.5    Long-term photometry of 11 RS CVn stars     (Heckert, 2012)

Two decades of optical photometry of short-period eclipsing RS CVn systems and other active chromosphere systems. Heckert P.A. <J. Astron. Data, 18, 5-16 (2012)> =2012JAD....18....5H
ADC_Keywords: Stars, variable ; Photometry, UBVRI ; Binaries, eclipsing Keywords: technique: photometric - stars: variable - stars: eclipsing - stars: RS CVn Abstract: I present BVRI photometry of short-period (P<1d) eclipsing RS CVn binary star systems collected between 1988 and 2009 at Mount Laguna Observatory. Most of the data are for ER Vul and WY Cnc, with light curves nearly every year during that time period. I also present light curves for at least several years for XY UMa, BH Vir, CG Cyg, RT And, and UV Psc. I have fewer light curves for SV Cam, UV Leo, 1E1919+0427, and GSC 2038-0293. In addition to the eclipsing short-period systems, I also include UBVRI data for two longer period non-eclipsing RS CVn binary systems: UZ Lib and DM UMa, as well as two active chromosphere single stars: FK Com and HD 199178. Description: I used the 0.6-m (24") telescope at Mount Laguna Observatory operated by San Diego State University for all the observations reported in this paper. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file stars.dat 103 11 List of studied stars table3.dat 30 11948 WY Cancri photometry table4.dat 30 13018 ER Vulpeculae photometry table5.dat 30 5431 XY Ursa Majoris photometry table6.dat 30 8137 BH Virginis photometry table7.dat 30 9124 CG Cygni photometry table8.dat 30 6424 RT Andromedae photometry table9.dat 30 3680 UV Psc photometry table10.dat 30 1104 SV Cam photometry table11.dat 30 480 UV Leo photometry table12.dat 30 948 GSC 2038-0293 photometry table13.dat 30 746 1E1919+0427 photometry
Byte-by-byte Description of file: stars.dat
Bytes Format Units Label Explanations
1- 15 A15 --- Star Star name 17- 50 A34 --- Years Years of observations 52- 64 A13 --- Comp Comparison star name 65 A1 --- n_Comp [*] Note on Comp (1) 66- 78 F13.5 d T0 T0 used for phase (2) 81- 91 F11.9 d Per Period used for phase (2) 93-103 A11 --- FileName Name of the file with photometry
Note (1): For 1E1919+0427, the comparison star is Star A of Summers & Heckert, 1997AJ....113.2242S, identified as 2MASS 19215198+0433384 by CDS. Note (2): Phase=T0+Per*E.
Byte-by-byte Description of file: table*.dat
Bytes Format Units Label Explanations
1- 2 A2 --- Band [BVRIv 50] Observed band (1) 5- 9 F5.3 --- Phase Phase 11- 17 F7.4 mag Dmag Differential magnitude in Band 19- 30 F12.4 d HJD ? Heliocentric Julian date
Note (1): BVRI in standard Johnson-Cousins system (except for WY Cnc 2009), v is the instrumental v band, and 50 is unexplained. observed with Mt Laguna Observatory 24" telescope.
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 10-Jul-2012
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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