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J/A+A/376/158       SV Cam BVR light curves                  (Albayrak+, 2001)

A light and period study of SV Camelopardalis Albayrak B., Demircan O., Djurasevic G., Erkapic S., Ak H. <Astron. Astrophys. 376, 158 (2001)> =2001A&A...376..158A
ADC_Keywords: Binaries, eclipsing ; Photometry Keywords: stars: binaries: eclipsing - stars: individual: SV Cam Abstract: New BVR light curves and times of minimum light for the short period RS CVn system SV Cam were analysed to derive the physical parameters of the system and the parameters of the third body orbit. The light curves obtained at the TUEBITAK National Observatory during two nights in 2000 show considerable asymmetry and night-to-night variations. The analysis of the light curves is made using Djurasevic's inverse problem method. The Roche model with spotted areas on the hotter primary component yields a good fit to observations. The extensive series of published photoelectric minima times indicate that the eclipsing pair orbits around the common mass center of the triple system with a period of 41.32yr. Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 06 41 19.1 +82 16 02 SV Cam ---------------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 34 242 The photoelectric observations of SV Cam obtained in B, V, and R filters table1.tex 77 284 LaTeX version of table1
Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 13 F13.5 d HJD Heliocentric Julian date 15- 20 F6.3 mag DBmag Differential B magnitude (variable minus comp.) 22- 26 F5.3 mag DVmag Differential V magnitude 28- 32 F5.3 mag DRmag Differential R magnitude
Acknowledgements: B. Albayrak
(End) Patricia Bauer [CDS] 13-Jul-2001
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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