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J/A+A/440/735       V light curves of EK Dra                 (Jaervinen+, 2005)

Spots on EK Draconis - Active longitudes and cycles from long-term photometry. Jaervinen S.P., Berdyugina S.V., Strassmeier K.G. <Astron. Astrophys. 440, 735 (2005)> =2005A&A...440..735J
ADC_Keywords: Stars, variable ; Photometry Keywords: stars: activity - stars: starspot Description: We analyse photometric observations of the young active dwarf EK Dra, spanning altogether 21 years, and including previously unpublished data. The data in Table 2 was observed at the Fairbourn Observatory in southern Arizona using Amadeus, a 0.75m automatic photoelectric telescope (APT) of the University of Vienna. Amadeus is optimised for red wavelengths with an EMI-9828 tube and Johnson-Cousins V(RI)C filters. Differential V magnitudes are variable (EK Dra) - comparison (HD 129390) and check (HD 129798) - comparison (HD 129390). HD 129390 Vmag=7.567 Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 14 39 00.2 +64 17 30 EK DRA = V* EK Dra 14 39 22.8 +64 09 14 HD 129390 = BD+64 1018 14 42 03.2 +61 15 43 HD 129798 = V* DL Dra ---------------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table2.dat 38 2921 The new photometry of EK Dra
See also: J/A+AS/125/11 : UBV + V(RI)c photometry of 23 active stars (Strassmeier+ 1997) Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 9 A9 --- Star Star designation (EK Dra or HD 129798) 11- 23 F13.5 d HJD Heliocentric Julian Day 26- 31 F6.3 mag DVmag Differential V magnitude, Star - HD 129390 34- 38 F5.3 mag e_Vmag V1 standard error of mean
Acknowledgements: Silva Jarvinen, silva.jarvinen(at)iki.fi
(End) Patricia Vannier [CDS] 12-Jul-2005
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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