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J/PASP/121/699      BVR photometry of V343 Ori               (Yang+, 2009)

BVR observations and period variation of the neglected contact binary V343 Orionis. Yang Y.-G. <Publ. Astron. Soc. Pac., 121, 699-707 (2009)> =2009PASP..121..699Y
ADC_Keywords: Stars, variable ; Photometry, UBVRI Abstract: BVR light curves of V343 Orionis were observed with the 85cm telescope at Xinglong Station of the National Astronomical Observatories of the Chinese Academy of Sciences, in 2007 and 2008. Using the Wilson-Devinney program, the photometric solution of V343 Ori was first deduced from those observations. Photometric results indicated that V343 Ori is an A-subtype W Ursae Majoris binary, whose mass ratio and overcontact degree are q=0.253(±0.004) and f=86.9%(±2.1%), respectively. Description: Photometric observations for V343 Ori were performed in 2007 December and 2008 October, using the 85cm telescope at Xinglong Station of National Astronomical Observatories of the Chinese Academy of Sciences (NAOC). Objects: --------------------------------------------------- RA (2000) DE Designation(s) --------------------------------------------------- 06 05 00.3 +12 33 05 V343 Ori = V* V343 Ori --------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table2.dat 21 2407 BVR-band observations for eclipsing binary V343 Ori
Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1 A1 --- Band [BVR] Observed band 3- 14 F12.4 d HJD Heliocentric Julian date 16- 21 F6.3 mag Dmag Differential magnitude in Band (1)
Note (1): Coordinates of the Variable, Comparison, and Check stars: Variable : RA=06:05:00.3, DE=+12:33:04.8 (J2000) (V343 Ori) Comparison : RA=06:05:16.5, DE=+12:37:58.0 (J2000) (GSC 725-895) Check : RA=06:04:58.7, DE=+12:30:14.6 (J2000) (GSC 725-450)
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 30-Dec-2009
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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