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J/A+AS/127/423      VI photometry of Westerlund 1 and 2  (Piatti+ 1998)

Fundamental parameters of the highly reddened young open clusters Westerlund 1 and 2 Piatti A.E., Bica E., Claria J.J. <Astron. Astrophys. Suppl. Ser. 127, 423 (1998)> =1998A&AS..127..423P (SIMBAD/NED BibCode)
ADC_Keywords: Clusters, open ; Photometry, CCD Keywords: open clusters: individual: Weterlund 1, Westerlund 2 - open clusters: general - HR diagram Description: We have carried out CCD observations of stars in the region of the open cluster Westerlund 1 through the V and I passbands. The direct images were obtained with the 24-inch telescope of the University of Toronto Southern Observatory situated at Las Campanas Observatory, Chile. After cross-correlating all independent V, (V-I) tables we have obtained a improved set of colour and magnitude values as compared to those based on a single measure. Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 16 48.2 -45 50 Westerlund 1 = C 1644-457 10 23.9 -57 45 Westerlund 2 = C 1022-575 ---------------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table 59 233 Photometric data
See also: J/ApJS/116/263 : VI photometry of open clusters (Piatti+ 1998) Byte-by-byte Description of file: table
Bytes Format Units Label Explanations
1- 3 A3 --- ID Star number 7- 12 F6.2 pix Xpos X coordinate (1) 16- 21 F6.2 pix Ypos Y coordinate (1) 25- 30 F6.3 mag Vmag V magnitude 34- 38 F5.3 mag e_Vmag ? V magnitude error 42- 46 F5.3 mag V-I V-I colour 50- 54 F5.3 mag e_V-I ? V-I colour error 58 I1 --- o_Vmag Number of measurements
Note (1): X and Y coordinates increase toward the north and west, respectively.
Acknowledgements: Andres Piatti
(End) Patricia Bauer [CDS] 02-Jun-1997
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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