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J/A+A/410/523       Carina Spiral Feature ubvybeta photometry (Kaltcheva, 2003)

The Carina Spiral Feature: Stroemgren-Hβ photometry approach. I. The photometric data-base Kaltcheva N.T. <Astron. Astrophys. 410, 523 (2003)> =2003A&A...410..523K
ADC_Keywords: Stars, early-type ; Photometry, uvby, beta Keywords: stars: early-type Abstract: A data-base collating all uvbyβ photometry available at present for O-B9 stars brighter than 10th visual magnitude in the field of the Carina Spiral Feature is presented. The completeness and homogeneity of the data-base are discussed. Description: In table 1, the data-base is presented. An identification (HD or CPD) is given in the first column. Columns 2, 3, 4, 5, and 6 give V, b-y, m1, c1 and Hβ. The Galactic coordinates, cross-identifications and the spectral type follow. The stars without photometry or with partial photometry only are left in the data-base as future program stars. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 101 1171 Data-base of uvbyβ in Carina
See also: J/A+AS/128/309 : ubvy-beta photometry of CarOB1 & CarOB2 stars (Kaltcheva 1998) J/A+AS/146/365 : O + B stars uvby-Hbeta photometry. III. (Kaltcheva+, 2000) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 13 A13 --- Name Star designation 15- 20 F6.3 mag Vmag Johnson V magnitude 22- 27 F6.3 mag (b-y) ? Stroemgren b-y colour index 29- 34 F6.3 mag m1 ? Stroemgren m1 colour index 36- 41 F6.3 mag c1 ? Stroemgren c1 colour index 43- 47 F5.3 mag Hbeta ? Hβ index 49- 54 F6.2 deg GLON Galactic longitude 56- 60 F5.2 deg GLAT Galactic latitude 62- 71 A10 --- CPD ? CPD number 73- 78 I6 --- PPM ? PPM number 80- 87 A8 --- LS ? LS number 89-101 A13 --- SpType ? MK Spectral and Luminosity Classification
Acknowledgements: Nadia Kaltcheva
(End) Patricia Bauer [CDS] 21-Oct-2003
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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