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J/A+AS/121/499      BV and rg photometry of Pal 13 (Borissova+ 1997)

CCD photometry of the globular cluster Palomar 13 Borissova J., Markov H., Spassova N. <Astron. Astrophys. Suppl. Ser. 121, 499 (1997)> =1997A&AS..121..499B (SIMBAD/NED BibCode)
ADC_Keywords: Photometry, CCD ; Clusters, globular Keywords: globular clusters: individual: Palomar 13 - Hertzprung-Russel diagram Abstract: A new CCD photometry of the halo cluster Palomar 13 is used to construct a color-magnitude diagram in the Thuan-Gunn and the B, V photometric systems. The color-magnitude diagram of the cluster shows as already noted by Ortolani et al. (1985AJ.....90..473O) an extremely poor red horizontal branch and a very sparsely populated giant branch. Seven BSS candidates are identified in the field of Palomar 13. The age of the cluster determined by fitting with the isochrones of Proffitt & Vanden Berg (1991ApJS...77..473P) and Bergbusch & Vanden Berg (1992ApJS...81..163B) and by a differential comparison of the color-magnitude diagram with that of Pal 5 is 12±2Gyr. Objects: ------------------------------------------- RA (2000) DE Designation(s) ------------------------------------------- 23 06.5 +12 44 Pal 13 = C 2304+124 ------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table6 35 80 B,V photometry of Pal 13 table7 36 175 g,r photometry of Pal 13
Byte-by-byte Description of file: table6
Bytes Format Units Label Explanations
1- 2 I2 --- ID Identification number 7- 11 F5.1 pix Xpos X position (1 pix = 0.30 arcsec) 15- 19 F5.1 pix Ypos Y position (1 pix = 0.34 arcsec) 24- 28 F5.2 mag Vmag V magnitude 32- 35 F4.2 mag B-V B-V color index
Byte-by-byte Description of file: table7
Bytes Format Units Label Explanations
2- 4 I3 --- ID Identification number 8- 13 F6.2 pix Xpos X position (1 pix = 0.30 arcsec) 16- 21 F6.2 pix Ypos Y position (1 pix = 0.34 arcsec) 25- 29 F5.2 mag gmag g magnitude 32- 36 F5.2 mag g-r g-r color index
Acknowledgements: J. Borissova
(End) Patricia Bauer [CDS] 28-Jun-1996
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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