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J/AJ/106/1024      BV photometry in NGC 288                     (Bergbusch 1993)

Luminosity functions for post-turnoff stars in globular clusters. I. NGC 288 BERGBUSCH P.A. <Astron. J. 106, 1024 (1993)> =1993AJ....106.1024B
ADC_Keywords: Clusters, globular; Photometry Notes: The "appendix" file reaches approximately 1.5 magnitudes fainter than the table 7 in Appendix B of the paper, but the fainter data are highly uncertain. The data were derived from profile-fitting photometry as performed by DAOPHOT and the stand alone routine ALLSTAR, both of which have been developed by Peter Stetson of the DAO, Victoria, B.C. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file appendix 69 5601 The photometry for all stars (see above note)
Byte-by-byte Description of file: appendix
Bytes Format Units Label Explanations
3- 6 I4 --- ID Star number in cluster 10- 15 F6.2 pix X Position (North lies in the direction of decreasing X) 19- 24 F6.2 pix Y Position (West lies in the direction of decreasing Y) 28- 33 F6.3 mag Bmag B magnitude 38- 42 F5.3 mag e_Bmag Standard deviation on B 46- 51 F6.3 mag Vmag V magnitude 56- 60 F5.3 mag e_Vmag Standard deviation on V 65- 69 F5.3 --- chi mean chi value which indicates the quality of the profile fit
Historical Notes: Courtesy Peter A. Bergbush ()
(End) Francois Ochsenbein [CDS] 23-Dec-1993
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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