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J/ApJS/85/293      HST Observations of core of 47 Tuc          (de Marchi+ 1993)

The structure of the core of 47 Tucanae from Hubble Space Telescope observations DE MARCHI G., PARESCE F., FERRARO F.R. <Astrophys. J. Suppl. Ser. 85, 293 (1993)> =1993ApJS...85..293D
ADC_Keywords: Clusters, globular; Positional data; Photometry Keywords: globular clusters: individual (47 Tuc) - Hertsprung-Russel diagram - stars: luminosity function, mass function - techniques: image processing File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1 32 3567 Stellar photometry: U band table2 40 391 Stellar photometry: F220W and U bands table3 64 134 Stellar photometry: F140W, F220W and UBV bands
Byte-by-byte Description of file: table1
Bytes Format Units Label Explanations
5- 8 I4 --- ID [1-3567]+ ID number 14- 16 I3 pix X X position form the lower left corner of Fig.4 21- 24 I4 pix Y Y position form the lower left corner of Fig.4 29- 32 F4.1 mag m342 HST instrumental magnitude of all the 3567 stars detected and measured on the 44" x 44" U-band image named Fig.4
Byte-by-byte Description of file: table2
Bytes Format Units Label Explanations
5- 8 I4 --- ID ID number 14- 16 I3 pix X X position as in table1 22- 24 I3 pix Y Y position as in table1 29- 32 F4.1 mag m220 HST instrumental magnitudes of all the 391 stars measured on the summed FOC F220W filter frame named Fig.3 37- 40 F4.1 mag m342 Corresponding m342 magnitude
Byte-by-byte Description of file: table3
Bytes Format Units Label Explanations
5- 8 I4 --- ID ID number 14- 16 I3 pix X X position 22- 24 I3 pix Y Y position 29- 32 F4.1 mag m140 magnitude at 140 nm 37- 40 F4.1 mag m220 magnitude at 220 nm 45- 48 F4.1 mag m342 m342 magnitude 53- 56 F4.1 mag B []? B magnitude 61- 64 F4.1 mag V []? V magnitude
Note: This table list m140, m220, m342, B and V magnitudes of all the stars having either HST instrumental magnitude m140 (measured on Fig. 2 of this paper) or B or V magnitudes available. B and V magnitudes are taken from the list provided by Auriere, Koch-Miramond & Ortolani (1989, A&A, 204, 106) when available. For those blue straggler stars which were not measured by these Authors, we took B and V magnitudes from Paresce et al. (1991, Nature, 352, 297). Corutesy: Guido De Marchi
(End) Patricia Bauer [CDS] 24-Jun-1994
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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