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J/A+AS/121/451      VI photometry of Berkeley 66 (Guarnieri+ 1997)

VI photometry of the galactic cluster Berkeley 66 Guarnieri M.D., Carraro G. <Astron. Astrophys. Suppl. Ser. 121, 451 (1997)> =1997A&AS..121..451G (SIMBAD/NED BibCode)
ADC_Keywords: Clusters, open ; Photometry Keywords: open clusters: Berkeley 66 - HR diagram Abstract: A colour magnitude diagram (CMD) extending to V≃19mag is given for 444 stars in the region of the galactic cluster Berkeley 66. The V and I photometry of a nearby field is also reported. This object appears very faint, highly contaminated by foreground stars and very reddened. The apparent distance modulus (m-M) and the colour excess EV-I are guessed to be 17.5 and 1.1, respectively, with an uncertainty of at least 30%. Adopting these values the comparison of the CMD with theoretical isochrones from the Padova group provides an age around 1.0Gyr. Objects: ------------------------------------------------ RA (2000) DE Designation(s) ------------------------------------------------ 03 04.3 +58 46 Berkeley 66 = C 0300+585 ------------------------------------------------ File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table2 42 444 VI photometry
Byte-by-byte Description of file: table2
Bytes Format Units Label Explanations
1- 3 I3 --- ID Identification number 5- 10 F6.3 mag Vmag V magnitude 12- 17 F6.3 mag Imag I magnitude 19- 24 F6.3 mag V-I V-I color index 26- 33 F8.3 pix Xpos X coordinate (1 pix = 0.47") 35- 42 F8.3 pix Ypos Y coordinate (1 pix = 0.47")
Table1: Journal of observations, 1.05m telescope, Pino Torinese, Torino (Italy) ------------------------------------------------------------------------------- Field Filter Exposure Seeing number (sec) (FWHM) ------------------------------------------------------------------------------- November 30, 1994 #1 I 60 1.41 #2 I 300 1.80 #3 I 180 1.35 #4 V 180 1.54 #5 V 120 1.54 #6 V 300 1.67 March 7, 1995 V 300 2.24 I 120 2.19 Acknowledgements: Giovanni Carraro
(End) Patricia Bauer [CDS] 18-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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