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J/A+AS/134/317      BR photometry of UGC 685                 (Hopp, 1999)

Distance, structure and bright stellar content of the dwarf irregular galaxy UGC 685. Hopp U. <Astron. Astrophys. Suppl. Ser. 134, 317 (1999)> =1999A&AS..134..317H
ADC_Keywords: Galaxies, photometry ; Photometry, CCD Keywords: galaxies - dwarfs; galaxies - structure; galaxies - distances Abstract: B and R CCD images and J NICMOS3 frames taken with the Calar Alto 3.5m telescope of the dwarf irregular galaxy UGC 685 are presented. The brightest part of the stellar population is resolved in B and R, very few also in J. The stellar color-magnitude diagram is discussed. An estimate of the distance to UGC 685 of 5. 5Mpc is derived based on the brightest blue supergiant stars. Most of the resolved bright stars show colors in the range -0.1≤B-R≤+0.7. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table3.dat 48 171 Stars found in B and R on the UGC 685 frames
Byte-by-byte Description of file: table3.dat
Bytes Format Units Label Explanations
1- 3 I3 --- [H99] Sequential number 5- 9 F5.1 arcsec Xpos X position (1) 12- 16 F5.1 arcsec Ypos Y position (1) 19- 23 F5.2 mag Bmag B magnitude 26- 29 F4.2 mag e_Bmag rms uncertainty on Bmag 32- 36 F5.2 mag Rmag R magnitude 39- 42 F4.2 mag e_Rmag rms uncertainty on Rmag 44- 48 F5.2 mag B-R B-R colour index
Note (1): +x increases towards East and +y increases towards South
History: Prepared via OCR at CDS.
(End) James Marcout, Patricia Bauer [CDS] 27-Aug-1999
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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