Disclaimer: The following document (from catalogue J/PASP/104/553) results from an on-line translation from latex to html (the cgiprint tool developed at CDS). The correct presentation requires an execution of latex on the original file
(Odewahn, S. C., Bryja, C., and Humphreys, R. M.)
The authors have combined multiple nights of CCD observations of NGC 7790, NGC
7006, and NGC 4147 in order to establish deep sequences of photometric
standards whose errors have been objectively derived through statistical
comparisons. Values are given for B, V, and R for stars in the magnitude range
12.8 to 20.2.
This document describes the indigenous characteristics of the machine-readable version of the Improved CCD Standard Fields to a computer. A copy should be transmitted with any additional copy of this catalog.
The Improved CCD Standard Fields as distributed here is in a single fixed block file. It contains 273 records of 80 bytes each. The four tables in the printed paper have been concatenated into one with the SGP field first, followed by F401 and with all data for each quasar on a single line.
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Note: X is positive to the west; Y is positive to the north.