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Previous Page: 1983
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Previous: Photometric standards
Up: Appendices
Next: Some useful procedures
Previous Page: 1983
Next Page: References
The following table contains useful sequences for CCD observations. The
coordinates refer to the frame centre, and "No" is the number of stars in each
sequence falling within the 6 x 4 arcmin CCD frame of the INT prime focus.
V
and V
specify the range of magnitudes in broad-band V.
