An Alternative Approach for Finding and Applying Extinction-corrected Magnitude Transformations

Details An Alternative Approach for Finding and Applying Extinction-corrected Magnitude Transformations An Alternative Approach for Finding and Applying Extinction-corrected Magnitude Transformations

May 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011sass...30..127b&link_type=abstract

The Society for Astronomical Sciences 30th Annual Symposium on Telescope Science. Held May 24-26, 2011 at Big Bear Lake, CA. Pu

Astronomy and Astrophysics

Astronomy

Scientific paper

We describe and demonstrate an alternative approach for finding and applying the transformations required to convert instrumental magnitudes to magnitudes on a photometric standard system including correction for atmospheric extinction. The method is aimed at those using differential photometry with small-field CCD cameras and working in climates where photometric conditions occur only rarely. Both primary and secondary standard stars are used to enable observers at geographical latitudes far from the equator to measure the required parameters over a wide air mass range.

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