The design and testing of filter-detector systems using synthetic photometry

Details The design and testing of filter-detector systems using synthetic photometry The design and testing of filter-detector systems using synthetic photometry

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pasp..101..849b&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 101, Sept. 1989, p. 849-858.

Astronomy and Astrophysics

Astronomy

26

Astronomical Photometry, Charge Coupled Devices, Optical Filters, Bandwidth, Research And Development, Stellar Color

Scientific paper

Synthetic photometry is applied to the problem of designing a filter set that, when combined with a CCD, provides photometry that can be transferred to the Johnson (1955) UBV and the Kron-Cousins (1976) VRI systems. A filter set with transformation coefficients less than 0.07 is developed. The color and magnitude residuals from the synthetic photometry show that the transformations are linear over the color ranges, (B-V) between 0.0 and 1.4, (V-R) between 0.0 and 1.0, and (R-I) between 0.0 and 0.8.

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