Numerical convolution photometry - an example using the Stromgren four-color system

Details Numerical convolution photometry - an example using the Stromgren four-color system Numerical convolution photometry - an example using the Stromgren four-color system

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986aj.....91..171h&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 91, Jan. 1986, p. 171-176.

Astronomy and Astrophysics

Astronomy

4

Blue Stars, Convolution Integrals, Stellar Color, Stellar Spectrophotometry, Bandpass Filters, Linear Transformations, Stellar Spectra, Stellar Temperature, White Dwarf Stars

Scientific paper

The method of numerical convolution photometry is presented. This method is then applied to spectrophotometric observations of hot blue stars using the Strömgren four-color photometric system. New color relations are discussed as well as their usefulness in determining some intrinsic properties of the program stars, in particular, the white dwarfs. A discussion of the errors involved and the accuracy of this method is also included.

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