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Flux Calibration Issues

Published online by Cambridge University Press:  01 December 2006

Andrew J. Pickles
Andrew J. Pickles*
Affiliation:
Caltech, 1200 E. California Blvd., Pasadena, CA 91225, USA email: pick@astro.caltech.edu
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Abstract

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Recent stellar spectral libraries have sought higher resolution and the accurate determination of specific optical spectral indeces as stellar population indicators. But the value of accurate flux comparisons over wide wavelength regions should still be emphasized, particularly as more and better spectro-photometric data for composite populations becomes available.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S241: Stellar Populations as Building Blocks of Galaxies , December 2006 , pp. 82 - 86
Copyright
Copyright © International Astronomical Union 2007

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