The important role of stellar atmosphere spectra for a consistent spectrophotometric calibration from the optical to the infrared wavelengths

Details The important role of stellar atmosphere spectra for a consistent spectrophotometric calibration from the optical to the infrared wavelengths The important role of stellar atmosphere spectra for a consistent spectrophotometric calibration from the optical to the infrared wavelengths

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008phst..133a4024d&link_type=abstract

Physica Scripta, Volume 133, Issue , pp. 014024 (2008).

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Scientific paper

We discuss the role of stellar atmosphere models in the spectrophotometric calibration pedigree. It is shown that stellar atmosphere spectra form an essential ingredient for spectrophotometric calibration. Compared with other (infrared) calibration networks currently available, the marcs grid is shown to provide the calibration community with spectral reference energy distributions of higher accuracy improving the spectrophotometric calibration of infrared spectrometers by more than 3%.

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