Use of νFν spectral energy distributions for multiwavelength astronomy.

Details Use of νFν spectral energy distributions for multiwavelength astronomy. Use of νFν spectral energy distributions for multiwavelength astronomy.

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997ncimb.112...11g&link_type=abstract

Nuovo Cimento B, Vol. 112B, No. 1, p. 11 - 15

Astronomy and Astrophysics

Astronomy

5

Energy Distribution: Spectra, Spectra: Multiwavelength Observations

Scientific paper

Spectral energy distribution (SED) plots of log(νFν) vs. log(ν) have become popular for multiwavelength astronomy because they give the source power per logarithmic frequency interval and thereby directly show the relative energy output in each frequency band. They also allow easy manipulation and integration of black-body spectra. However, usage can be tricky and misuse is common. This paper derives equations for manipulating SEDs.

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