A determination of the K-correction for quasars

Details A determination of the K-correction for quasars A determination of the K-correction for quasars

Jun 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981cha%26a...5..174x&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 5, Issue 2, p. 174-182.

Astronomy and Astrophysics

Astrophysics

Scientific paper

The K-correction is made up of an emission line component and a continuum component. These two components are iteratively determined in this paper from line widths and intensities, redshifts, U,B,V colours and radio spectral indices for 355 quasars. The colors B-V and U-B, corrected for the emission line portion of the K-correction, are plotted against Z, giving 2 mean relations. Eliminating Z between these gives a mean optical continuum, which is then used to calculate the continuum portion of the K-correction.

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