A new estimate of the local luminosity function of Seyfert 1 nuclei

Details A new estimate of the local luminosity function of Seyfert 1 nuclei A new estimate of the local luminosity function of Seyfert 1 nuclei

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984xue..conf...25c&link_type=abstract

In Max-Planck Inst. für Physik und Astrophysik X-Ray and UV Emission from Active Galactic Nuclei p 25-27 (SEE N85-17790 08-88)

Astronomy and Astrophysics

Astrophysics

Galactic Nuclei, Seyfert Galaxies, Stellar Luminosity, Galactic Radiation, Root-Mean-Square Errors, Stellar Color

Scientific paper

The nuclear magnitudes of all confirmed Seyfert 1 and 1.5 galaxies in the area covered by the first 9 Markarian lists were estimated using the color given method. A comparison with independent estimates obtained by subtracting from the observed flux the expected contribution of an appropriate template galaxy and with the nuclear magnitudes derived for 11 Seyfert 1's on the basis of detailed multicolor surface photometry, suggests that the rms errors are 0.4 mag in the U band and 0.5 mag in the B band.

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