Hostname: page-component-586b7cd67f-dlnhk Total loading time: 0 Render date: 2024-11-28T10:10:14.088Z Has data issue: false hasContentIssue false
  • English
  • Français

K-Correction Biases and the Quasar Luminosity Function

Published online by Cambridge University Press:  19 July 2016

A. C. Baker  and
P. C. Hewett
A. C. Baker
Affiliation:
Institute of Astronomy, Madingley Road, Cambridge, CB3 0HA England
P. C. Hewett
Affiliation:
Institute of Astronomy, Madingley Road, Cambridge, CB3 0HA England

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

By characterising the range of quasar UV-optical spectral indices and any correlation with it e.g. luminosity or line parameters, we hope to remove one more bias from the quasar luminosity function (QLF).

Type
Poster contributions: Statistical Studies and Evolution
Information
Symposium - International Astronomical Union , Volume 159: Multi-Wavelength Continuum Emission of AGN , 1994 , pp. 498
Copyright
Copyright © Kluwer 1994