Volume 399, Number 3, March I 2003
|Page(s)||829 - 832|
|Section||Cosmology (including clusters of galaxies)|
|Published online||14 February 2003|
Evidence for the class of the most luminous quasars
IV. Cosmological Malmquist bias and the Λ term
Tuorla Observatory, University of Turku, 21500 Piikkiö, Finland
Corresponding author: firstname.lastname@example.org
Accepted: 3 December 2002
We study if the evidence for the optically luminous subclass of radio quasars (Teerikorpi 2000, 2001), depends on the Friedmann model used, especially on the presence or not of a Λ term. Previously this grouping, with distinct properties, was found at (, ). The cosmological Malmquist bias approach shows that the member candidates, separated by an empty luminosity range from fainter quasars, as well or better appear in the currently favoured flat models with a non-zero Λ. We briefly illustrate the effect of Λ on the Malmquist bias, depending on the steeper volume derivative and longer luminosity distance in Λ models.
Key words: quasars: general / cosmology: observations
© ESO, 2003
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.