The UVX quasar optical luminosity function and its evolution
The recently-finished Edinburgh UVX quasar survey at B < 18 is used together with other complete samples to estimate the shape and evolution of the optical luminosity function in the redshift range 0.3 < z < 2.2. There is a significantly higher space density of quasars at high l...
Main Authors: | Goldschmidt, P, Miller, L |
---|---|
Formato: | Journal article |
Idioma: | English |
Publicado: |
1997
|
Títulos similares
-
Quasar Luminosity Function at z = 7
por: Yoshiki Matsuoka, et al.
Publicado: (2023-01-01) -
Search for dark sector by repurposing the UVX Brazilian synchrotron
por: L. Duarte, et al.
Publicado: (2023-06-01) -
Reverberation Mapping of High-Luminosity Quasars
por: Shai Kaspi, et al.
Publicado: (2017-10-01) -
PERIODICITY OF LUMINOSITY OF QUASARS AND GALAXIES AT COSMOLOGICAL SCALE
por: A. P. Miroshnichenko
Publicado: (2017-04-01) -
A Left and Right Truncated Schechter Luminosity Function for Quasars
por: Lorenzo Zaninetti
Publicado: (2017-05-01)