Issue |
A&A
Volume 589, May 2016
|
|
---|---|---|
Article Number | C2 | |
Number of page(s) | 3 | |
Section | Cosmology (including clusters of galaxies) | |
DOI | https://doi.org/10.1051/0004-6361/201527392e | |
Published online | 11 April 2016 |
The extended Baryon Oscillation Spectroscopic Survey: Variability selection and quasar luminosity function (Corrigendum)
1
CEA, Centre de Saclay,
Irfu/SPP,
91 191
Gif-sur-Yvette,
France
e-mail:
nathalie.palanque-delabrouille@cea.fr
2
INAF−Osservatorio
Astronomico di Trieste, via G. B. Tiepolo 11, 34131
Trieste,
Italy
3
UPMC-CNRS, UMR7095, Institut d’Astrophysique de
Paris, 75014
Paris,
France
4
Department of Physics and Astronomy, University of
Utah, Salt Lake City,
UT
84112,
USA
5
Steward Observatory, University of Arizona,
933 North Cherry Avenue,
Tucson, AZ
85 721,
USA
6
Department of Physics and Astronomy, University of
Wyoming, Laramie,
WY
82 071,
USA
7
Department of Astronomy and Space Science, Sejong
University, 143-747
Seoul,
Korea
8
Lawrence Berkeley National Laboratory,
1 Cyclotron Road, Berkeley, CA
94 720,
USA
9
Department of Astronomy and Astrophysics, 525 Davey Laboratory,
The Pennsylvania State University, University Park, PA
16 802,
USA
10
Institute for Gravitation and the Cosmos, The Pennsylvania State
University, University
Park, PA
16802,
USA
11
Instituto de Astrofisica de Canarias (IAC),
38200, La Laguna, Tenerife, Spain
12
Universidad de La Laguna (ULL), Dept. Astrofisica, 38206,
La Laguna, Tenerife,
Spain
13
Center for Cosmology and Particle Physics, New York
University, New York,
NY
10 003,
USA
Key words: quasars: general / large-scale structure of Universe / surveys / errata, addenda
An error occurred in Tables 6 and 7 during the production process.
The correct tables are published below.
Predicted differential quasar counts over 15.5 <g< 25 and 0 <z< 6 for a survey covering 10 000 deg2, based on our best-fit PLE or PLE+LEDE luminosity function model.
Predicted differential quasar counts over 15.5 <r< 24 and 0 <z< 6 for a survey covering 10 000 deg2, based on our best-fit PLE or PLE+LEDE luminosity function model.
© ESO, 2016
All Tables
Predicted differential quasar counts over 15.5 <g< 25 and 0 <z< 6 for a survey covering 10 000 deg2, based on our best-fit PLE or PLE+LEDE luminosity function model.
Predicted differential quasar counts over 15.5 <r< 24 and 0 <z< 6 for a survey covering 10 000 deg2, based on our best-fit PLE or PLE+LEDE luminosity function model.
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