First discoveries of z ∼ 6 quasars with the Kilo-Degree Survey and VISTA Kilo-Degree Infrared Galaxy survey

被引:79
作者
Venemans, B. P. [1 ]
Kleijn, G. A. Verdoes [2 ]
Mwebaze, J. [2 ]
Valentijn, E. A. [2 ]
Banados, E. [1 ]
Decarli, R. [1 ]
de Jong, J. T. A. [3 ]
Findlay, J. R. [4 ]
Kuijken, K. H. [3 ]
La Barbera, F. [5 ]
McFarland, J. P. [2 ]
McMahon, R. G. [6 ,7 ]
Napolitano, N. [5 ]
Sikkema, G. [2 ]
Sutherland, W. J. [8 ]
机构
[1] Max Planck Inst Astron, D-69117 Heidelberg, Germany
[2] Univ Groningen, Kapteyn Astron Inst, NL-9700 AV Groningen, Netherlands
[3] Leiden Univ, Leiden Observ, NL-2300 RA Leiden, Netherlands
[4] Univ Wyoming, Dept Phys & Astron, Laramie, WY 82071 USA
[5] INAF, Astron Observ Capodimonte, I-80131 Naples, Italy
[6] Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England
[7] Univ Cambridge, Kavli Inst Cosmol, Cambridge CB3 0HA, England
[8] Univ London, Sch Math Sci, Astron Unit, London E1 4NS, England
关键词
galaxies: active; quasars: general; cosmology: observations; DIGITAL SKY SURVEY; STAR-FORMATION; Z-SIMILAR-TO-6; QUASARS; HOST GALAXIES; MOLECULAR GAS; BLACK-HOLES; REDSHIFT; SPECTROSCOPY; EVOLUTION; SYSTEM;
D O I
10.1093/mnras/stv1774
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the results of our first year of quasar search in the ongoing ESO public Kilo-Degree Survey (KiDS) and VISTA Kilo-Degree Infrared Galaxy (VIKING) surveys. These surveys are among the deeper wide-field surveys that can be used to uncover large numbers of z similar to 6 quasars. This allows us to probe a more common population of z similar to 6 quasars that is fainter than the well-studied quasars from the main Sloan Digital Sky Survey. From this first set of combined survey catalogues covering similar to 250 deg(2) we selected point sources down to Z(AB) = 22 that had a very red i - Z (i - Z > 2.2) colour. After follow-up imaging and spectroscopy, we discovered four new quasars in the redshift range 5.8 < z < 6.0. The absolute magnitudes at a rest-frame wavelength of 1450 angstrom are between -26.6 < M-1450 < -24.4, confirming that we can find quasars fainter than M*, which at z = 6 has been estimated to be between M* =-25.1 and M* =-27.6. The discovery of four quasars in 250 deg(2) of survey data is consistent with predictions based on the z similar to 6 quasar luminosity function. We discuss various ways to push the candidate selection to fainter magnitudes and we expect to find about 30 new quasars down to an absolute magnitude of M-1450 =-24. Studying this homogeneously selected faint quasar population will be important to gain insight into the onset of the co-evolution of the black holes and their stellar hosts.
引用
收藏
页码:2259 / 2266
页数:8
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