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Constraints on the Faint End of the Quasar Luminosity Function at z ∼ 5 in the COSMOS Field

  • Authors: H. Ikeda, T. Nagao, K. Matsuoka, Y. Taniguchi, Y. Shioya, M. Kajisawa, M. Enoki, P. Capak, F. Civano, A. M. Koekemoer, D. Masters, T. Morokuma, M. Salvato, E. Schinnerer, and N. Z. Scoville

Ikeda et al. 2012 The Astrophysical Journal 756 160.

  • Provider: AAS Journals

Caption: Figure 9.

Redshift evolution of the quasar space density. Red, green, blue, magenta, light blue, orange, black, and purple lines are the space density of quasars with M 1450 = −20, −21, −22, −23, −24, −25, −26, and −27, respectively. Filled squares, open circles, filled circle, and open triangles denote the results of different quasar surveys, as described in the upper-left side of the panel (see the main text for details). For comparison, the results of COSMOS and previous surveys are connected by the dashed lines while the results of NDWFS and DLS (Glikman et al. 2011) are connected by the dotted lines.

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