Figure 2 from Constraints on the Faint End of the Quasar Luminosity Function at z ∼ 5 in the COSMOS Field

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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 2.

Reduced spectrum of object No. 11 in Table 1 (upper panel) and typical sky spectrum (lower panel). The dotted lines show the expected wavelengths of quasar emission lines: Lyα λ1216 and C iv λ1549.

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