Abstract
We present a determination of the optical/UV AGN luminosity function and its evolution, based on a large sample of faint (R < 24) QSOs identified in the COMBO-17 survey. Using multi-band photometry in 17 filters within 350 nm < λobs < 930 nm, we could simultaneously determine photometric redshifts with an accuracy of σ z ≃ 0.03 and obtain spectral energy distributions. We select a sample covering the redshift range across 1.2 < z < 4.8. Even at z ≃ 3, the sample reaches below luminosities corresponding to M B = –23, conventionally employed to distinguish between Seyfert galaxies and quasars.
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Wolf, C., Wisotzki, L., Borch, A., Dye, S., Kleinheinrich, M., Meisenheimer, K. The Luminosity Function of AGN at z ~ 5 ...1. In: Renzini, A., Bender, R. (eds) Multiwavelength Mapping of Galaxy Formation and Evolution. ESO Astrophysics Symposia. Springer, Berlin, Heidelberg. https://doi.org/10.1007/10995020_115
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DOI: https://doi.org/10.1007/10995020_115
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Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-540-25665-6
Online ISBN: 978-3-540-31641-1
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