Home News About Us Contact Contributors Disclaimer Privacy Policy Help FAQ

Quick Search
My eDoc
Session History
Support Wiki
Direct access to
document ID:

          Institute: MPI für Astronomie     Collection: Publikationen_mpia     Display Documents

ID: 660899.0, MPI für Astronomie / Publikationen_mpia
Constraints on the faint end of the quasar luminosity function at z ~ 5 in the COSMOS field
Authors:Ikeda, H.; Nagao, T.; Matsuoka, K.; Taniguchi, Y.; Shioya, Y.; Kajisawa, M.; Enoki, M.; Capak, P.; Civano, F.; Koekemoer, A. M.; Masters, D.; Morokuma, T.; Salvato, M.; Schinnerer, E.; Scoville, N. Z.
Date of Publication (YYYY-MM-DD):2012
Journal Abbrev.:The Astrophysical Journal
Issue / Number:2
Start Page:id. 160
Audience:Not Specified
Abstract / Description:We present the result of our low-luminosity quasar survey in the redshift range of 4.5 <~ z <~ 5.5 in the COSMOS field. Using the COSMOS photometric catalog, we selected 15 quasar candidates with 22 < i' < 24 at z ~ 5 that are ~3 mag fainter than the Sloan Digital Sky Survey quasars in the same redshift range. We obtained optical spectra for 14 of the 15 candidates using FOCAS on the Subaru Telescope and did not identify any low-luminosity type-1 quasars at z ~ 5, while a low-luminosity type-2 quasar at z ~ 5.07 was discovered. In order to constrain the faint end of the quasar luminosity function at z ~ 5, we calculated the 1σ confidence upper limits of the space density of type-1 quasars. As a result, the 1σ confidence upper limits on the quasar space density are Φ < 1.33 × 10-7 Mpc-3 mag-1 for -24.52 < M 1450 < -23.52 and Φ < 2.88 × 10-7 Mpc-3 mag-1 for -23.52 < M 1450 < -22.52. The inferred 1σ confidence upper limits of the space density are then used to provide constraints on the faint-end slope and the break absolute magnitude of the quasar luminosity function at z ~ 5. We find that the quasar space density decreases gradually as a function of redshift at low luminosity (M 1450 ~ -23), being similar to the trend found for quasars with high luminosity (M 1450 < -26). This result is consistent with the so-called downsizing evolution of quasars seen at lower redshifts.
Free Keywords:cosmology: observations; quasars: general; surveys
External Publication Status:published
Document Type:Article
Communicated by:N. N.
Affiliations:MPI für Astronomie
The scope and number of records on eDoc is subject to the collection policies defined by each institute - see "info" button in the collection browse view.