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The Infrared Medium-deep Survey. III. Survey of Luminous Quasars at 4.7 ≤ z ≤ 5.4
Ist Teil von
The Astrophysical journal. Supplement series, 2017-08, Vol.231 (2), p.16
Ort / Verlag
Saskatoon: IOP Publishing
Erscheinungsjahr
2017
Quelle
Free E-Journal (出版社公開部分のみ)
Beschreibungen/Notizen
Abstract
We present the first results of our survey for high-redshift quasars at
. The search for quasars in this redshift range has been known to be challenging due to the limitations of the filter sets used in previous studies. We conducted a quasar survey for two specific redshift ranges, 4.60 ≤
z
≤ 5.40 and 5.50 ≤
z
≤ 6.05, using multi-wavelength data that include observations made with custom-designed filters,
is
and
iz
. Using these filters and a new selection technique, we were able to reduce the fraction of interlopers. Through optical spectroscopy, we confirmed six quasars at 4.7 ≤
z
≤ 5.4 with
that recently were discovered independently by another group. We estimated black hole masses and Eddington ratios of four of these quasars from optical and near-infrared spectra, and found that these quasars are undergoing nearly Eddington-limited accretion that is consistent with the rapid growth of supermassive black holes in luminous quasars at
z
∼ 5.