The Infrared Medium-deep Survey. VI. Discovery of Faint Quasars at with a Medium-band-based Approach
arXiv:1811.08606 · doi:10.3847/1538-4357/aaf387
Abstract
The faint quasars with mag are known to hold the key to the determination of the ultraviolet emissivity for the cosmic re-ionization. But only a few have been identified so far because of the limitations on the survey data. Here, we present the first results of the faint quasar survey with the Infrared Medium-deep Survey (IMS), which covers deg areas in -band to the depths of mag. To improve selection methods, the medium-band follow-up imaging has been carried out using the SED camera for QUasars in Early uNiverse (SQUEAN) on the Otto Struve 2.1 m Telescope. The optical spectra of the candidates were obtained with 8-m class telescopes. We newly discovered 10 quasars with at , among which three have been missed in a previous survey using the same optical data over the same area, implying the necessity for improvements in high redshift faint quasars selection. We derived photometric redshifts from the medium-band data, and find that they have high accuracies of . The medium-band-based approach allows us to rule out many of the interlopers that contaminate of the broad-band-selected quasar candidates. These results suggest that the medium-band-based approach is a powerful way to identify quasars and measure their redshifts at high accuracy (1-2 %). It is also a cost-effective way to understand the contribution of quasars to the cosmic re-ionization history.
arXiv comment24 pages, 9 figures, 6 tables. Accepted for publication in ApJ
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