A very bright i=16.44 quasar in the `redshift desert' discovered by LAMOST

TL;DR

This paper reports the discovery of a very bright quasar at redshift 2.427 in the 'redshift desert', demonstrating the effectiveness of near-IR and optical color criteria in identifying quasars missed by traditional surveys, and highlights its significance for understanding quasar evolution.

Contribution

The study introduces a new selection criterion combining near-IR and optical colors to find quasars in the redshift desert, leading to the discovery of the brightest quasar in that range.

Findings

Discovered a bright quasar with i=16.44 at z=2.427.

Derived a supermassive black hole mass of up to 3.9×10^10 M_sun.

Confirmed the effectiveness of near-IR and optical color criteria for quasar detection.

Abstract

The redshift range from 2.2 to 3, is known as the 'redshift desert' of quasars because quasars with redshift in this range have similar optical colors as normal stars and are thus difficult to be found in optical sky surveys. A quasar candidate, SDSS J085543.40-001517.7, which was selected by a recently proposed criterion involving near-IR $Y-K$ and optical $g-z$ colors, was identified spectroscopically as a new quasar with redshift of 2.427 by the LAMOST commissioning observation in December 2009 and confirmed by the observation made with the NAOC/Xinglong 2.16m telescope in March 2010. This quasar was not targeted in the SDSS spectroscopic survey because it locates in the stellar locus of the optical color-color diagrams, while it is clearly separated from stars in the $Y-K$ vs. $g-z$ diagram. Comparing with other SDSS quasars we found this new quasar with $i$ magnitude of 16.44 is apparently the brightest one in the redshift range from 2.3 to 2.7. From the spectral properties we derived its central black hole mass as $(1.4\sim3.9) \times 10^{10} M_\odot$ and the bolometric luminosity as $3.7\times 10^{48}$ \ergs, which indicates that this new quasar is intrinsically very bright and belongs to the most luminous quasars in the universe. Our identification supports that quasars in the redshift desert can be found by the quasar selection criterion involving the near-IR colors. More missing quasars are expected to be recovered by the future LAMOST spectroscopic surveys, which is important to the study of the cosmological evolution of quasars at redshift higher than 2.2.