We report the discovery of eight new quasars in one extragalactic field (a five-degree field centered at RA=08(h)58(m)08.2(s), Dec=01 degrees 32'29.7 '') with the Guoshoujing Telescope (LAMOST) commissioning observations made on 2009 December 18. These quasars, with i magnitudes from 16.44 to 19.34 and redshifts from 0.898 to 2.773, were not identified in the SDSS spectroscopic survey, though six of them with redshifts less than 2.5 were selected as quasar targets in SDSS. Except for one source without near-IR Y-band data, seven of these eight new quasars satisfy a newly proposed quasar selection criterion involving both near-IR and optical colors. Two of them were found in the 'redshift desert' for quasars (z from 2.2 t...
The identification of quasars in the redshift range 2.2 < z < 3 is known to be very inefficien...
High-redshift quasars are important tracers of structure and evolution in the early universe. Howeve...
We present the discovery of nine quasars at z similar to 6 identified in the Sloan Digital Sky Surve...
The redshift range from 2.2 to 3 is known as the 'redshift desert' of quasars because quasar...
The redshift range from 2.2 to 3 is known as the 'redshift desert' of quasars because quas...
We present initial results from the first systematic survey of luminous z ~ 5.5 quasars. Quasars at ...
We present a sample of quasars discovered in an area near the Galactic Anti-Center covering 150 degr...
High-redshift quasars are currently the only probes of the growth of supermassive black holes and po...
Quasars with redshifts greater than 4 are rare, and can be used to probe the structure and evolution...
The authors present the discovery of seven quasars at z > 5.7, selected from {approx} 2000 deg{su...
We present initial results from the first systematic survey of luminous z similar to 5.5 quasars. Qu...
We present initial results from the first systematic survey of luminous z ∼ 5.5 quasars. Quasars at ...
The identification of quasars at intermediate redshifts (2.2 < z < 3.5) has been inefficient i...
We present the discovery of eight quasars at z ∼ 6 identified in the Sloan Digital Sky Survey (SDSS)...
We present the discovery of eight quasars at z similar to 6 identified in the Sloan Digital Sky Surv...
The identification of quasars in the redshift range 2.2 < z < 3 is known to be very inefficien...
High-redshift quasars are important tracers of structure and evolution in the early universe. Howeve...
We present the discovery of nine quasars at z similar to 6 identified in the Sloan Digital Sky Surve...
The redshift range from 2.2 to 3 is known as the 'redshift desert' of quasars because quasar...
The redshift range from 2.2 to 3 is known as the 'redshift desert' of quasars because quas...
We present initial results from the first systematic survey of luminous z ~ 5.5 quasars. Quasars at ...
We present a sample of quasars discovered in an area near the Galactic Anti-Center covering 150 degr...
High-redshift quasars are currently the only probes of the growth of supermassive black holes and po...
Quasars with redshifts greater than 4 are rare, and can be used to probe the structure and evolution...
The authors present the discovery of seven quasars at z > 5.7, selected from {approx} 2000 deg{su...
We present initial results from the first systematic survey of luminous z similar to 5.5 quasars. Qu...
We present initial results from the first systematic survey of luminous z ∼ 5.5 quasars. Quasars at ...
The identification of quasars at intermediate redshifts (2.2 < z < 3.5) has been inefficient i...
We present the discovery of eight quasars at z ∼ 6 identified in the Sloan Digital Sky Survey (SDSS)...
We present the discovery of eight quasars at z similar to 6 identified in the Sloan Digital Sky Surv...
The identification of quasars in the redshift range 2.2 < z < 3 is known to be very inefficien...
High-redshift quasars are important tracers of structure and evolution in the early universe. Howeve...
We present the discovery of nine quasars at z similar to 6 identified in the Sloan Digital Sky Surve...