We present a catalog of 37,842 quasars in the Sloan Digital Sky Survey (SDSS) Data Release 7, which have counterparts within 6 '' in the Wide-field Infrared Survey Explorer (WISE) Preliminary Data Release. The overall WISE detection rate of the SDSS quasars is 86.7%, and it decreases to less than 50.0% when the quasar magnitude is fainter than i = 20.5. We derive the median color-redshift relations based on this SDSS-WISE quasar sample and apply them to estimate the photometric redshifts of the SDSS-WISE quasars. We find that by adding the WISE W1- and W2-band data to the SDSS photometry we can increase the photometric redshift reliability, defined as the percentage of sources with photometric and spectroscopic redshift difference...
The identification of quasars in the redshift range 2.2 < z < 3 is known to be very inefficient beca...
The identification of quasars in the redshift range 2.2 < z < 3 is known to be very inefficient beca...
With a recently constructed composite quasar spectrum and the chi(2) minimization technique, we desc...
We present a sample of 8498 quasars with both Sloan Digital Sky Survey (SDSS) ugriz optical and Unit...
High-redshift quasars are important tracers of structure and evolution in the early universe. Howeve...
The identification of quasars at intermediate redshifts (2.2 < z < 3.5) has been inefficient i...
High-redshift quasars are important tracers of structure and evolution in the early universe. Howeve...
Studies of the most luminous quasars at high redshift directly probe the evolution of the most massi...
We present a new algorithm to estimate quasar photometric redshifts (photo-zs), by considering the a...
Abstract We present a new algorithm to estimate quasar photometric redshifts (photo-zs), by consider...
The Sloan Digital Sky Survey has obtained images in five broad-band colors for several hundred squar...
We present a new algorithm to estimate quasar photometric redshifts (photo-zs), by considering the a...
The identification of quasars in the redshift range 2.2 < z < 3 is known to be very inefficien...
We present a catalog of 100,563 unresolved, UV-excess (UVX) quasar candidates to g 21 from 2099 deg...
With a recently constructed composite quasar spectrum and the \chi^2 minimization technique, we demo...
The identification of quasars in the redshift range 2.2 < z < 3 is known to be very inefficient beca...
The identification of quasars in the redshift range 2.2 < z < 3 is known to be very inefficient beca...
With a recently constructed composite quasar spectrum and the chi(2) minimization technique, we desc...
We present a sample of 8498 quasars with both Sloan Digital Sky Survey (SDSS) ugriz optical and Unit...
High-redshift quasars are important tracers of structure and evolution in the early universe. Howeve...
The identification of quasars at intermediate redshifts (2.2 < z < 3.5) has been inefficient i...
High-redshift quasars are important tracers of structure and evolution in the early universe. Howeve...
Studies of the most luminous quasars at high redshift directly probe the evolution of the most massi...
We present a new algorithm to estimate quasar photometric redshifts (photo-zs), by considering the a...
Abstract We present a new algorithm to estimate quasar photometric redshifts (photo-zs), by consider...
The Sloan Digital Sky Survey has obtained images in five broad-band colors for several hundred squar...
We present a new algorithm to estimate quasar photometric redshifts (photo-zs), by considering the a...
The identification of quasars in the redshift range 2.2 < z < 3 is known to be very inefficien...
We present a catalog of 100,563 unresolved, UV-excess (UVX) quasar candidates to g 21 from 2099 deg...
With a recently constructed composite quasar spectrum and the \chi^2 minimization technique, we demo...
The identification of quasars in the redshift range 2.2 < z < 3 is known to be very inefficient beca...
The identification of quasars in the redshift range 2.2 < z < 3 is known to be very inefficient beca...
With a recently constructed composite quasar spectrum and the chi(2) minimization technique, we desc...