SDSS QUASARS IN THE WISE PRELIMINARY DATA RELEASE AND QUASAR CANDIDATE SELECTION WITH OPTICAL/INFRARED COLORS
- 1. Department of Astronomy, School of Physics, Peking University, Beijing 100871 (China)
- 2. National Astronomical Observatories, Chinese Academy of Sciences, Datun Road A20, Beijing 100012 (China)
Description
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 less than 0.2, from 70.3% to 77.2%. We also obtain the samples of WISE-detected normal and late-type stars with SDSS spectroscopy, and present a criterion in the z – W1 versus g – z color-color diagram, z – W1 > 0.66(g – z) + 2.01, to separate quasars from stars. With this criterion we can recover 98.6% of 3089 radio-detected SDSS-WISE quasars with redshifts less than four and overcome the difficulty in selecting quasars with redshifts between 2.2 and 3 from SDSS photometric data alone. We also suggest another criterion involving the WISE color only, W1 – W2 > 0.57, to efficiently separate quasars with redshifts less than 3.2 from stars. In addition, we compile a catalog of 5614 SDSS quasars detected by both WISE and UKIDSS surveys and present their color-redshift relations in the optical and infrared bands. By using the SDSS ugriz, UKIDSS, YJHK, and WISE W1- and W2-band photometric data, we can efficiently select quasar candidates and increase the photometric redshift reliability up to 87.0%. We discuss the implications of our results on the future quasar surveys. An updated SDSS-WISE quasar catalog consisting of 101,853 quasars with the recently released WISE all-sky data is also provided.
Availability note (English)
Available from http://dx.doi.org/10.1088/0004-6256/144/2/49Additional details
Identifiers
Publishing Information
- Journal Title
- Astronomical Journal (New York, N.Y. Online)
- Journal Volume
- 144
- Journal Issue
- 2
- Journal Page Range
- [11 p.]
- ISSN
- 1538-3881
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 43123283
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ASTRONOMY; ASTROPHYSICS; CATALOGS; COLOR; DETECTION; DIAGRAMS; EMISSION SPECTROSCOPY; GALAXIES; INFRARED SURVEYS; PHOTOMETRY; QUASARS; RED SHIFT; RELIABILITY; STARS
- Descriptors DEC
- COSMIC RADIO SOURCES; DOCUMENT TYPES; GEOLOGIC SURVEYS; GEOPHYSICAL SURVEYS; INFORMATION; OPTICAL PROPERTIES; ORGANOLEPTIC PROPERTIES; PHYSICAL PROPERTIES; PHYSICS; SPECTROSCOPY