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WISE detections of known QSOs at redshifts greater than six

Blain, Andrew W. and Assef, Roberto and Stern, Daniel and Tsai, Chao-Wei and Eisenhardt, Peter and Bridge, Carrie and Benford, Dominic and Jarrett, Tom and Cutri, Roc and Petty, Sara and Wu, Jingwen and Wright, Edward L. (2013) WISE detections of known QSOs at redshifts greater than six. Astrophysical Journal, 778 (2). Art. No. 113. ISSN 0004-637X.

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We present WISE All-Sky mid-infrared (IR) survey detections of 55% (17/31) of the known QSOs at z > 6 from a range of surveys: the SDSS, the CFHT-LS, FIRST, Spitzer, and UKIDSS. The WISE catalog thus provides a substantial increase in the quantity of IR data available for these sources: 17 are detected in the WISE W1 (3.4 μm) band, 16 in W2 (4.6 μm), 3 in W3 (12 μm), and 0 in W4 (22 μm). This is particularly important with Spitzer in its warm-mission phase and no faint follow-up capability at wavelengths longward of 5 μm until the launch of James Webb Space Telescope (JWST). WISE thus provides a useful tool for understanding QSOs found in forthcoming large-area optical/IR sky surveys using PanSTARRS, SkyMapper, VISTA, DES, and LSST. The rest-UV properties of the WISE-detected and the WISE-non-detected samples differ: the detections have brighter i/z-band magnitudes and redder rest-UV colors. This suggests that a more aggressive hunt for very high redshift QSOs by combining WISE W1 and W2 data with red, observed optical colors could be effective at least for a subset of dusty candidate QSOs. Stacking the WISE images of the WISE-non-detected QSOs indicates that they are, on average, significantly fainter than the WISE-detected examples, and are thus not narrowly missing detection in the WISE catalog. The WISE catalog detection of three of our sample in the W3 band indicates that their mid-IR flux can be detected individually, although there is no stacked W3 detection of sources detected in W1 but not W3. Stacking analyses of WISE data for large active galactic nucleus samples will be a useful tool, and high-redshift QSOs of all types will be easy targets for JWST.

Item Type:Article
Related URLs:
URLURL TypeDescription Paper
Blain, Andrew W.0000-0001-7489-5167
Assef, Roberto0000-0002-9508-3667
Stern, Daniel0000-0003-2686-9241
Tsai, Chao-Wei0000-0002-9390-9672
Benford, Dominic0000-0002-9884-4206
Jarrett, Tom0000-0002-4939-734X
Cutri, Roc0000-0002-0077-2305
Petty, Sara0000-0003-0624-3276
Wu, Jingwen0000-0001-7808-3756
Wright, Edward L.0000-0001-5058-1593
Additional Information:© 2013 American Astronomical Society. Received 2012 August 15; accepted 2013 September 25; published 2013 November 11. We thank the anonymous referee for a careful reading and helpful suggestions. This publication makes use of data products from the Wide-field Infrared Survey Explorer (WISE). WISE is a joint project of the University of California, Los Angeles, and the Jet Propulsion Laboratory/California Institute of Technology, funded by the National Aeronautics and Space Administration. This research has made use of both the NASA/IPAC Infrared Science Archive (IRSA) and the NASA/IPAC Extragalactic Database (NED), which are operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. R.J.A. was supported by an appointment to the NASA Postdoctoral Program at the Jet Propulsion Laboratory, administered by Oak Ridge Associated Universities through a contract with NASA. Facility: WISE
Group:Infrared Processing and Analysis Center (IPAC)
Funding AgencyGrant Number
NASA Postdoctoral ProgramUNSPECIFIED
Subject Keywords: galaxies: active; galaxies: evolution; infrared: galaxies; quasars: general
Issue or Number:2
Record Number:CaltechAUTHORS:20140106-094902432
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Official Citation:WISE Detections of Known QSOs at Redshifts Greater than Six Andrew W. Blain et al. 2013 ApJ 778 113
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:43219
Deposited By: Ruth Sustaita
Deposited On:06 Jan 2014 18:07
Last Modified:09 Dec 2019 21:29

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