Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/36170
Title: NuSTAR AND XMM-NEWTON OBSERVATIONS OF LUMINOUS, HEAVILY OBSCURED, WISE-SELECTED QUASARS AT Z similar to 2
Authors: Stern, D.
Lansbury, G. B.
Assef, R. J.
Brandt, W. N.
Alexander, D. M.
Ballantyne, D. R.
Balokovic, M.
Bauer, F. E.
Benford, D.
Blain, Andrew W.
Boggs, S. E.
Bridge, C.
Brightman, M.
Christensen, F. E.
Comastri, A.
Craig, W. W.
Del Moro, A.
Eisenhardt, P. R. M.
Gandhi, P.
Griffith, R. L.
Hailey, C. J.
Harrison, F. A.
Hickox, R. C.
Jarrett, T. H.
Koss, M.
Lake, S.
LaMassa, S. M.
Luo, B.
Tsai, C-W.
Urry, C. M.
Walton, D. J.
Wright, E. L.
Wu, J.
Yan, L.
Zhang, W. W.
First Published: 29-Sep-2014
Publisher: IOP Publishing LTD
Citation: Astrophysical Journal, 2014, 794 (2), 102
Abstract: We report on a NuSTAR and XMM-Newton program that has observed a sample of three extremely luminous, heavily obscured WISE-selected active galactic nuclei (AGNs) at z ~ 2 across a broad X-ray band (0.1 – 79 keV). The parent sample, selected to be faint or undetected in the WISE 3.4 μm (W1) and 4.6 μm (W2) bands but bright at 12 μm (W3) and 22 μm (W4), are extremely rare, with only ~1000 so-called "W1W2-dropouts" across the extragalactic sky. Optical spectroscopy reveals typical redshifts of z ~ 2 for this population, implying rest-frame mid-IR luminosities of νL [Subscript: ν](6 μm) ~ 6 × 10[Superscript: 46] erg s[Superscript: –1] and bolometric luminosities that can exceed L [Subscript: bol] ~ 10[Superscript: 14] L [Subscript: ☉]. The corresponding intrinsic, unobscured hard X-ray luminosities are L(2-10 keV) ~ 4 × 10[Superscript: 45] erg s[Superscript: –1 ] for typical quasar templates. These are among the most AGNs known, though the optical spectra rarely show evidence of a broad-line region and the selection criteria imply heavy obscuration even at rest-frame 1.5 μm. We designed our X-ray observations to obtain robust detections for gas column densities N [Subscript: H] ≤ 10[Superscript: 24] cm[Superscript: –2]. In fact, the sources prove to be fainter than these predictions. Two of the sources were observed by both NuSTAR and XMM-Newton, with neither being detected by NuSTAR (f [Subscript: 3-24 keV] ≲ 10[Superscript: –13 ] erg cm[Superscript: –2] s[Superscript: –1]), and one being faintly detected by XMM-Newton (f [Subscript: 0.5-10] keV ~ 5 × 10[Superscript: –15] erg cm[Superscript: –2] s[Superscript: –1]). A third source was observed only with XMM-Newton, yielding a faint detection (f [Subscript: 0.5-10 keV ]~ 7 × 10[Superscript: –15] erg cm[Superscript: –2] s[Superscript: –1]). The X-ray data imply these sources are either X-ray weak, or are heavily obscured by column densities N [Subscript: H] ≳ 10[Superscript: 24] cm[Superscript: –2]. The combined X-ray and mid-IR analysis seems to favor this second possibility, implying the sources are extremely obscured, consistent with Compton-thick, luminous quasars. The discovery of a significant population of heavily obscured, extremely luminous AGNs would not conform to the standard paradigm of a receding torus, in which more luminous quasars are less likely to be obscured, and instead suggests that an additional source of obscuration is present in these extreme sources.
DOI Link: 10.1088/0004-637X/794/2/102
ISSN: 0004-637X
eISSN: 1538-4357
Links: http://iopscience.iop.org/article/10.1088/0004-637X/794/2/102/
http://hdl.handle.net/2381/36170
Version: Publisher Version
Status: Peer-reviewed
Type: Journal Article
Rights: Copyright © 2014. The American Astronomical Society. All rights reserved. Archived with reference to the Publisher's Copyright Policy available at http://aas.org/publications/aas-copyright-policy
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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