Eddington-limited Accretion in z ~ 2 WISE -selected Hot, Dust-obscured Galaxies

Wu, Jingwen; Jun, Hyunsung D.; Assef, Roberto J.; Tsai, Chao-Wei; Wright, Edward L.; Eisenhardt, Peter R.  M.; Blain, Andrew; Stern, Daniel; Díaz-Santos, Tanio; Denney, Kelly D.; Hayden, Brian T.; Perlmutter, Saul; Aldering, Greg; Boone, Kyle; Fagrelius, Parker

doi:10.3847/1538-4357/aa9ff3

Eddington-limited Accretion in z ~ 2 WISE -selected Hot, Dust-obscured Galaxies

Journal Article · Thu Jan 11 00:00:00 EST 2018 · The Astrophysical Journal (Online)

DOI:https://doi.org/10.3847/1538-4357/aa9ff3· OSTI ID:1544053

^[1]; ^[2]; ^[3]; ^[4]; ^[4]; Eisenhardt, Peter R. M. ^[2]; ^[5]; ^[2]; ^[3]; Denney, Kelly D. ^[6]; ^[7]; Perlmutter, Saul ^[7]; Aldering, Greg ^[7]; ^[7]; ^[7]

Chinese Academy of Sciences (CAS), Beijing (China)
California Inst. of Technology (CalTech), Pasadena, CA (United States)
Universidad Diego Portales, (Chile)
Univ. of California, Los Angles, CA (United States)
Univ. of Leicester (United Kingdom)
The Ohio State Univ., Columbus, OH (United States)
Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)

Hot, dust-obscured galaxies, or "Hot DOGs," are a rare, dusty, hyperluminous galaxy population discovered by the WISE mission. Predominantly at redshifts 2–3, they include the most luminous known galaxies in the universe. Their high luminosities likely come from accretion onto highly obscured supermassive black holes (SMBHs). We have conducted a pilot survey to measure the SMBH masses of five $$z\sim 2$$ Hot DOGs via broad Hα emission lines, using Keck/MOSFIRE and Gemini/FLAMINGOS-2. We detect broad Hα emission in all five Hot DOGs. We find substantial corresponding SMBH masses for these Hot DOGs ($$\sim {10}^{9}\,{M}_{\odot }$$), and their derived Eddington ratios are close to unity. These $$z\sim 2$$ Hot DOGs are the most luminous active galactic nuclei for their BH masses, suggesting that they are accreting at the maximum rates for their BHs. A similar property is found for known $$z\sim 6$$ quasars. Our results are consistent with scenarios in which Hot DOGs represent a transitional, high-accretion phase between obscured and unobscured quasars. Finally, Hot DOGs may mark a special evolutionary stage before the red quasar and optical quasar phases, and they may be present at other cosmic epochs.

View Accepted Manuscript (DOE)

Research Organization:: Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States). National Energy Research Scientific Computing Center (NERSC)

Sponsoring Organization:: USDOE

OSTI ID:: 1544053

Journal Information:: The Astrophysical Journal (Online), Journal Name: The Astrophysical Journal (Online) Journal Issue: 2 Vol. 852; ISSN 1538-4357

Publisher:: Institute of Physics (IOP)Copyright Statement

Country of Publication:: United States

Language:: English

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Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies Kormendy, John; Ho, Luis C. arXiv https://doi.org/10.48550/arxiv.1304.7762	text	January 2013
Narrow-line region gas kinematics of 24,264 optically-selected AGN: the radio connection Mullaney, J. R.; Alexander, D. M.; Fine, S. arXiv https://doi.org/10.48550/arxiv.1305.0263	text	January 2013
Dynamical Versus Stellar Masses in Compact Early-Type Galaxies: Further Evidence for Systematic Variation in the Stellar Initial Mass Function Conroy, Charlie; Dutton, Aaron A.; Graves, Genevieve J. arXiv https://doi.org/10.48550/arxiv.1306.2316	text	January 2013
Physical Properties of Luminous Dust Poor Quasars Jun, Hyunsung David; Im, Myungshin arXiv https://doi.org/10.48550/arxiv.1310.3034	text	January 2013
Similarity of ionized gas nebulae around unobscured and obscured quasars Liu, Guilin; Zakamska, Nadia L.; Greene, Jenny E. arXiv https://doi.org/10.48550/arxiv.1401.0536	text	January 2014
Dusty Star-Forming Galaxies at High Redshift Casey, Caitlin M.; Narayanan, Desika; Cooray, Asantha arXiv https://doi.org/10.48550/arxiv.1402.1456	text	January 2014
Quasar feedback and the origin of radio emission in radio-quiet quasars Zakamska, Nadia L.; Greene, Jenny E. arXiv https://doi.org/10.48550/arxiv.1402.6736	text	January 2014
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Interferometric Follow-Up of WISE Hyper-Luminous Hot, Dust-Obscured Galaxies Wu, Jingwen; Bussmann, R. Shane; Tsai, Chao-Wei arXiv https://doi.org/10.48550/arxiv.1405.1147	text	January 2014
Half of the Most Luminous Quasars May Be Obscured: Investigating the Nature of WISE-Selected Hot, Dust-Obscured Galaxies Assef, Roberto J.; Eisenhardt, Peter R. M.; Stern, Daniel arXiv https://doi.org/10.48550/arxiv.1408.1092	text	January 2014
A Spectroscopic Survey of WISE-selected Obscured Quasars with the Southern African Large Telescope Hainline, Kevin N.; Hickox, Ryan C.; Carroll, Christopher M. arXiv https://doi.org/10.48550/arxiv.1409.4773	text	January 2014
Black hole feedback in the luminous quasar PDS 456 Nardini, E.; Reeves, J. N.; Gofford, J. arXiv https://doi.org/10.48550/arxiv.1502.06636	text	January 2015
An ultra-luminous quasar at z=5.363 with a ten billion solar mass black hole and a Metal-Rich DLA at z~5 Wang, Feige; Wu, Xue-Bing; Fan, Xiaohui arXiv https://doi.org/10.48550/arxiv.1506.01765	text	January 2015
Hot Dust Obscured Galaxies with Excess Blue Light: Dual AGN or Single AGN Under Extreme Conditions? Assef, R. J.; Walton, D. J.; Brightman, M. arXiv https://doi.org/10.48550/arxiv.1511.05155	text	January 2015
Discovery of a 0.42-s pulsar in the ultraluminous X-ray source NGC 7793 P13 Israel, G. L.; Papitto, A.; Esposito, P. arXiv https://doi.org/10.48550/arxiv.1609.06538	text	January 2016
Extremely Red Quasars in BOSS Hamann, Fred; Zakamska, Nadia L.; Ross, Nicholas arXiv https://doi.org/10.48550/arxiv.1609.07241	text	January 2016
An accreting pulsar with extreme properties drives an ultraluminous x-ray source in NGC 5907 Israel, G. L.; Belfiore, A.; Stella, L. arXiv https://doi.org/10.48550/arxiv.1609.07375	text	January 2016
The role of the most luminous, obscured AGN in galaxy assembly at z~2 Farrah, Duncan; Petty, Sara; Connolly, Brian arXiv https://doi.org/10.48550/arxiv.1705.02649	text	January 2017
Caught in the act: a helium-reionizing quasar near the line of sight to Q0302-003 Jakobsen, P.; Jansen, R. A.; Wagner, S. arXiv https://doi.org/10.48550/arxiv.astro-ph/0211035	text	January 2002
FeII/MgII Emission Line Ratio in High Redshift Quasars Dietrich, M.; Hamann, F.; Appenzeller, I. arXiv https://doi.org/10.48550/arxiv.astro-ph/0306584	text	January 2003
Central Masses and Broad-Line Region Sizes of Active Galactic Nuclei. II. A Homogeneous Analysis of a Large Reverberation-Mapping Database Peterson, B. M.; Ferrarese, L.; Gilbert, K. M. arXiv https://doi.org/10.48550/arxiv.astro-ph/0407299	text	January 2004
A Unified, Merger-Driven Model for the Origin of Starbursts, Quasars, the Cosmic X-Ray Background, Supermassive Black Holes and Galaxy Spheroids Hopkins, Philip F.; Hernquist, Lars; Cox, Thomas J. arXiv https://doi.org/10.48550/arxiv.astro-ph/0506398	text	January 2005
Systematic Effects in Measurement of Black Hole Masses by Emission-Line Reverberation of Active Galactic Nuclei: Eddington Ratio and Inclination Collin, Suzy; Kawaguchi, Toshihiro; Peterson, Brad arXiv https://doi.org/10.48550/arxiv.astro-ph/0603460	text	January 2006
Spitzer Mid-Infrared Spectroscopy of Infrared Luminous Galaxies at z~2 I: the Spectra Yan, Lin; Sajina, Anna; Fadda, Dario arXiv https://doi.org/10.48550/arxiv.astro-ph/0612297	text	January 2006
Reverberation Measurements for 17 Quasars and the Size-Mass-Luminosity Relations in Active Galactic Nuclei Kaspi, Shai; Smith, Paul S.; Netzer, Hagai arXiv https://doi.org/10.48550/arxiv.astro-ph/9911476	text	January 1999
The seventh data release of the sloan digital sky survey Abazajian, K. N.; Al, Et; Adelman-McCarthy, J. K. Institute of Physics Publishing https://doi.org/10.5167/uzh-30878	text	January 2009
Heavy X-ray obscuration in the most-luminous galaxies discovered by WISE Vito, Fabio; Brandt, W. N.; Stern, D. Zenodo https://doi.org/10.5281/zenodo.1473601	text	January 2018
The Seventh Data Release of the Sloan Digital Sky Survey Abazajian, Kevork N.; Adelman-McCarthy, Jennifer K.; Agüeros, Marcel Andre Columbia University https://doi.org/10.7916/d8n879qg	text	January 2009

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