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Evidence for the thermal Sunyaev-Zel'dovich effect associated with quasar feedback

Title: Evidence for the thermal Sunyaev-Zel'dovich effect associated with quasar feedback.
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Name(s): Crichton, Devin, author
Gralla, Megan B., author
Hall, Kirsten, author
Marriage, Tobias A., author
Zakamska, Nadia L., author
Battaglia, Nick, author
Bond, J. Richard, author
Devlin, Mark J., author
Hill, J. Colin, author
Hilton, Matt, author
Hincks, Adam D., author
Huffenberger, Kevin M., author
Hughes, John P., author
Kosowsky, Arthur, author
Moodley, Kavilan, author
Niemack, Michael D., author
Page, Lyman A., author
Partridge, Bruce, author
Sievers, Jonathan L., author
Sifon, Cristobal, author
Staggs, Suzanne T., author
Viero, Marco P., author
Wollack, Edward J., author
Type of Resource: text
Genre: Text
Date Issued: 2016-05-11
Physical Form: computer
online resource
Extent: 1 online resource
Language(s): English
Abstract/Description: Using a radio-quiet subsample of the Sloan Digital Sky Survey spectroscopic quasar catalogue, spanning redshifts 0.5-3.5, we derive the mean millimetre and far-infrared quasar spectral energy distributions (SEDs) via a stacking analysis of Atacama Cosmology Telescope and Herschel-Spectral and Photometric Imaging REceiver data. We constrain the form of the far-infrared emission and find 3 sigma-4 sigma evidence for the thermal Sunyaev-Zel'dovich (SZ) effect, characteristic of a hot ionized gas component with thermal energy (6.2 +/- 1.7) x 10(60) erg. This amount of thermal energy is greater than expected assuming only hot gas in virial equilibrium with the dark matter haloes of (1-5) x 10(12) h(-1) M-circle dot that these systems are expected to occupy, though the highest quasar mass estimates found in the literature could explain a large fraction of this energy. Our measurements are consistent with quasars depositing up to (14.5 +/- 3.3) per cent of their radiative energy into their circumgalactic environment if their typical period of quasar activity is tau(8) x 10(8) yr. For high quasar host masses, similar to 10(13) h(-1) M-circle dot this percentage will be reduced. Furthermore, the uncertainty on this percentage is only statistical and additional systematic uncertainties enter at the 40 per cent level. The SEDs are dust dominated in all bands and we consider various models for dust emission. While sufficiently complex dust models can obviate the SZ effect, the SZ interpretation remains favoured at the 3 sigma-4 sigma level for most models.
Identifier: FSU_libsubv1_wos_000374569600027 (IID), 10.1093/mnras/stw344 (DOI)
Keywords: absorption-line quasars, active galactic nuclei, atacama cosmology telescope, digital-sky-survey, extreme gas kinematics, galaxies: active, intergalactic medium, luminous obscured quasars, quasars: general, radio-quiet quasars, similar-to 1.5, spectral energy-distributions, supermassive black-holes
Publication Note: The publisher’s version of record is available at http://www.dx.doi.org/10.1093/mnras/stw344
Persistent Link to This Record: http://purl.flvc.org/fsu/fd/FSU_libsubv1_wos_000374569600027
Owner Institution: FSU
Is Part Of: Monthly Notices of the Royal Astronomical Society.
0035-8711
Issue: iss. 2, vol. 458

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Crichton, D., Gralla, M. B., Hall, K., Marriage, T. A., Zakamska, N. L., Battaglia, N., … Wollack, E. J. (2016). Evidence for the thermal Sunyaev-Zel'dovich effect associated with quasar feedback. Monthly Notices Of The Royal Astronomical Society. Retrieved from http://purl.flvc.org/fsu/fd/FSU_libsubv1_wos_000374569600027