The mid-IR-and X-ray-selected QSO luminosity function

R. J. Assef, C. S. Kochanek, M. L N Ashby, M. Brodwin, M. J I Brown, R. Cool, W. Forman, A. H. Gonzalez, R. C. Hickox, Buell Tomasson Jannuzi, C. Jones, E. Le Floc'h, J. Moustakas, S. S. Murray, D. Stern

Research output: Contribution to journalArticle

20 Citations (Scopus)

Abstract

We present the J-band luminosity function (LF) of 1838 mid-infrared and X-ray-selected active galactic nuclei (AGNs) in the redshift range 0 < z < 5.85. These LFs are constructed by combining the deep multi-wavelength broadband observations from the UV to the mid-IR of the NDWFS Bootes field with the X-ray observations of the XBootes survey and the spectroscopic observations of the same field by AGES. Our sample is primarily composed of IRAC-selected AGNs, targeted using modifications of the Stern et al. criteria, complemented by MIPS 24 μm and X-ray-selected AGNs to alleviate the biases of IRAC mid-IR selection against z ∼ 4.5 quasars and AGNs faint with respect to their hosts. This sample provides an accurate link between low-and high-redshift AGN LFs and does not suffer from the usual incompleteness of optical samples at z ∼ 3. We use a set of low-resolution spectral energy distribution templates for AGNs and galaxies presented in a previous paper by Assef et al. to model the selection function of these sources and apply host and reddening corrections. We find that the space density of the brightest quasars strongly decreases from z = 3 to z = 0, while the space density of faint quasars is at least flat, and possibly increasing, over the same redshift range. At z > 3, we observe a decrease in the space density of quasars of all brightnesses. We model the LF by a double power law and find that its evolution cannot be described by either pure luminosity or pure density evolution, but must be a combination of both. We used the bright-end slope determined by Croom et al. (2QZ) as a prior to fit the data in order to minimize the effects of our small survey area. The bright-end power-law index of our best-fit model remains consistent with the prior, while the best-fit faint-end index is consistent with the low-redshift measurements based on the 2QZ and 2SLAQ surveys. Our best-fit model generally agrees with the number of bright quasars predicted by other LFs at all redshifts. If we construct the QSO luminosity function using only the IRAC-selected AGNs, we find that the biases inherent to this selection method significantly modify the behavior of the characteristic density Φ*(z) only for z < 1 and have no significant impact upon the characteristic magnitude M*,J(z).

Original languageEnglish (US)
JournalAstrophysical Journal
Volume728
Issue number1
DOIs
StatePublished - Feb 10 2011
Externally publishedYes

Fingerprint

quasars
luminosity
active galactic nuclei
power law
x rays
space density
brightness
slopes
index

Keywords

  • Galaxies: active
  • Galaxies: distances and redshifts
  • Galaxies: luminosity function, mass function
  • Quasars: general

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

Assef, R. J., Kochanek, C. S., Ashby, M. L. N., Brodwin, M., Brown, M. J. I., Cool, R., ... Stern, D. (2011). The mid-IR-and X-ray-selected QSO luminosity function. Astrophysical Journal, 728(1). https://doi.org/10.1088/0004-637X/728/1/56

The mid-IR-and X-ray-selected QSO luminosity function. / Assef, R. J.; Kochanek, C. S.; Ashby, M. L N; Brodwin, M.; Brown, M. J I; Cool, R.; Forman, W.; Gonzalez, A. H.; Hickox, R. C.; Jannuzi, Buell Tomasson; Jones, C.; Le Floc'h, E.; Moustakas, J.; Murray, S. S.; Stern, D.

In: Astrophysical Journal, Vol. 728, No. 1, 10.02.2011.

Research output: Contribution to journalArticle

Assef, RJ, Kochanek, CS, Ashby, MLN, Brodwin, M, Brown, MJI, Cool, R, Forman, W, Gonzalez, AH, Hickox, RC, Jannuzi, BT, Jones, C, Le Floc'h, E, Moustakas, J, Murray, SS & Stern, D 2011, 'The mid-IR-and X-ray-selected QSO luminosity function', Astrophysical Journal, vol. 728, no. 1. https://doi.org/10.1088/0004-637X/728/1/56
Assef RJ, Kochanek CS, Ashby MLN, Brodwin M, Brown MJI, Cool R et al. The mid-IR-and X-ray-selected QSO luminosity function. Astrophysical Journal. 2011 Feb 10;728(1). https://doi.org/10.1088/0004-637X/728/1/56
Assef, R. J. ; Kochanek, C. S. ; Ashby, M. L N ; Brodwin, M. ; Brown, M. J I ; Cool, R. ; Forman, W. ; Gonzalez, A. H. ; Hickox, R. C. ; Jannuzi, Buell Tomasson ; Jones, C. ; Le Floc'h, E. ; Moustakas, J. ; Murray, S. S. ; Stern, D. / The mid-IR-and X-ray-selected QSO luminosity function. In: Astrophysical Journal. 2011 ; Vol. 728, No. 1.
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AU - Ashby, M. L N

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AU - Brown, M. J I

AU - Cool, R.

AU - Forman, W.

AU - Gonzalez, A. H.

AU - Hickox, R. C.

AU - Jannuzi, Buell Tomasson

AU - Jones, C.

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AU - Moustakas, J.

AU - Murray, S. S.

AU - Stern, D.

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N2 - We present the J-band luminosity function (LF) of 1838 mid-infrared and X-ray-selected active galactic nuclei (AGNs) in the redshift range 0 < z < 5.85. These LFs are constructed by combining the deep multi-wavelength broadband observations from the UV to the mid-IR of the NDWFS Bootes field with the X-ray observations of the XBootes survey and the spectroscopic observations of the same field by AGES. Our sample is primarily composed of IRAC-selected AGNs, targeted using modifications of the Stern et al. criteria, complemented by MIPS 24 μm and X-ray-selected AGNs to alleviate the biases of IRAC mid-IR selection against z ∼ 4.5 quasars and AGNs faint with respect to their hosts. This sample provides an accurate link between low-and high-redshift AGN LFs and does not suffer from the usual incompleteness of optical samples at z ∼ 3. We use a set of low-resolution spectral energy distribution templates for AGNs and galaxies presented in a previous paper by Assef et al. to model the selection function of these sources and apply host and reddening corrections. We find that the space density of the brightest quasars strongly decreases from z = 3 to z = 0, while the space density of faint quasars is at least flat, and possibly increasing, over the same redshift range. At z > 3, we observe a decrease in the space density of quasars of all brightnesses. We model the LF by a double power law and find that its evolution cannot be described by either pure luminosity or pure density evolution, but must be a combination of both. We used the bright-end slope determined by Croom et al. (2QZ) as a prior to fit the data in order to minimize the effects of our small survey area. The bright-end power-law index of our best-fit model remains consistent with the prior, while the best-fit faint-end index is consistent with the low-redshift measurements based on the 2QZ and 2SLAQ surveys. Our best-fit model generally agrees with the number of bright quasars predicted by other LFs at all redshifts. If we construct the QSO luminosity function using only the IRAC-selected AGNs, we find that the biases inherent to this selection method significantly modify the behavior of the characteristic density Φ*(z) only for z < 1 and have no significant impact upon the characteristic magnitude M*,J(z).

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KW - Galaxies: distances and redshifts

KW - Galaxies: luminosity function, mass function

KW - Quasars: general

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