A significant population of very luminous dust-obscured galaxies at redshift z ∼ 2

Arjun Dey, B. T. Soifer, Vandana Desai, Kate Brand, Emeric Le Floc'h, Michael J I Brown, Buell Tomasson Jannuzi, Lee Armus, Shane Bussmann, Mark Brodwin, Chao Bian, Peter Eisenhardt, Sarah J. Higdon, Daniel Weedman, S. P. Willner

Research output: Contribution to journalArticle

209 Citations (Scopus)

Abstract

The Spitzer Space Telescope has revealed a significant population of high-redshift (z ∼ 2) dust-obscured galaxies with large mid-infrared to ultraviolet luminosity ratios. Due to their optical faintness, these galaxies have been previously missed in traditional optical studies of the distant universe. We present a simple method for selecting this high-redshift population based solely on the ratio of the observed mid-infrared 24 μm to optical R-band flux density. We apply this method to observations of the ≈8.6 deg2 NOAO Deep Wide-Field Survey Bootes field, and uncover ≈2600 dust-obscured galaxy candidates [i.e., 0.089 arcmin-2) with 24 μm flux densities F24 μm ≥ 0.3 mJy and (R - [24]) > 14 (i.e., Fν(24 μm)/Fν(R) ≳ 1000]. These galaxies have no counterparts in the local universe. They represent 7% ± 0.6% of the 24 μm source population at F24 μm ≥ 1 mJy but increase to ≈13% ± 1% of the population at ≈0.3 mJy. These galaxies exhibit evidence of both star formation and AGN activity, with the brighter 24 μm sources being more AGN-dominated. We have measured spectroscopic redshifts for 86 of these galaxies, and find a broad redshift distribution centered at z̄ ≈ 1.99 ± 0.05. The space density of this population is ⊃DOG(F24μm ≥ 0.3 mJy) = (2.82 ± 0.05) × 10-5h703 Mpc-3, similar to that of bright submillimeter-selected galaxies at comparable redshifts. These redshifts imply large luminosities, with median νLν(8 μm) ≈ 4 × 1011 L. The infrared luminosity density contributed by this relatively rare dust-obscured galaxy population is log(IRLD) ≈8.23-0.30+0.18. This is ≈60 -15+40% of that contributed by z ∼ 2 ultraluminous infrared galaxies (ULIRGs, with LIR > 1012 L ); our simple selection thus identifies a significant fraction of z ∼ 2 ULIRGs. This IRLD is ≈26% ± 14% of the total contributed by all z ∼ 2 galaxies. We suggest that these dust-obscured galaxies are the progenitors of luminous (∼4L*) present-day galaxies, seen undergoing an extremely luminous, short-lived phase of both bulge and black hole growth. They may represent a brief evolutionary phase between submillimeter-selected galaxies and less obscured quasars or galaxies.

Original languageEnglish (US)
Pages (from-to)943-956
Number of pages14
JournalAstrophysical Journal
Volume677
Issue number2
DOIs
StatePublished - Apr 20 2008
Externally publishedYes

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dust
galaxies
field survey
luminosity
flux density
universe
Space Infrared Telescope Facility
space density
method
quasars
star formation

Keywords

  • Galaxies: formation
  • Galaxies: high-redshift
  • Galaxies: starburst

ASJC Scopus subject areas

  • Space and Planetary Science

Cite this

Dey, A., Soifer, B. T., Desai, V., Brand, K., Le Floc'h, E., Brown, M. J. I., ... Willner, S. P. (2008). A significant population of very luminous dust-obscured galaxies at redshift z ∼ 2. Astrophysical Journal, 677(2), 943-956. https://doi.org/10.1086/529516

A significant population of very luminous dust-obscured galaxies at redshift z ∼ 2. / Dey, Arjun; Soifer, B. T.; Desai, Vandana; Brand, Kate; Le Floc'h, Emeric; Brown, Michael J I; Jannuzi, Buell Tomasson; Armus, Lee; Bussmann, Shane; Brodwin, Mark; Bian, Chao; Eisenhardt, Peter; Higdon, Sarah J.; Weedman, Daniel; Willner, S. P.

In: Astrophysical Journal, Vol. 677, No. 2, 20.04.2008, p. 943-956.

Research output: Contribution to journalArticle

Dey, A, Soifer, BT, Desai, V, Brand, K, Le Floc'h, E, Brown, MJI, Jannuzi, BT, Armus, L, Bussmann, S, Brodwin, M, Bian, C, Eisenhardt, P, Higdon, SJ, Weedman, D & Willner, SP 2008, 'A significant population of very luminous dust-obscured galaxies at redshift z ∼ 2', Astrophysical Journal, vol. 677, no. 2, pp. 943-956. https://doi.org/10.1086/529516
Dey A, Soifer BT, Desai V, Brand K, Le Floc'h E, Brown MJI et al. A significant population of very luminous dust-obscured galaxies at redshift z ∼ 2. Astrophysical Journal. 2008 Apr 20;677(2):943-956. https://doi.org/10.1086/529516
Dey, Arjun ; Soifer, B. T. ; Desai, Vandana ; Brand, Kate ; Le Floc'h, Emeric ; Brown, Michael J I ; Jannuzi, Buell Tomasson ; Armus, Lee ; Bussmann, Shane ; Brodwin, Mark ; Bian, Chao ; Eisenhardt, Peter ; Higdon, Sarah J. ; Weedman, Daniel ; Willner, S. P. / A significant population of very luminous dust-obscured galaxies at redshift z ∼ 2. In: Astrophysical Journal. 2008 ; Vol. 677, No. 2. pp. 943-956.
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abstract = "The Spitzer Space Telescope has revealed a significant population of high-redshift (z ∼ 2) dust-obscured galaxies with large mid-infrared to ultraviolet luminosity ratios. Due to their optical faintness, these galaxies have been previously missed in traditional optical studies of the distant universe. We present a simple method for selecting this high-redshift population based solely on the ratio of the observed mid-infrared 24 μm to optical R-band flux density. We apply this method to observations of the ≈8.6 deg2 NOAO Deep Wide-Field Survey Bootes field, and uncover ≈2600 dust-obscured galaxy candidates [i.e., 0.089 arcmin-2) with 24 μm flux densities F24 μm ≥ 0.3 mJy and (R - [24]) > 14 (i.e., Fν(24 μm)/Fν(R) ≳ 1000]. These galaxies have no counterparts in the local universe. They represent 7{\%} ± 0.6{\%} of the 24 μm source population at F24 μm ≥ 1 mJy but increase to ≈13{\%} ± 1{\%} of the population at ≈0.3 mJy. These galaxies exhibit evidence of both star formation and AGN activity, with the brighter 24 μm sources being more AGN-dominated. We have measured spectroscopic redshifts for 86 of these galaxies, and find a broad redshift distribution centered at z̄ ≈ 1.99 ± 0.05. The space density of this population is ⊃DOG(F24μm ≥ 0.3 mJy) = (2.82 ± 0.05) × 10-5h703 Mpc-3, similar to that of bright submillimeter-selected galaxies at comparable redshifts. These redshifts imply large luminosities, with median νLν(8 μm) ≈ 4 × 1011 L⊙. The infrared luminosity density contributed by this relatively rare dust-obscured galaxy population is log(IRLD) ≈8.23-0.30+0.18. This is ≈60 -15+40{\%} of that contributed by z ∼ 2 ultraluminous infrared galaxies (ULIRGs, with LIR > 1012 L ⊙); our simple selection thus identifies a significant fraction of z ∼ 2 ULIRGs. This IRLD is ≈26{\%} ± 14{\%} of the total contributed by all z ∼ 2 galaxies. We suggest that these dust-obscured galaxies are the progenitors of luminous (∼4L*) present-day galaxies, seen undergoing an extremely luminous, short-lived phase of both bulge and black hole growth. They may represent a brief evolutionary phase between submillimeter-selected galaxies and less obscured quasars or galaxies.",
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T1 - A significant population of very luminous dust-obscured galaxies at redshift z ∼ 2

AU - Dey, Arjun

AU - Soifer, B. T.

AU - Desai, Vandana

AU - Brand, Kate

AU - Le Floc'h, Emeric

AU - Brown, Michael J I

AU - Jannuzi, Buell Tomasson

AU - Armus, Lee

AU - Bussmann, Shane

AU - Brodwin, Mark

AU - Bian, Chao

AU - Eisenhardt, Peter

AU - Higdon, Sarah J.

AU - Weedman, Daniel

AU - Willner, S. P.

PY - 2008/4/20

Y1 - 2008/4/20

N2 - The Spitzer Space Telescope has revealed a significant population of high-redshift (z ∼ 2) dust-obscured galaxies with large mid-infrared to ultraviolet luminosity ratios. Due to their optical faintness, these galaxies have been previously missed in traditional optical studies of the distant universe. We present a simple method for selecting this high-redshift population based solely on the ratio of the observed mid-infrared 24 μm to optical R-band flux density. We apply this method to observations of the ≈8.6 deg2 NOAO Deep Wide-Field Survey Bootes field, and uncover ≈2600 dust-obscured galaxy candidates [i.e., 0.089 arcmin-2) with 24 μm flux densities F24 μm ≥ 0.3 mJy and (R - [24]) > 14 (i.e., Fν(24 μm)/Fν(R) ≳ 1000]. These galaxies have no counterparts in the local universe. They represent 7% ± 0.6% of the 24 μm source population at F24 μm ≥ 1 mJy but increase to ≈13% ± 1% of the population at ≈0.3 mJy. These galaxies exhibit evidence of both star formation and AGN activity, with the brighter 24 μm sources being more AGN-dominated. We have measured spectroscopic redshifts for 86 of these galaxies, and find a broad redshift distribution centered at z̄ ≈ 1.99 ± 0.05. The space density of this population is ⊃DOG(F24μm ≥ 0.3 mJy) = (2.82 ± 0.05) × 10-5h703 Mpc-3, similar to that of bright submillimeter-selected galaxies at comparable redshifts. These redshifts imply large luminosities, with median νLν(8 μm) ≈ 4 × 1011 L⊙. The infrared luminosity density contributed by this relatively rare dust-obscured galaxy population is log(IRLD) ≈8.23-0.30+0.18. This is ≈60 -15+40% of that contributed by z ∼ 2 ultraluminous infrared galaxies (ULIRGs, with LIR > 1012 L ⊙); our simple selection thus identifies a significant fraction of z ∼ 2 ULIRGs. This IRLD is ≈26% ± 14% of the total contributed by all z ∼ 2 galaxies. We suggest that these dust-obscured galaxies are the progenitors of luminous (∼4L*) present-day galaxies, seen undergoing an extremely luminous, short-lived phase of both bulge and black hole growth. They may represent a brief evolutionary phase between submillimeter-selected galaxies and less obscured quasars or galaxies.

AB - The Spitzer Space Telescope has revealed a significant population of high-redshift (z ∼ 2) dust-obscured galaxies with large mid-infrared to ultraviolet luminosity ratios. Due to their optical faintness, these galaxies have been previously missed in traditional optical studies of the distant universe. We present a simple method for selecting this high-redshift population based solely on the ratio of the observed mid-infrared 24 μm to optical R-band flux density. We apply this method to observations of the ≈8.6 deg2 NOAO Deep Wide-Field Survey Bootes field, and uncover ≈2600 dust-obscured galaxy candidates [i.e., 0.089 arcmin-2) with 24 μm flux densities F24 μm ≥ 0.3 mJy and (R - [24]) > 14 (i.e., Fν(24 μm)/Fν(R) ≳ 1000]. These galaxies have no counterparts in the local universe. They represent 7% ± 0.6% of the 24 μm source population at F24 μm ≥ 1 mJy but increase to ≈13% ± 1% of the population at ≈0.3 mJy. These galaxies exhibit evidence of both star formation and AGN activity, with the brighter 24 μm sources being more AGN-dominated. We have measured spectroscopic redshifts for 86 of these galaxies, and find a broad redshift distribution centered at z̄ ≈ 1.99 ± 0.05. The space density of this population is ⊃DOG(F24μm ≥ 0.3 mJy) = (2.82 ± 0.05) × 10-5h703 Mpc-3, similar to that of bright submillimeter-selected galaxies at comparable redshifts. These redshifts imply large luminosities, with median νLν(8 μm) ≈ 4 × 1011 L⊙. The infrared luminosity density contributed by this relatively rare dust-obscured galaxy population is log(IRLD) ≈8.23-0.30+0.18. This is ≈60 -15+40% of that contributed by z ∼ 2 ultraluminous infrared galaxies (ULIRGs, with LIR > 1012 L ⊙); our simple selection thus identifies a significant fraction of z ∼ 2 ULIRGs. This IRLD is ≈26% ± 14% of the total contributed by all z ∼ 2 galaxies. We suggest that these dust-obscured galaxies are the progenitors of luminous (∼4L*) present-day galaxies, seen undergoing an extremely luminous, short-lived phase of both bulge and black hole growth. They may represent a brief evolutionary phase between submillimeter-selected galaxies and less obscured quasars or galaxies.

KW - Galaxies: formation

KW - Galaxies: high-redshift

KW - Galaxies: starburst

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