Excess AGN activity in the z = 2.30 Protocluster in HS 1700+64

J. A. Digby-North, K. Nandra, E. S. Laird, C. C. Steidel, A. Georgakakis, Milan Bogosavljevic, D. K. Erb, A. E. Shapley, N. A. Reddy, J. Aird

Research output: Contribution to journalArticle

Abstract

We present the results of spectroscopic, narrow-band and X-ray observations of a z = 2.30 protocluster in the field of the QSO HS 1700+643. Using a sample of BX/MD galaxies, which are selected to be at z ∼ 2.2-2.7 by their rest-frame ultraviolet colours, we find that there are five protocluster AGN which have been identified by characteristic emission-lines in their optical/near-IR spectra; this represents an enhancement over the field significant at >98.5 per cent confidence. Using a ∼200-ks Chandra/ACIS-I observation of this field we detect a total of 161 X-ray point sources to a Poissonian false-probability limit of 4 × 10-6 and identify eight of these with BX/MD galaxies. Two of these are spectroscopically confirmed protocluster members and are also classified as emission-line AGN. When compared to a similarly selected field sample, the analysis indicates this is also evidence for an enhancement of X-ray selected BX/MD AGN over the field, significant at >99 per cent confidence. Deep Lyα narrow-band imaging reveals that a total of 4/123 Lyα emitters (LAEs) are found to be associated with X-ray sources, with two of these confirmed protocluster members and one highly likely member. We do not find a significant enhancement of AGN activity in this LAE sample over that of the field (result is significant at only 87 per cent confidence). The X-ray emitting AGN fractions for the BX/MD and LAE samples are found to be 6.9-4.4+9.2 and 2.9-1.6+2.9 per cent, respectively, for protocluster AGN with L2-10 keV ≥ 4.6 × 1043 erg s-1 at z = 2.30. These findings are similar to results from the z = 3.09 protocluster in the SSA 22 field found by Lehmer et al. (2009), in that both suggest AGN activity is favoured in dense environments at z > 2.

Original languageEnglish (US)
Pages (from-to)846-853
Number of pages8
JournalMonthly Notices of the Royal Astronomical Society
Volume407
Issue number2
DOIs
StatePublished - Sep 1 2010

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confidence
x rays
narrowband
augmentation
galaxies
erg
quasars
point sources
point source
emitters
color
analysis

Keywords

  • Galaxies: active
  • Galaxies: clusters: general
  • Galaxies: high-redshift
  • Surveys
  • X-rays: general

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Digby-North, J. A., Nandra, K., Laird, E. S., Steidel, C. C., Georgakakis, A., Bogosavljevic, M., ... Aird, J. (2010). Excess AGN activity in the z = 2.30 Protocluster in HS 1700+64. Monthly Notices of the Royal Astronomical Society, 407(2), 846-853. https://doi.org/10.1111/j.1365-2966.2010.16977.x

Excess AGN activity in the z = 2.30 Protocluster in HS 1700+64. / Digby-North, J. A.; Nandra, K.; Laird, E. S.; Steidel, C. C.; Georgakakis, A.; Bogosavljevic, Milan; Erb, D. K.; Shapley, A. E.; Reddy, N. A.; Aird, J.

In: Monthly Notices of the Royal Astronomical Society, Vol. 407, No. 2, 01.09.2010, p. 846-853.

Research output: Contribution to journalArticle

Digby-North, JA, Nandra, K, Laird, ES, Steidel, CC, Georgakakis, A, Bogosavljevic, M, Erb, DK, Shapley, AE, Reddy, NA & Aird, J 2010, 'Excess AGN activity in the z = 2.30 Protocluster in HS 1700+64', Monthly Notices of the Royal Astronomical Society, vol. 407, no. 2, pp. 846-853. https://doi.org/10.1111/j.1365-2966.2010.16977.x
Digby-North, J. A. ; Nandra, K. ; Laird, E. S. ; Steidel, C. C. ; Georgakakis, A. ; Bogosavljevic, Milan ; Erb, D. K. ; Shapley, A. E. ; Reddy, N. A. ; Aird, J. / Excess AGN activity in the z = 2.30 Protocluster in HS 1700+64. In: Monthly Notices of the Royal Astronomical Society. 2010 ; Vol. 407, No. 2. pp. 846-853.
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AU - Nandra, K.

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AU - Steidel, C. C.

AU - Georgakakis, A.

AU - Bogosavljevic, Milan

AU - Erb, D. K.

AU - Shapley, A. E.

AU - Reddy, N. A.

AU - Aird, J.

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