An extreme EXO: A type 2 QSO at z = 1.87

A. Del Moro, M. G. Watson, S. Mateos, M. Akiyama, Y. Hashimoto, N. Tamura, K. Ohta, F. J. Carrera, G. Stewart

Research output: Contribution to journalArticle

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Abstract

Aims. We aim to understand the multi-wavelength properties of 2XMM J123204+215255, the source with the most extreme X-ray-to-optical flux ratio amongst a sample of bright X-ray selected EXOs drawn from a cross-correlation of the 2XMMp catalogue with the SDSS-DR5 catalogue. Methods. We use 2XMMp X-ray data, SDSS-DR5, NOT and UKIRT optical/NIR photometric data and Subaru MOIRCS IR spectroscopy to study the properties of 2XMM J123204+215255. We created a model SED including an obscured QSO and the host galaxy component to constrain the optical/IR extinction and the relative contribution of the AGN and the galaxy to the total emission. Results. 2XMM J123204+215255 is a bright X-ray source with fx ≈ 10-12 erg cm-2 s-1 (2-10 keV energy band) which has no detection down to a magnitude i′ 25.2. NIR imaging reveals a faint K-band counterpart and NIR spectroscopy shows a single broad (FWHM =≃ 5300 km s-1) emission line, which is almost certainly Hα at z = 1.87. The X-ray spectrum shows evidence of significant absorption (NH > 1023 cm-2), typical of type 2 AGN, but the broad Hα emission suggests a type 1 AGN classification. The very red optical/NIR colours (i′ - K > 5.3) strongly suggest significant reddening however. We find that simple modelling can successfully reproduce the NIR continuum and strongly constrain the intrinsic nuclear optical/IR extinction to Av ≈ 4, which turns out to be much smaller than the expected from the X-ray absorption (assuming Galactic gas-to-dust ratio).

Original languageEnglish
Pages (from-to)445-451
Number of pages7
JournalAstronomy and Astrophysics
Volume493
Issue number2
DOIs
Publication statusPublished - 2009 Jan 1

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quasars
x rays
catalogs
extinction
spectroscopy
galaxies
extremely high frequencies
erg
cross correlation
energy bands
dust
continuums
wavelength
color
gases
gas
wavelengths
modeling
energy

Keywords

  • Galaxies: active
  • Galaxies: quasars: general
  • Infrared: galaxies
  • X-rays: galaxies

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Del Moro, A., Watson, M. G., Mateos, S., Akiyama, M., Hashimoto, Y., Tamura, N., ... Stewart, G. (2009). An extreme EXO: A type 2 QSO at z = 1.87. Astronomy and Astrophysics, 493(2), 445-451. https://doi.org/10.1051/0004-6361:200809665

An extreme EXO : A type 2 QSO at z = 1.87. / Del Moro, A.; Watson, M. G.; Mateos, S.; Akiyama, M.; Hashimoto, Y.; Tamura, N.; Ohta, K.; Carrera, F. J.; Stewart, G.

In: Astronomy and Astrophysics, Vol. 493, No. 2, 01.01.2009, p. 445-451.

Research output: Contribution to journalArticle

Del Moro, A, Watson, MG, Mateos, S, Akiyama, M, Hashimoto, Y, Tamura, N, Ohta, K, Carrera, FJ & Stewart, G 2009, 'An extreme EXO: A type 2 QSO at z = 1.87', Astronomy and Astrophysics, vol. 493, no. 2, pp. 445-451. https://doi.org/10.1051/0004-6361:200809665
Del Moro A, Watson MG, Mateos S, Akiyama M, Hashimoto Y, Tamura N et al. An extreme EXO: A type 2 QSO at z = 1.87. Astronomy and Astrophysics. 2009 Jan 1;493(2):445-451. https://doi.org/10.1051/0004-6361:200809665
Del Moro, A. ; Watson, M. G. ; Mateos, S. ; Akiyama, M. ; Hashimoto, Y. ; Tamura, N. ; Ohta, K. ; Carrera, F. J. ; Stewart, G. / An extreme EXO : A type 2 QSO at z = 1.87. In: Astronomy and Astrophysics. 2009 ; Vol. 493, No. 2. pp. 445-451.
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