The spectral energy distribution of PKS 2004-447

A compact steep-spectrum source and possible radio-loud narrow-line Seyfert 1 galaxy

L. C. Gallo, P. G. Edwards, E. Ferrero, Jun Kataoka, D. R. Lewis, S. P. Ellingsen, Z. Misanovic, W. F. Welsh, M. Whiting, Th Boller, W. Brinkmann, J. Greenhill, A. Oshlack

Research output: Contribution to journalArticle

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Abstract

An investigation of the spectral energy distribution (SED) of the compact steep-spectrum (CSS) source and possible radio-loud narrow-line Seyfert 1 galaxy (NLS1), PKS 2004-447, is presented. Five out of six well-studied radio-loud NLS1 hare this dual classification [optically defined as an NLS1 with radio definition of a CSS or gigahertz-peaked spectrum (GPS) source], suggesting that the connection could have a physical origin. The SED is created from simultaneous observations (within 24 h) at radio (from Australia Telescope Compact Array), optical/near-infrared (MR) (from Siding Spring) and UV/X-ray (from XMM-Newton) wavelengths. The X-ray data show evidence of short-term variability (primarily a ∼30 per cent increase in the final 4 ks of the observation), a possible soft excess and negligible absorption. Together with the rest of the SED, the X-ray emission is excessive in comparison to synchrotron plus synchrotron self-Compton (SSC) models. The SED can be described with a two-component model consisting of extended synchrotron/SSC emission with Comptonization in the X-rays, though SSC models with a very high electron-to-magnetic energy density ratio cannot be excluded either. The peak emission in the SED appears to be in the MR, which can be attributed to thermal emission (T ≈ 1000 K) from a dusty torus. Analysis of a non-contemporaneous, low-resolution optical spectrum suggests that the narrow-line region (NLR) is much more reddened than the X-ray emitting region suggesting that the gas-to-dust ratio in PKS 2004-447 may be very different than in our own Galaxy. This could be achieved if the radio jets in PKS 2004-447 deposits material from the nucleus into the NLR. Long-term radio monitoring of PKS 2004-447 shows a rather constant light curve over nearly a six-month period with the exception of one outburst when the 6.65-GHz flux increased by ∼35 per cent over 19 d. It is not possible to differentiate between intrinsic or extrinsic (i.e. interstellar scintillation) origins for this outburst, but the detection of the rare event demonstrates the importance of intensive monitoring campaigns. In comparison to general samples of GPS sources, which appear to be X-ray weak, NLS1-CSS/GPS sources possess stronger X-ray emission relative to radio (comparable to normal radio-loud AGN). In addition, NLS1-CSS/GPS sources also exhibit lower intrinsic absorption than GPS sources of similar X-ray luminosity. This is consistent with the additional X-ray component required for PKS 2004-447, but larger samples of NLS1-CSS/GPS are needed before any conclusive remarks can be made.

Original languageEnglish
Pages (from-to)245-254
Number of pages10
JournalMonthly Notices of the Royal Astronomical Society
Volume370
Issue number1
DOIs
Publication statusPublished - 2006 Jul
Externally publishedYes

Fingerprint

spectral energy distribution
radio
galaxies
energy
synchrotrons
compact galaxies
x rays
outburst
distribution
thermal emission
XMM-Newton telescope
monitoring
newton
light curve
scintillation
optical spectrum
flux density
dust
near infrared
deposits

Keywords

  • Galaxies: active
  • Galaxies: nuclei
  • Quasars: individual: PKS 2004-447
  • Radio continuum: galaxies
  • X-rays: galaxies

ASJC Scopus subject areas

  • Space and Planetary Science

Cite this

The spectral energy distribution of PKS 2004-447 : A compact steep-spectrum source and possible radio-loud narrow-line Seyfert 1 galaxy. / Gallo, L. C.; Edwards, P. G.; Ferrero, E.; Kataoka, Jun; Lewis, D. R.; Ellingsen, S. P.; Misanovic, Z.; Welsh, W. F.; Whiting, M.; Boller, Th; Brinkmann, W.; Greenhill, J.; Oshlack, A.

In: Monthly Notices of the Royal Astronomical Society, Vol. 370, No. 1, 07.2006, p. 245-254.

Research output: Contribution to journalArticle

Gallo, LC, Edwards, PG, Ferrero, E, Kataoka, J, Lewis, DR, Ellingsen, SP, Misanovic, Z, Welsh, WF, Whiting, M, Boller, T, Brinkmann, W, Greenhill, J & Oshlack, A 2006, 'The spectral energy distribution of PKS 2004-447: A compact steep-spectrum source and possible radio-loud narrow-line Seyfert 1 galaxy', Monthly Notices of the Royal Astronomical Society, vol. 370, no. 1, pp. 245-254. https://doi.org/10.1111/j.1365-2966.2006.10482.x
Gallo, L. C. ; Edwards, P. G. ; Ferrero, E. ; Kataoka, Jun ; Lewis, D. R. ; Ellingsen, S. P. ; Misanovic, Z. ; Welsh, W. F. ; Whiting, M. ; Boller, Th ; Brinkmann, W. ; Greenhill, J. ; Oshlack, A. / The spectral energy distribution of PKS 2004-447 : A compact steep-spectrum source and possible radio-loud narrow-line Seyfert 1 galaxy. In: Monthly Notices of the Royal Astronomical Society. 2006 ; Vol. 370, No. 1. pp. 245-254.
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T1 - The spectral energy distribution of PKS 2004-447

T2 - A compact steep-spectrum source and possible radio-loud narrow-line Seyfert 1 galaxy

AU - Gallo, L. C.

AU - Edwards, P. G.

AU - Ferrero, E.

AU - Kataoka, Jun

AU - Lewis, D. R.

AU - Ellingsen, S. P.

AU - Misanovic, Z.

AU - Welsh, W. F.

AU - Whiting, M.

AU - Boller, Th

AU - Brinkmann, W.

AU - Greenhill, J.

AU - Oshlack, A.

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N2 - An investigation of the spectral energy distribution (SED) of the compact steep-spectrum (CSS) source and possible radio-loud narrow-line Seyfert 1 galaxy (NLS1), PKS 2004-447, is presented. Five out of six well-studied radio-loud NLS1 hare this dual classification [optically defined as an NLS1 with radio definition of a CSS or gigahertz-peaked spectrum (GPS) source], suggesting that the connection could have a physical origin. The SED is created from simultaneous observations (within 24 h) at radio (from Australia Telescope Compact Array), optical/near-infrared (MR) (from Siding Spring) and UV/X-ray (from XMM-Newton) wavelengths. The X-ray data show evidence of short-term variability (primarily a ∼30 per cent increase in the final 4 ks of the observation), a possible soft excess and negligible absorption. Together with the rest of the SED, the X-ray emission is excessive in comparison to synchrotron plus synchrotron self-Compton (SSC) models. The SED can be described with a two-component model consisting of extended synchrotron/SSC emission with Comptonization in the X-rays, though SSC models with a very high electron-to-magnetic energy density ratio cannot be excluded either. The peak emission in the SED appears to be in the MR, which can be attributed to thermal emission (T ≈ 1000 K) from a dusty torus. Analysis of a non-contemporaneous, low-resolution optical spectrum suggests that the narrow-line region (NLR) is much more reddened than the X-ray emitting region suggesting that the gas-to-dust ratio in PKS 2004-447 may be very different than in our own Galaxy. This could be achieved if the radio jets in PKS 2004-447 deposits material from the nucleus into the NLR. Long-term radio monitoring of PKS 2004-447 shows a rather constant light curve over nearly a six-month period with the exception of one outburst when the 6.65-GHz flux increased by ∼35 per cent over 19 d. It is not possible to differentiate between intrinsic or extrinsic (i.e. interstellar scintillation) origins for this outburst, but the detection of the rare event demonstrates the importance of intensive monitoring campaigns. In comparison to general samples of GPS sources, which appear to be X-ray weak, NLS1-CSS/GPS sources possess stronger X-ray emission relative to radio (comparable to normal radio-loud AGN). In addition, NLS1-CSS/GPS sources also exhibit lower intrinsic absorption than GPS sources of similar X-ray luminosity. This is consistent with the additional X-ray component required for PKS 2004-447, but larger samples of NLS1-CSS/GPS are needed before any conclusive remarks can be made.

AB - An investigation of the spectral energy distribution (SED) of the compact steep-spectrum (CSS) source and possible radio-loud narrow-line Seyfert 1 galaxy (NLS1), PKS 2004-447, is presented. Five out of six well-studied radio-loud NLS1 hare this dual classification [optically defined as an NLS1 with radio definition of a CSS or gigahertz-peaked spectrum (GPS) source], suggesting that the connection could have a physical origin. The SED is created from simultaneous observations (within 24 h) at radio (from Australia Telescope Compact Array), optical/near-infrared (MR) (from Siding Spring) and UV/X-ray (from XMM-Newton) wavelengths. The X-ray data show evidence of short-term variability (primarily a ∼30 per cent increase in the final 4 ks of the observation), a possible soft excess and negligible absorption. Together with the rest of the SED, the X-ray emission is excessive in comparison to synchrotron plus synchrotron self-Compton (SSC) models. The SED can be described with a two-component model consisting of extended synchrotron/SSC emission with Comptonization in the X-rays, though SSC models with a very high electron-to-magnetic energy density ratio cannot be excluded either. The peak emission in the SED appears to be in the MR, which can be attributed to thermal emission (T ≈ 1000 K) from a dusty torus. Analysis of a non-contemporaneous, low-resolution optical spectrum suggests that the narrow-line region (NLR) is much more reddened than the X-ray emitting region suggesting that the gas-to-dust ratio in PKS 2004-447 may be very different than in our own Galaxy. This could be achieved if the radio jets in PKS 2004-447 deposits material from the nucleus into the NLR. Long-term radio monitoring of PKS 2004-447 shows a rather constant light curve over nearly a six-month period with the exception of one outburst when the 6.65-GHz flux increased by ∼35 per cent over 19 d. It is not possible to differentiate between intrinsic or extrinsic (i.e. interstellar scintillation) origins for this outburst, but the detection of the rare event demonstrates the importance of intensive monitoring campaigns. In comparison to general samples of GPS sources, which appear to be X-ray weak, NLS1-CSS/GPS sources possess stronger X-ray emission relative to radio (comparable to normal radio-loud AGN). In addition, NLS1-CSS/GPS sources also exhibit lower intrinsic absorption than GPS sources of similar X-ray luminosity. This is consistent with the additional X-ray component required for PKS 2004-447, but larger samples of NLS1-CSS/GPS are needed before any conclusive remarks can be made.

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KW - Galaxies: nuclei

KW - Quasars: individual: PKS 2004-447

KW - Radio continuum: galaxies

KW - X-rays: galaxies

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