High-redshift sdss quasars with weak emission lines

Aleksandar M. Diamond-Stanic, Xiaohui Fan, W. N. Brandt, Ohad Shemmer, Michael A. Strauss, Scott F. Anderson, Christopher L. Carilli, Robert R. Gibson, Linhua Jiang, J. Serena Kim, Gordon T. Richards, Gary D. Schmidt, Donald P. Schneider, Yue Shen, Paul S. Smith, Marianne Vestergaard, Jason E. Young

Research output: Contribution to journalArticle

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Abstract

We identify a sample of 74 high-redshift quasars (z > 3) with weak emission lines from the Fifth Data Release of the Sloan Digital Sky Survey and present infrared, optical, and radio observations of a subsample of four objects at z > 4. These weak emission-line quasars (WLQs) constitute a prominent tail of the Lyα + N v equivalent width distribution, and we compare them to quasars with more typical emission-line properties and to low-redshift active galactic nuclei with weak/absent emission lines, namely BL Lac objects. We find that WLQs exhibit hot (T 1000K) thermal dust emission and have rest-frame 0.1-5 μm spectral energy distributions that are quite similar to those of normal quasars. The variability, polarization, and radio properties of WLQs are also different from those of BL Lacs, making continuum boosting by a relativistic jet an unlikely physical interpretation. The most probable scenario for WLQs involves broad-line region properties that are physically distinct from those of normal quasars.

Original languageEnglish (US)
Pages (from-to)782-799
Number of pages18
JournalAstrophysical Journal
Volume699
Issue number1
DOIs
StatePublished - 2009

Fingerprint

quasars
radio
radio observation
spectral energy distribution
active galactic nuclei
polarization
dust
continuums
energy

Keywords

  • Quasars: emission lines
  • Quasars: general

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

Diamond-Stanic, A. M., Fan, X., Brandt, W. N., Shemmer, O., Strauss, M. A., Anderson, S. F., ... Young, J. E. (2009). High-redshift sdss quasars with weak emission lines. Astrophysical Journal, 699(1), 782-799. https://doi.org/10.1088/0004-637X/699/1/782

High-redshift sdss quasars with weak emission lines. / Diamond-Stanic, Aleksandar M.; Fan, Xiaohui; Brandt, W. N.; Shemmer, Ohad; Strauss, Michael A.; Anderson, Scott F.; Carilli, Christopher L.; Gibson, Robert R.; Jiang, Linhua; Kim, J. Serena; Richards, Gordon T.; Schmidt, Gary D.; Schneider, Donald P.; Shen, Yue; Smith, Paul S.; Vestergaard, Marianne; Young, Jason E.

In: Astrophysical Journal, Vol. 699, No. 1, 2009, p. 782-799.

Research output: Contribution to journalArticle

Diamond-Stanic, AM, Fan, X, Brandt, WN, Shemmer, O, Strauss, MA, Anderson, SF, Carilli, CL, Gibson, RR, Jiang, L, Kim, JS, Richards, GT, Schmidt, GD, Schneider, DP, Shen, Y, Smith, PS, Vestergaard, M & Young, JE 2009, 'High-redshift sdss quasars with weak emission lines', Astrophysical Journal, vol. 699, no. 1, pp. 782-799. https://doi.org/10.1088/0004-637X/699/1/782
Diamond-Stanic AM, Fan X, Brandt WN, Shemmer O, Strauss MA, Anderson SF et al. High-redshift sdss quasars with weak emission lines. Astrophysical Journal. 2009;699(1):782-799. https://doi.org/10.1088/0004-637X/699/1/782
Diamond-Stanic, Aleksandar M. ; Fan, Xiaohui ; Brandt, W. N. ; Shemmer, Ohad ; Strauss, Michael A. ; Anderson, Scott F. ; Carilli, Christopher L. ; Gibson, Robert R. ; Jiang, Linhua ; Kim, J. Serena ; Richards, Gordon T. ; Schmidt, Gary D. ; Schneider, Donald P. ; Shen, Yue ; Smith, Paul S. ; Vestergaard, Marianne ; Young, Jason E. / High-redshift sdss quasars with weak emission lines. In: Astrophysical Journal. 2009 ; Vol. 699, No. 1. pp. 782-799.
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AU - Fan, Xiaohui

AU - Brandt, W. N.

AU - Shemmer, Ohad

AU - Strauss, Michael A.

AU - Anderson, Scott F.

AU - Carilli, Christopher L.

AU - Gibson, Robert R.

AU - Jiang, Linhua

AU - Kim, J. Serena

AU - Richards, Gordon T.

AU - Schmidt, Gary D.

AU - Schneider, Donald P.

AU - Shen, Yue

AU - Smith, Paul S.

AU - Vestergaard, Marianne

AU - Young, Jason E.

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N2 - We identify a sample of 74 high-redshift quasars (z > 3) with weak emission lines from the Fifth Data Release of the Sloan Digital Sky Survey and present infrared, optical, and radio observations of a subsample of four objects at z > 4. These weak emission-line quasars (WLQs) constitute a prominent tail of the Lyα + N v equivalent width distribution, and we compare them to quasars with more typical emission-line properties and to low-redshift active galactic nuclei with weak/absent emission lines, namely BL Lac objects. We find that WLQs exhibit hot (T 1000K) thermal dust emission and have rest-frame 0.1-5 μm spectral energy distributions that are quite similar to those of normal quasars. The variability, polarization, and radio properties of WLQs are also different from those of BL Lacs, making continuum boosting by a relativistic jet an unlikely physical interpretation. The most probable scenario for WLQs involves broad-line region properties that are physically distinct from those of normal quasars.

AB - We identify a sample of 74 high-redshift quasars (z > 3) with weak emission lines from the Fifth Data Release of the Sloan Digital Sky Survey and present infrared, optical, and radio observations of a subsample of four objects at z > 4. These weak emission-line quasars (WLQs) constitute a prominent tail of the Lyα + N v equivalent width distribution, and we compare them to quasars with more typical emission-line properties and to low-redshift active galactic nuclei with weak/absent emission lines, namely BL Lac objects. We find that WLQs exhibit hot (T 1000K) thermal dust emission and have rest-frame 0.1-5 μm spectral energy distributions that are quite similar to those of normal quasars. The variability, polarization, and radio properties of WLQs are also different from those of BL Lacs, making continuum boosting by a relativistic jet an unlikely physical interpretation. The most probable scenario for WLQs involves broad-line region properties that are physically distinct from those of normal quasars.

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