The radio-loud fraction of quasars is a strong function of redshift and optical luminosity

Linhua Jiang, Xiaohui Fan, Žeuko Ivezić, Gordon T. Richards, Donald P. Schneider, Michael A. Strauss, Brandon C. Kelly

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Abstract

Using a sample of optically selected quasars from the Sloan Digital Sky Survey, we have determined the radio-loud fraction (RLF) of quasars as a function of redshift and optical luminosity. The sample contains more than 30,000 objects and spans a redshift range of 0 < z ≤ 5 and a luminosity range of -30 ≤ Mi < -22. We use both the radio-to-optical flux ratio (R parameter) and the radio luminosity to define radio-loud quasars. After breaking the correlation between redshift and luminosity due to the flux-limited nature of the sample, we find that the RLF of quasars decreases with increasing redshift and decreasing luminosity. The relation can be described in the form of log [RLF/( 1 - RLF)] = b0 + bz log (1 + z) + bM(M2500 + 26), where M2500 is the absolute magnitude at rest-frame 2500 Å, and bz, b M < 0. When using R > 10 to define radio-loud quasars, we find that b0 = -0.132 ±0.116, bz = -2.052 ± 0.261, and bM = -0.183 ± 0.025. The RLF at z = 0.5 declines from 24.3% to 5.6% as luminosity decreases from M2500 = -26 to -22, and the RLF at M2500 = -26 declines from 24.3% to 4.1% as redshift increases from 0.5 to 3, suggesting that the RLF is a strong function of both redshift and luminosity. We also examine the impact of flux-related selection effects on the RLF determination using a series of tests and find that the dependence of the RLF on redshift and luminosity is highly likely to be physical, and that the selection effects we considered are not responsible for the dependence.

Original languageEnglish (US)
Pages (from-to)680-690
Number of pages11
JournalAstrophysical Journal
Volume656
Issue number2 I
DOIs
StatePublished - Feb 20 2007

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quasars
luminosity
radio

Keywords

  • Galaxies: active
  • Quasars: general
  • Radio continuum: galaxies

ASJC Scopus subject areas

  • Space and Planetary Science

Cite this

Jiang, L., Fan, X., Ivezić, Ž., Richards, G. T., Schneider, D. P., Strauss, M. A., & Kelly, B. C. (2007). The radio-loud fraction of quasars is a strong function of redshift and optical luminosity. Astrophysical Journal, 656(2 I), 680-690. https://doi.org/10.1086/510831

The radio-loud fraction of quasars is a strong function of redshift and optical luminosity. / Jiang, Linhua; Fan, Xiaohui; Ivezić, Žeuko; Richards, Gordon T.; Schneider, Donald P.; Strauss, Michael A.; Kelly, Brandon C.

In: Astrophysical Journal, Vol. 656, No. 2 I, 20.02.2007, p. 680-690.

Research output: Contribution to journalArticle

Jiang, L, Fan, X, Ivezić, Ž, Richards, GT, Schneider, DP, Strauss, MA & Kelly, BC 2007, 'The radio-loud fraction of quasars is a strong function of redshift and optical luminosity', Astrophysical Journal, vol. 656, no. 2 I, pp. 680-690. https://doi.org/10.1086/510831
Jiang L, Fan X, Ivezić Ž, Richards GT, Schneider DP, Strauss MA et al. The radio-loud fraction of quasars is a strong function of redshift and optical luminosity. Astrophysical Journal. 2007 Feb 20;656(2 I):680-690. https://doi.org/10.1086/510831
Jiang, Linhua ; Fan, Xiaohui ; Ivezić, Žeuko ; Richards, Gordon T. ; Schneider, Donald P. ; Strauss, Michael A. ; Kelly, Brandon C. / The radio-loud fraction of quasars is a strong function of redshift and optical luminosity. In: Astrophysical Journal. 2007 ; Vol. 656, No. 2 I. pp. 680-690.
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abstract = "Using a sample of optically selected quasars from the Sloan Digital Sky Survey, we have determined the radio-loud fraction (RLF) of quasars as a function of redshift and optical luminosity. The sample contains more than 30,000 objects and spans a redshift range of 0 < z ≤ 5 and a luminosity range of -30 ≤ Mi < -22. We use both the radio-to-optical flux ratio (R parameter) and the radio luminosity to define radio-loud quasars. After breaking the correlation between redshift and luminosity due to the flux-limited nature of the sample, we find that the RLF of quasars decreases with increasing redshift and decreasing luminosity. The relation can be described in the form of log [RLF/( 1 - RLF)] = b0 + bz log (1 + z) + bM(M2500 + 26), where M2500 is the absolute magnitude at rest-frame 2500 {\AA}, and bz, b M < 0. When using R > 10 to define radio-loud quasars, we find that b0 = -0.132 ±0.116, bz = -2.052 ± 0.261, and bM = -0.183 ± 0.025. The RLF at z = 0.5 declines from 24.3{\%} to 5.6{\%} as luminosity decreases from M2500 = -26 to -22, and the RLF at M2500 = -26 declines from 24.3{\%} to 4.1{\%} as redshift increases from 0.5 to 3, suggesting that the RLF is a strong function of both redshift and luminosity. We also examine the impact of flux-related selection effects on the RLF determination using a series of tests and find that the dependence of the RLF on redshift and luminosity is highly likely to be physical, and that the selection effects we considered are not responsible for the dependence.",
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AU - Ivezić, Žeuko

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AU - Schneider, Donald P.

AU - Strauss, Michael A.

AU - Kelly, Brandon C.

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N2 - Using a sample of optically selected quasars from the Sloan Digital Sky Survey, we have determined the radio-loud fraction (RLF) of quasars as a function of redshift and optical luminosity. The sample contains more than 30,000 objects and spans a redshift range of 0 < z ≤ 5 and a luminosity range of -30 ≤ Mi < -22. We use both the radio-to-optical flux ratio (R parameter) and the radio luminosity to define radio-loud quasars. After breaking the correlation between redshift and luminosity due to the flux-limited nature of the sample, we find that the RLF of quasars decreases with increasing redshift and decreasing luminosity. The relation can be described in the form of log [RLF/( 1 - RLF)] = b0 + bz log (1 + z) + bM(M2500 + 26), where M2500 is the absolute magnitude at rest-frame 2500 Å, and bz, b M < 0. When using R > 10 to define radio-loud quasars, we find that b0 = -0.132 ±0.116, bz = -2.052 ± 0.261, and bM = -0.183 ± 0.025. The RLF at z = 0.5 declines from 24.3% to 5.6% as luminosity decreases from M2500 = -26 to -22, and the RLF at M2500 = -26 declines from 24.3% to 4.1% as redshift increases from 0.5 to 3, suggesting that the RLF is a strong function of both redshift and luminosity. We also examine the impact of flux-related selection effects on the RLF determination using a series of tests and find that the dependence of the RLF on redshift and luminosity is highly likely to be physical, and that the selection effects we considered are not responsible for the dependence.

AB - Using a sample of optically selected quasars from the Sloan Digital Sky Survey, we have determined the radio-loud fraction (RLF) of quasars as a function of redshift and optical luminosity. The sample contains more than 30,000 objects and spans a redshift range of 0 < z ≤ 5 and a luminosity range of -30 ≤ Mi < -22. We use both the radio-to-optical flux ratio (R parameter) and the radio luminosity to define radio-loud quasars. After breaking the correlation between redshift and luminosity due to the flux-limited nature of the sample, we find that the RLF of quasars decreases with increasing redshift and decreasing luminosity. The relation can be described in the form of log [RLF/( 1 - RLF)] = b0 + bz log (1 + z) + bM(M2500 + 26), where M2500 is the absolute magnitude at rest-frame 2500 Å, and bz, b M < 0. When using R > 10 to define radio-loud quasars, we find that b0 = -0.132 ±0.116, bz = -2.052 ± 0.261, and bM = -0.183 ± 0.025. The RLF at z = 0.5 declines from 24.3% to 5.6% as luminosity decreases from M2500 = -26 to -22, and the RLF at M2500 = -26 declines from 24.3% to 4.1% as redshift increases from 0.5 to 3, suggesting that the RLF is a strong function of both redshift and luminosity. We also examine the impact of flux-related selection effects on the RLF determination using a series of tests and find that the dependence of the RLF on redshift and luminosity is highly likely to be physical, and that the selection effects we considered are not responsible for the dependence.

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