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\title{Disk-Jet Connection in Active Supermassive Black Holes in the Standard Accretion Disk Regime
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\author{\speaker{Yoshiyuki Inoue}\\
        ISAS/JAXA
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        E-mail: \email{yinoue@astro.isas.jaxa.jp
}}

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\abstract{
  Previous gamma-ray blazar studies revealed that the jet production efficiency is ~1. Here, we studied the disk-jet connection in active supermassive black holes by investigating the properties of optical and radio emissions of radio-loud quasars. We found that the jet powers correlate with the bolometric disk luminosities as log P$_{jet}$= 0.96 log L$_{disk}$+ 0.79. This suggests the jet production efficiency of ~ 0.011, implying low black hole spin parameters and/or low magnetic flux for radio-loud quasars. This result contradicts previous jet power studies based on gamma-ray blazars. We will discuss the cause of this discrepancy and discuss possible uncertainties in jet power evaluation. This work is published as [Inoue et al. 2017, ApJ, 840, 12.][1] 


  [1]: http://adsabs.harvard.edu/abs/2017ApJ...840...46I
}

\FullConference{7th Fermi Symposium 2017\\
		15-20 October 2017\\
		Garmisch-Partenkirchen, Germany}


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