Figure 2 from Detection of Time Lags between Quasar Continuum Emission Bands Based On Pan-STARRS Light Curves

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Detection of Time Lags between Quasar Continuum Emission Bands Based On Pan-STARRS Light Curves

Authors: Yan-Fei Jiang (姜燕飞), Paul J. Green, Jenny E. Greene, Eric Morganson, Yue Shen, Anna Pancoast, Chelsea L. MacLeod, Scott F. Anderson, W. N. Brandt, C. J. Grier, H.-W. Rix, John J. Ruan, Pavlos Protopapas, Caroline Scott, W. S. Burgett, K. W. Hodapp, M. E. Huber, N. Kaiser, R. P. Kudritzki, E. A. Magnier, N. Metcalfe, J. T. Tonry, R. J. Wainscoat, and C. Waters

2017 The Astrophysical Journal 836 186.

Provider: AAS Journals

Caption: Figure 2.

Distributions of the estimated bolometric luminosity L, black-hole mass ﹩{M}_{\mathrm{BH}}﹩, and normalized g-band excess variance ﹩{\sigma }_{\mathrm{rms}}^{2}﹩ for the 200 quasars with detected lags. Each quasar is color coded by Eddington ratio. The 39 quasars with significant detections (subsample cLD) are labeled by the open red squares. The diagonal panels are the histograms of L, ﹩{M}_{\mathrm{BH}}﹩, and ﹩{\sigma }_{\mathrm{rms}}^{2}﹩ in the two redshift bins.

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