Figure 12 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 12.

Distributions of lag with luminosity for the 39 cLD quasars with significant, consistent detections. Each data point is color coded by the estimated black-hole mass. From top to bottom, the three panels are rest frame lags between g − r, g − i, and g − z bands respectively. The dashed black lines in each panel indicate 0 lags.

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