Figure 3. The g, r, i, and z band light curves 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 3. The g, r, i, and z band light curves

The complete figure set (200 images) is available in the online journal.

Example light-curves in the g, r, i, and z bands for the two sample quasars J022020.02–034331.1 in MD01 and J221917.01–000757.5 in MD09. The shaded region is the weighted mean of JAVELIN light curves that are consistent with the data and the ﹩1\sigma ﹩ dispersion of those light curves. Light curves for the full sample with JAVELIN fits are available online.

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