Figure 7 from THE SLOAN DIGITAL SKY SURVEY REVERBERATION MAPPING PROJECT: AN INVESTIGATION OF BIASES IN C IV EMISSION LINE PROPERTIES

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THE SLOAN DIGITAL SKY SURVEY REVERBERATION MAPPING PROJECT: AN INVESTIGATION OF BIASES IN C IV EMISSION LINE PROPERTIES

Authors: K. D. Denney, Keith Horne, Yue Shen, W. N. Brandt, Luis C. Ho, B. M. Peterson, Gordon T. Richards, J. R. Trump, and J. Ge

2016 The Astrophysical Journal Supplement Series 224 14.

Provider: AAS Journals

Caption: Figure 7.

Left: same as the left panel of Figure 5, but comparing our GH polynomial fits to the two-component Gaussian fits of Shen et al. (2016b) made with a fully automated pipeline fitting procedure applied to the same data.

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