Exploring Changes in Quasar Spectral Energy Distributions across C IV Parameter Space
Authors: Angelica B. Rivera, Gordon T. Richards, Sarah C. Gallagher, Trevor V. McCaffrey, Amy L. Rankine, Paul C. Hewett, Ohad Shemmer
Angelica B. Rivera et al
2022 The Astrophysical Journal931.
Provider: AAS Journals
Caption: Figure 5.
Histogram of Δ(g − i) values for our sample. Objects that are more likely to be dust reddened (as opposed to intrinsically red) will have larger values in the red (right) tail of the Δ(g − i) distribution.