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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 Journal 931 .

  • Provider: AAS Journals

Caption: Figure 9.

Left: C IV parameter space for our sample colored by the log of He II EQW. The error bars are the same as in Figure 2. Right: same plot colored by α ox instead. The markers are the same as the top panel of Figure 4. Despite our cut on Γ to remove absorbed objects, it is clear that there are still factors that affect the usefulness of α ox as an indicator of the shape of the ionizing SED in comparison to the log of He II EQW, such as variability.

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