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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 6.

Left: C IV parameter space colored by Γ. Right: C IV parameter space colored by Δα ox. The error bars are the same as those used for Figure 2. The markers are the same as for the top panel of Figure 4. The Chandra/HST sample, the SDSS-RM sample, and the Nardini et al. (2019) sample are highlighted in black. Though general trends exist in both parameter spaces, outliers are possible at all values of C IV EQW and blueshift.

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