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Active Galactic Nuclei Are Not Responsible for Systematics in the Empirical Properties of Type Ia Supernovae

  • Authors: Peter Clark

Peter Clark 2026 Research Notes of the AAS 10 .

  • Provider: AAS Journals

Caption: Figure 1.

The Δμ distribution of the full SNe Ia sample versus host mass (purple shading). Red upward triangles mark SNe in AGN-hosting galaxies, while teal downward triangles show mass-matched non-AGN counterparts. Weighted means (dashed lines) agree within uncertainties. Full-sample means are shown as circles and hexagons.

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