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Figuring Out Gas & Galaxies In Enzo (FOGGIE). XIV. The Observability of Emission from Accretion and Feedback in the Circumgalactic Medium with Current and Future Instruments

  • Authors: Vida Saeedzadeh, Jason Tumlinson, Molly S. Peeples, Brian W. O'Shea, Cassandra Lochhaas, Lauren Corlies, Cameron W. Trapp, Britton D. Smith, Jessica K. Werk, Ayan Acharyya, Ramona Augustin, Nicolas Lehner, Anna C. Wright

Vida Saeedzadeh et al 2026 The Astrophysical Journal 1004 .

  • Provider: AAS Journals

Caption: Figure 15.

Observable CGM mass fraction as a function of spatial resolution (x-axis) and surface brightness sensitivity (y-axis), for eight emission lines, averaged over six FOGGIE halos, edge-on. Each cell shows the percentage of total CGM mass detectable above the given sensitivity limit at the specified resolution, with values color coded and overlaid. As expected, observability decreases with lower sensitivity and coarser resolution, though sensitivity plays a stronger role: at fixed resolution, increasing the detection threshold from 100 to 500 reduces the detectable mass by more than 50% in several ions. These results emphasize that achieving high sensitivity is critical for maximizing CGM detection, particularly for tracing diffuse, highly ionized gas.

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