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The Circumgalactic Medium from the CAMELS Simulations: Forecasting Constraints on Feedback Processes from Future Sunyaev–Zeldovich Observations

  • Authors: Emily Moser, Nicholas Battaglia, Daisuke Nagai, Erwin Lau, Luis Fernando Machado Poletti Valle, Francisco Villaescusa-Navarro, Stefania Amodeo, Daniel Anglés-Alcázar, Greg L. Bryan, Romeel Dave, Lars Hernquist, Mark Vogelsberger

Emily Moser et al 2022 The Astrophysical Journal 933 .

  • Provider: AAS Journals

Caption: Figure 6.

Corner plots showing constraints from the CMASS emulator for CAMELS-IllustrisTNG (left) and CAMELS-SIMBA (right) for the different radial components of the profiles, as discussed in Section 3.1.2. The blue contours show the forecasted constraints of the feedback parameter using the inner profile (inward of 3′), and the red contours show the forecasted constraints using the outer profile. These profiles and derivatives were calculated using a Gaussian beam, and the ± 1σ value of the distribution for each parameter is shown above each panel on the diagonal and is listed in Table 2. It can be seen from all panels that the inner profile provides tighter contraints than the outer profile, which is expected due to the smaller error bars.

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