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Spectroscopic Confirmation of Two X-Ray Diffuse and Massive Galaxy Clusters at Low Redshift

  • Authors: Kaiyuan Chen, Weiwei Xu, Linhua Jiang

Kaiyuan Chen et al 2022 The Astrophysical Journal 940 .

  • Provider: AAS Journals

Caption: Figure 5.

Galaxy number densities (shown as stars) as a function of radius. The magenta curve shows the X-ray photon number profile (units are labeled on the right). The green solid line is the best fit of the NFW model profile using the data points between 1 and 2 Mpc. The green dashed line is prediction from the best fit.

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