Quantifying observational projection effects with a simulation-based hot CGM model

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Volume 697 (May 2025)

A&A, 697 (2025) A22

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Table 3.

For every stellar mass bin, we present the best-fitting parameters of the model (see Eq. (7)).

log₁₀M_★/M_⊙ min	log₁₀S₀	r_c [kpc]	β	r_s [kpc]	ϵ
10.5–11	$36 . 963_{- 0.001}^{+ 0.001}$ $36.963_{-0.001}^{+0.001}$	$11 . 37_{- 0.05}^{+ 0.05}$ $11.37_{-0.05}^{+0.05}$	$0 . 443_{- 0.001}^{+ 0.000}$ $0.443_{-0.001}^{+0.000}$	$441_{- 6}^{+ 4}$ $441_{-6}^{+4}$	$4 . 5_{- 0.1}^{+ 0.1}$ $4.5_{-0.1}^{+0.1}$
11–11.25	$37 . 631_{- 0.002}^{+ 0.002}$ $37.631_{-0.002}^{+0.002}$	$5 . 39_{- 0.07}^{+ 0.06}$ $5.39_{-0.07}^{+0.06}$	$0 . 283_{- 0.001}^{+ 0.001}$ $0.283_{-0.001}^{+0.001}$	$328_{- 2}^{+ 2}$ $328_{-2}^{+2}$	$4 . 24_{- 0.05}^{+ 0.05}$ $4.24_{-0.05}^{+0.05}$
11.25–11.5	$38 . 080_{- 0.003}^{+ 0.003}$ $38.080_{-0.003}^{+0.003}$	$4 . 00_{- 0.07}^{+ 0.08}$ $4.00_{-0.07}^{+0.08}$	$0 . 249_{- 0.001}^{+ 0.001}$ $0.249_{-0.001}^{+0.001}$	$407_{- 2}^{+ 2}$ $407_{-2}^{+2}$	$4 . 70_{- 0.03}^{+ 0.03}$ $4.70_{-0.03}^{+0.03}$

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