Challenges of standard halo models in constraining galaxy properties from cosmic infrared background anisotropies

Open Access

Table 1.

Best-fit values with uncertainties and the ranges of uniform distributions used as priors for fitting the M21 HOD model to mock data from SIDES-Uchuu.

	log M_h, max	η_max	σ_{M_h0}	τ	SN₂₁₇	SN₃₅₃	SN₅₄₅	SN₈₅₇
	[M_⊙]				[Jy²/sr]	[Jy²/sr]	[Jy²/sr]	[Jy²/sr]
Best-fit value	$12 . 34_{- 0.08}^{+ 0.07}$ $12.34^{+0.07}_{-0.08}$	$0 . 27_{- 0.01}^{+ 0.01}$ $0.27^{+0.01}_{-0.01}$	$1 . 99_{- 0.12}^{+ 0.06}$ $1.99^{+0.06}_{-0.12}$	$1 . 06_{- 0.18}^{+ 0.16}$ $1.06^{+0.16}_{-0.18}$	$17 . 81_{- 0.32}^{+ 0.17}$ $17.81^{+0.17}_{-0.32}$	$300_{- 11}^{+ 10}$ $300^{+10}_{-11}$	$3684_{- 124}^{+ 122}$ $3684^{+122}_{-124}$	$43770_{- 927}^{+ 887}$ $43770^{+887}_{-927}$
Prior lower limit	8	0	0	0	14	240	2947	35016
Prior upper limit	15	1	2	3	21	360	4421	52524

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