Constraining the [C II] luminosity function from the power spectrum of line-intensity maps at redshift 3.6

Open Access

Table 1.

Schechter fits to the observed [C II] LF from L21 and Y20.

Sample	Ref.	${log}_{10} \frac{Ψ_{}}{{Mpc}^{- 3} {dex}^{- 1}}$ $\log_{10}\frac{{\Psi}_}{\mathrm{Mpc}^{-3}\,\mathrm{dex}^{-1}}$	${log}_{10} \frac{L_{}}{L_{⊙}}$ $\log_{10}\frac{L_}{L_\odot}$	α
Cluster	L21	$- 3 . 01_{- 0.61}^{+ 0.44}$ $-3.01^{+0.44}_{-0.61}$	$9 . 88_{- 0.55}^{+ 0.54}$ $9.88^{+0.54}_{-0.55}$	$- 0 . 92_{- 0.44}^{+ 0.56}$ $-0.92^{+0.56}_{-0.44}$
Combo	Y20	−3.08 ± 3	9.5 ± 0.6	−1.1 ± 0.3

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