Lyman-α emitters as tracers of the transitioning Universe

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Table 1

Best-fit results for Eq. (2).

log L_Lyα	z_tr	A F₀	θ

42.0	2.18	0.18	1.84
42.5	2.33	0.31	1.31
43.0	2.76	0.53	0.91

ULIRGs	2.52	0.2	2.28

Notes. The results at the bottom of the table refer to the best-fit parameters for a sample of LAE ULIRGs, presented in Nilsson & Møller (2009).

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