Open Access
Table B.2.
References used for the chi square calculation of each observable.
| Observable | redshifts | References used |
|---|---|---|
| UVLF of LBGs | 5-14 | Bouwens et al. (2022, 2021, 2023), Harikane et al. (2022), 2023a, 2024), Pérez-González et al. (2023), Atek et al. (2015, 2018), Oesch et al. (2018), Adams et al. (2022), Donnan et al. (2022), Donnan et al. (2024), Bowler et al. (2017), Willott et al. (2024), Naidu et al. (2022), McLeod et al. (2024), Robertson et al. (2024), Whitler et al. (2025), Leung et al. (2023), Adams et al. (2024), Casey et al. (2024) |
| SMF of LBGs | 5-10,12 | Navarro-Carrera et al. (2024), Song et al. (2016), Duncan et al. (2014), Bhatawdekar et al. (2019), Stefanon et al. (2021), Harvey et al. (2025) |
| BHMF of JWST AGNs | 5,6 | Kokorev et al. (2024), Matthee et al. (2023), Taylor et al. (2025) |
| bolometric LF of JWST AGNs | 5-8a | Kokorev et al. (2024), Akins et al. (2025a) |
a
Notes.When we use the − sign on the second column of redshifts, we refer to all inclusive redshifts separated by bins of Δz = 1. For example, 5−8 = {5, 6, 7, 8}.
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