Bolometric luminosity function of AGNs under the assumption of continuous accretion at the Eddington rate shown for the different values of Ω_Λ in the colour bar for our fiducial combination w₀ = −0.98, w_a = 0.08; the dashed line marks the result for the standard ΛCDM cosmology. We compared with the measurements of Akins et al. (2024), which are based on JWST observations (red circles), derived under the assumption that the emission of LRDs is entirely contributed by AGNs, and with those of Harikane et al. (2023a, orange pentagon). For comparison, we also show the pre-JWST measurements by Shen et al. (2020) as a shaded area, by Glikman et al. (2011, square), Grazian et al. (2023, diamonds), and the X-ray measurement through Chandra COSMOS data by Barlow-Hall & Aird (2025, triangles) and Barlow-Hall et al. (2023, star).