UV LFs at 15 ≤ z ≤ 20 based on the F200W-dropout selection of the ASTRODEEP-JWST catalogues, compared to results from the literature by Harikane et al. (2025), Donnan et al. (2024), Robertson et al. (2024), Casey et al. (2024), Finkelstein et al. (2024), Whitler et al. (2025), Kokorev et al. (2025), Weibel et al. (2025b) (see label for details). The UV LF at 15 ≤ z ≤ 20 is shown for the two scenarios discussed in Sect. 5: assuming that all candidates are at z > 15 (case 1: black circles and error-bars) or that they are all interlopers (case 2: red squares and 1-σ upper limits).