#Title: The galaxy ultraviolet luminosity function from $z=7$ to $15$ in the COLIBRE simulations
#
# Authors: Shengdong Lu, Carlos S. Frenk, Cedric G. Lacey, Andrea Gebek, Joop Schaye, Shaun Cole, Sownak Bose,
#          Anna Durrant, Nick Andreadis, Maarten Baes, Alejandro Benítez-Llambay, Evgenii Chaikin, Camila Correa,
#          Robert A. Crain, Filip Huško, Robert J. McGibbon, Sylvia Ploeckinger, Alexander J. Richings,
#          Matthieu Schaller, James W. Trayford

#================================================================================================================================================================================================
# This dataset contains UV luminosity functions (UVLFs) at z=7-15 from the new COLIBRE simulations post-processed with SKIRT. Only the fiducial model is
# included here, i.e. COLIBRE with the thermal AGN feedback model and the fiducial COLIBRE-SKIRT pipeline of Gebek et al. (2026), measured within a
# projected 50 kpc aperture.
#
# Each file name follows the format COLIBRE_RUN_FUV_REDSHIFT.txt:
#
# RUN       The COLIBRE run used to compute the UVLF. Possible values are "L050m5", "L200m6", "L400m7", and "combined". The latter denotes the
#           combination of the three runs, following the strategy described in the paper.
#
# REDSHIFT  The redshift of the UVLF. Possible values are "z7", "z9", "z10", "z12", and "z15".
#
# Each file contains five columns:
#
# MUV                 Centre of the UV absolute-magnitude bin, in the AB system.
# logPhi_attn         Dust-attenuated UVLF in the corresponding magnitude bin, expressed as log10(Mpc^-3 mag^-1).
# err_logPhi_attn     Uncertainty on logPhi_attn, estimated using the bootstrap method.
# logPhi_unattn       Dust-free UVLF in the corresponding magnitude bin, expressed as log10(Mpc^-3 mag^-1).
# err_logPhi_unattn   Uncertainty on logPhi_unattn, estimated using the bootstrap method.
#================================================================================================================================================================================================