#Title: Galaxy luminosity functions from far-UV to submillimetre at z=0 in the COLIBRE simulations
#Authors: Shengdong Lu, Carlos S. Frenk, Cedric G. Lacey, Andrea Gebek, Joop Schaye, Shaun Cole, Sownak Bose, 
          Nick Andreadis, Maarten Baes, Alejandro Benítez-Llambay, Evgenii Chaikin, Robert A. Crain, Anna Durrant, 
          Filip Huško, Sylvia Ploeckinger, Alexander J. Richings, Matthieu Schaller, James W. Trayford

#================================================================================================================================================================================================
# This dataset contains luminosity functions (LFs) 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), calculated within a projected 50kpc
# aperture.
#
# Each file name follows the format COLIBRE_RUN_BAND_REDSHIFT_DUST.txt:
#
# RUN       The COLIBRE run used to compute the LF. Possible values are "L025m5", "L200m6", "L400m7", and "combined". The latter denotes the
#           combination of the three runs, following the strategy described in the paper.
#
# BAND      The photometric band of the LF.
#
# REDSHIFT  The redshift of the LF. "z0" and "z0p3" denote z=0 and z=0.3 (only provided for L400m7), respectively. 
#
# DUST      The dust treatment. "with_dust" includes both dust attenuation and dust emission, while "no_dust" excludes both dust attenuation and dust
#           emission. The "no_dust" case is provided only for wavelengths shorter than 24 um.
#
# Each file contains two columns:
#
# lognuLnu/Lsun          Centre of the luminosity bin, expressed as log10(nu Lnu / Lsun), where Lsun = 3.828e26 W.
# logPhi/Mpc^-3 dex^-1   Number density in the corresponding luminosity bin, expressed as log10(Mpc^-3 dex^-1).
#================================================================================================================================================================================================