#############################################
# AMICO-miniJPAS catalog of galaxy clusters #
#############################################
#
# Catalog based on:
#   PDR201912: catalog of galaxies, r-band photometry
#   PDR201912: photo-z produced with the Lephare algorithm
#   AMICO, model based on luminosity function (Henning+ 2017, Zeneteno+ 2018) and NFW profile for M=1e14Msun/h
#   Chandra and XMM Newton X-ray data
#
# Range restricted to:
#   0.05<z<0.8
#   S/N>2.5
#
# Remarks:
#   Lambda_* is redshift independent up to z<0.56
#   we suggest to use the amplitude, A, as mass proxy
#   we suggest to use the redshift based on the probabilistic AMICO membership Z_PROB instead of Z 
#
# Reference:
#   The miniJPAS survey: Cluster and galaxy group detections with AMICO
#     M. Maturi et al. (2023)
#     https://ui.adsabs.harvard.edu/abs/2023A%26A...678A.145M
#
# Entries list:
#  1  SURVEY                          survey name
#  2  NAME                            object name
#  3  ID                              unique identification number of the cluster
#  4  IDAMICO                         AMICO identification number
#  5  RA                [deg]         position in the sky: x direction (R.A)
#  6  DEC               [deg]         position in the sky: y direction (Dec)
#  7  Z                 [redshift]    AMICO redshift
#  8  Z_ERR             [redhisft]    1σ uncertainty of AMICO redshift
#  9  Z_PROB            [redshift]    redshift based on AMICO membership
#  10 Z_PROB_ERR        [redshift]    1σ uncertainty based on AMICO membership
#  11 Z_SPEC            [redshift]    spectroscopic redshift (when available)
#  12 N_SPEC                          number of members with spectroscopic redshift
#  13 SN                              signal-to-noise ratio of AMP; noise = background + cluster
#  14 MSKFRC                          fraction of the cluster inaccessible because of mask
#  15 R_MEDIAN          [deg]         median separation of galaxies with P > 50%
#  16 R_50              [deg]         radius at which \int_0^r P(r) / \int_0^inf P(r) = 0.5
#  17 RICH                            apparent richness based on the filter formalism
#  18 AMP                             signal amplitude
#  19 AMP_ERR                         1 sigma error on AMP
#  20 LAMBDA                          richness based on membership
#  21 LAMBDA_ERR                      1 sigma error on LAMBDA_ERR
#  22 LAMBDA_STAR                     richness based on membership and mr < m∗ + 1.5 and r < rvir
#  23 LAMBDA_STAR_ERR                 1 sigma error on LAMBDA_STAR
#  24 LAMBDA_MSTAR      [10^12 Msun]  total stellar mass based on membership and log10(M∗) > 9.5
#  25 LAMBDA_MSTAR_ERR  [10^12 Msun]  1σ error on LAMBDA_MSTAR
#  26 MASS_AX           [10^13 Msun]  mass based on the amplitude and the X-ray scaling relation
#  27 MASS_AX_ERR       [10^13 Msun]  error of MASS_AX
#  28 MASS_X            [10^13 Msun]  mass based on X-rays
#  29 MASS_X_ERR        [10^13 Msun]  1σ error on MASS_X
#  30 L_X               [10^42erg/s]  X-ray luminosity
#  31 L_X_ERR           [10^42erg/s]  1σ error on L_X
#  32 SN_X                            signal-to-noise ratio of the X-ray flux
#  33 ID_BGG1                         identification number of the BGG galaxy, first choice
#  34 ID_BGG2                         identification number of the BGG galaxy, second choice