#************************************************************************************************************
# CLUMPY v3.0 formatted: 
# -------------------------
#
# The list below is the working list of CLUMPY DM haloes
# N.B.: the parameters for the Galactic halo must be given in clumpy_params.txt
#
# Format: 
#  - a line starting with # (or a blank line) is discarded
#  - Name: name of your object
#  - Type: DSPH, CLUSTER, or GALAXY (for external galaxies)
#  - Position: Given in galactic coordinates (l,b)
#  - d: distance given as comoving line-of-sight distance, d_c
#  - z: distance given as redshift. Either d or z must be set to -1
#  - Rdelta: outer bound of the halo
#  - DM DISTRIBUTION (RHO_TOT): structural parameters for the total DM distribution (see profile.h)
#  - Last 7 parameters for triaxiality are optional
#
# N.B.: 
#  1. A DM shape is always defined by a DM family (gENUM_PROFILE) 
#     and three shape parameters (#1 #2 #3). Set unused parameters to -1
#  2. Substructure properties must be set in clumpy_params.txt for each
#     object type (parameters gType_XXX)
#  3. Rdelta, rs, rhos = rho(rs) have to be provided in comoving coordinates
#
#*********************************************************************************************************************************************************#
#                  [OBJECT LOCATION AND SIZE]                |             DM DISTRIBUTION (RHO_TOT)                      [TRIAXIALITY]                   #
# Name           Type      l       b      d     z   Rdelta   |     rhos       rs     prof.   #1   #2   #3       IsTriaxial  a   b   c   rot1  rot2  rot3  #
#  -               -     [deg]   [deg]  [kpc]   -    [kpc]   |  [Msol/kpc3]  [kpc]  [enum]    -    -    -           -       -   -   -   [deg] [deg] [deg] #
#*********************************************************************************************************************************************************#

Coma_ACO1656    CLUSTER 58.0791 87.9577  -1  0.0234  2.3e3        1.61e5      609.   kZHAO   1.0 3.0  1.0  # after Sanchez-Conde et al. (2011)