aboutsummaryrefslogtreecommitdiffstats
path: root/fg21sim/configs/20-extragalactic.conf.spec
blob: a48dbeebcf793bbb1a7465f88d8c8f1d5036aa9b (plain)
1
2
3
4
5
6
7
8
9
10
11
12
13
14
15
16
17
18
19
20
21
22
23
24
25
26
27
28
29
30
31
32
33
34
35
36
37
38
39
40
41
42
43
44
45
46
47
48
49
50
51
52
53
54
55
56
57
58
59
60
61
62
63
64
65
66
67
68
69
70
71
72
73
74
75
76
77
78
79
80
81
82
83
84
85
86
87
88
89
90
91
92
93
94
95
96
97
98
99
100
101
102
103
104
105
106
107
108
109
110
111
112
113
114
115
116
117
118
119
120
121
122
123
124
125
126
127
128
129
130
131
132
133
134
135
136
# Configurations for "fg21sim"
# -*- mode: conf -*-
#
# Syntax: `ConfigObj`, https://github.com/DiffSK/configobj
#
# There are various configuration options that specify the input data
# and/or templates required by the simulations, the properties of the input
# data, the output products, as well as some parameters affecting the
# simulation behaviors.
#
# This file contains the options corresponding the extragalactic emission
# components, which currently includes the following components:
# - clusters: halos
# - pointsources


[extragalactic]

  # Extended emissions from the clusters of galaxies
  # The configurations in this ``[[clusters]]`` section may also be
  # used by the following ``[[halos]]`` section.
  [[clusters]]
  # The clusters catalog derived from the Hubble Volume Project (CSV file)
  catalog = string(default=None)
  # Output the effective/inuse clusters catalog data (CSV file)
  catalog_outfile = string(default=None)

  # Minimum mass change of the main cluster to be regarded as a merger
  # event instead of an accretion event.
  # Unit: [Msun]
  merger_mass_min = float(default=1e12, min=1e10, max=1e14)

  # Mass ratio of the main and sub clusters, below which is regarded as
  # a major merger event.
  ratio_major = float(default=3.0, min=1.0, max=10.0)

  # The merger timescale, which roughly describes the duration of the
  # merger-induced disturbance (~2-3 Gyr).  This timescale is much longer
  # the merger crossing time (~1 Gyr), and is also longer than the lifetime
  # of radio halos.
  # Unit: [Gyr]
  tau_merger = float(default=3.0, min=1.0, max=5.0)

  # Magnetic field scaling relation for clusters
  # Reference: Cassano et al. 2012, A&A, 548, A100, Eq.(1)
  #
  # The mean magnetic field assumed
  # Unit: [uG]
  b_mean = float(default=1.9, min=0.1, max=10)
  # The index of the scaling relation
  b_index = float(default=1.5, min=0.0, max=3.0)

  # Resolution for simulating each cluster templates, which are finally
  # mapped to the all-sky HEALPix map if used.
  # Unit: [arcsec]
  resolution = float(default=30.0, min=5.0)

  # Filename prefix for this component
  prefix = string(default="cluster")
  # Whether save this component to disk
  save = boolean(default=True)
  # Output directory to save the simulated results
  output_dir = string(default=None)


  # Emission of giant radio halos from galaxy clusters
  [[halos]]
  # Intensity of the turbulence acceleration.
  beta_turb = float(default=0.3, min=0.1, max=2.0)

  # Ratio of the total energy injected into cosmic-ray electrons during
  # the cluster life to its total thermal energy.
  eta_e = float(default=0.003, min=0.0, max=0.1)

  # Minimum and maximum Lorentz factor (i.e., energy) of the relativistic
  # electron spectrum.
  gamma_min = float(default=1e1)
  gamma_max = float(default=1e5)
  # Number of momentum points/cells for solving the Fokker-Planck
  # equation.
  gamma_np = integer(default=200, min=50)

  # Number of grid points used as the buffer region near the lower
  # boundary, and the value within this buffer region will be fixed to
  # avoid unphysical pile-up of low-energy electrons.
  # Reference: Donnert & Brunetti 2014, MNRAS, 443, 3564, Sec.(3.3)
  buffer_np = integer(default=5, min=0)

  # Time step for solving the Fokker-Planck equation
  # Unit: [Gyr]
  time_step = float(default=0.01, min=1e-5, max=1.0)

  # Index of the power-law spectrum assumed for the injected electrons.
  injection_index = float(default=2.5)


  # Extragalactic point sources
  [[pointsources]]
  # Whether save this point source catelogue to disk
  save = boolean(default=True)
  # Output directory to save the simulated catelogues
  output_dir = string(default="PS_tables")
  # PS components to be simulated
  pscomponents = string_list(default=list())
  # Resolution [arcmin]
  resolution = float(default=0.6, min=0.0)

    [[[starforming]]]
    # Number of samples
    numps = integer(default=1000)
    # Prefix
    prefix = string(default="SF")

    [[[starbursting]]]
    # Number of samples
    numps = integer(default=1000)
    # Prefix
    prefix = string(default="SB")

    [[[radioquiet]]]
    # Number of samples
    numps = integer(default=1000)
    # Prefix
    prefix = string(default="RQ")

    [[[FRI]]]
    # Number of samples
    numps = integer(default=1000)
    # Prefix
    prefix = string(default="FRI")

    [[[FRII]]]
    # Number of samples
    numps = integer(default=1000)
    # Prefix
    prefix = string(default="FRII")