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-rw-r--r--fg21sim/configs/20-extragalactic.conf.spec14
1 files changed, 10 insertions, 4 deletions
diff --git a/fg21sim/configs/20-extragalactic.conf.spec b/fg21sim/configs/20-extragalactic.conf.spec
index ea6479f..042a808 100644
--- a/fg21sim/configs/20-extragalactic.conf.spec
+++ b/fg21sim/configs/20-extragalactic.conf.spec
@@ -108,10 +108,6 @@
# 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
@@ -119,6 +115,16 @@
# Unit: [Gyr]
tau_merger = float(default=2.0, min=1.0, max=5.0)
+ # 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)
+
+ # Whether to use the maximum merger event (i.e., biggest mass of the
+ # sub cluster) within the above ``tau_merger`` timescale to simulate the
+ # subsequent radio halo simulation? Otherwise only the most recent major
+ # merger event will be used.
+ use_max_merger = boolean(default=False)
+
# The fraction of the magnetic field energy density w.r.t. the ICM
# thermal energy density, which is used to determine the mean magnetic
# field strength within the ICM and is also assumed to be uniform.