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* clusters/halo: Tune parameters kT_out and radius_indexAaron LI2019-03-011-2/+2
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* clusters/halo: Tune parametersAaron LI2019-02-271-7/+7
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* configs/manager: Add update() methodAaron LI2019-02-271-0/+4
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* configs/manager: Various more cleanupsAaron LI2019-02-271-21/+11
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* configs/manager: Clean up save()Aaron LI2019-02-271-11/+7
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* Several minor cleanupsAaron LI2019-02-271-4/+4
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* clusters/main: Implement _identify_halos() to determine genuine halosAaron LI2019-02-271-0/+5
| | | | | New configuration options 'extragalactic/halos/genuine_{emfacc,index}_th' are added to set the thresholds.
* clusters/halo: calc_acc_factor() no longer usedAaron LI2019-02-271-8/+0
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* clusters/main: Do not calculate acceleration factor and genuineAaron LI2019-02-271-4/+0
| | | | | A new method to determine the formation/genuineness of a radio halo will be used.
* configs/spec: Reorder options to be clearerAaron LI2019-02-271-16/+14
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* clusters/halo: Tune parameters based on various testsAaron LI2019-02-271-8/+8
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* clusters/main: Allow to disable map generationAaron LI2019-02-261-0/+4
| | | | | New configuration option 'extragalactic/clusters/make_maps' is added to control whether or not to make and save the simulated maps.
* configs/spec: Adjust some default values and minor tweaksAaron LI2019-02-261-7/+15
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* clusters/halo: Add velocity_turb_base() methodAaron LI2019-02-211-0/+5
| | | | | | | | | | This method calculates the velocity dispersion of the base turbulence, i.e., the turbulence existing in a relaxed system without the merger injection. Add new configuration option 'extragalactic/halos/x_turb' to parameterize the energy fraction of the base turbulence w.r.t. the ICM thernal energy.
* configs/spec: Adjust some min/max values for simplicityAaron LI2019-02-211-5/+5
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* clusters/halo: Further extend the halo radius calculationAaron LI2019-02-181-1/+5
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* clusters/main: Add 'genuine' property for halosAaron LI2019-01-301-0/+4
| | | | Configuration option 'genuine_threshold' is added together.
* clusters/halo: Add options bolo_freq_{min,max,num}Aaron LI2019-01-291-0/+8
| | | | Update the default bolometric frequency band to: 10 MHz -- 100 GHz.
* configs/manager: Minor cleanupsAaron LI2019-01-281-23/+15
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* configs/spec: Tweak gamma_max and gamma_npAaron LI2019-01-271-3/+3
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* clusters/halo: Rewrite is_genuine() to be calc_acc_factor()Aaron LI2019-01-271-7/+0
| | | | | | | Calculate the bolometric emissivity instead of the emissivity at a certain frequency. This should capture the acceleration effect more effectively. In addition, remove the now obsolete config options "fiducial_freq" and "fiducial_factor".
* configs/spec: Various minor tweaksAaron LI2019-01-251-31/+32
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* clusters/halo: Account for mass scaling in tau_acceleration()Aaron LI2019-01-251-0/+4
| | | | Add configuration option "mass_index" to specify the scaling index.
* clusters/halo: Fold parameter "zeta_ins" into "f_acc"Aaron LI2019-01-251-7/+3
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* clusters: Assume equipartition between B field and CRAaron LI2019-01-251-13/+3
| | | | | | Equipartition between the magnetic fields and cosmic rays is assumed, i.e., eta_b == x_cr. Therefore remove "extragalactic/clusters/eta_b" configuration option.
* Minor tweaksAaron LI2019-01-181-3/+3
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* configs/manager: Tweak a bitAaron LI2018-12-221-5/+4
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* clusters/halo: Apply option 'f_radius' to derive halo radiusAaron LI2018-11-081-4/+3
| | | | The config option 'f_radius' is renamed from the old 'f_lturb'.
* clusters/halo: Add and use 'f_rc' and 'beta' optionsAaron LI2018-11-081-0/+7
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* clusters/halo: Support to check whether halo is genuineAaron LI2018-11-011-0/+7
| | | | | | | Add the 'is_genuine()' method to check whether the radio halo is genuine by comparing the flux density to the fiducial value. Two new configuration options (fiducial_freq and fiducial_factor) are added to specify the frequency and limit whether the radio halo is regarded as genuine.
* PEP8 fixAaron LI2018-10-311-2/+2
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* configs/manager: Fix the loading of config specAaron LI2018-10-311-2/+1
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* clusters/halo: Update calculations of injection and halo radiusAaron LI2018-10-301-5/+4
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* Deprecate the pointsource component (2)Aaron LI2018-10-301-49/+0
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* configs: Merge config specs into one single fileAaron LI2018-10-304-263/+234
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* clusters/config: Tune parameter eta_eAaron LI2018-05-221-1/+1
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* clusters: Add parameter felong_minAaron LI2018-05-221-0/+7
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* clusters: Fix cluster distribution calculation about massAaron LI2018-05-121-8/+7
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* clusters/config: tune parameter x_cr; and improve parameter descriptionAaron LI2018-02-031-8/+9
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* clusters/config: tune parameters time_init->1, time_step->0.02Aaron LI2018-01-281-2/+2
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* clusters: minor updatesAaron LI2018-01-161-0/+2
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* configs: adjust default values of "merger_mass_min" and "kT_out"Aaron LI2018-01-051-2/+2
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* clusters: simulate and extract all recent merger eventsAaron LI2018-01-021-10/+0
| | | | Remove the obsolete options: ratio_major, use_max_merger
* clusters: rework the reuse of previously dumped cluster catalogAaron LI2018-01-022-7/+15
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* configs/checkers: add _check_file_existence() and some cleanupsAaron LI2018-01-021-14/+49
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* Minor changesAaron LI2018-01-011-1/+1
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* clusters/halo: Change option "tau_merger" to "time_traceback"Aaron LI2018-01-011-5/+5
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* clusters/halo: Rework the turbulence acceleration timescale calculationAaron LI2017-12-311-2/+14
| | | | | | | | The new method adopted to determine the turbulence acceleration timescale follows [miniati2015] and [pinzke2017], in which the merger-induced turbulence cascades into small scales (and thus accelerate electrons) through the TTD (transit-time damping) mechanism by scattering mainly with the relativistic particles (cosmic-ray protons and electrons).
* clusters/halo: calc turbulence velocity dispersion based on mergerAaron LI2017-12-311-9/+3
| | | | | Also update the description of option "extragalactic/halos/eta_turb" and change its default value to 0.1
* Minor cleanupsAaron LI2017-12-311-10/+17
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