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* clusters/halo: Rewrite _merger_time() to get the effective mergerAaron LI2019-01-261-8/+24
| | | | | If the acceleration durations of multiple mergers overlap, the one with the largest efficiency (i.e., smallest tau_acc) is chosen.
* clusters/halo: Replace "age" with "t" (time)Aaron LI2019-01-261-31/+31
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* clusters/main: Replace "age" with "t" (time)Aaron LI2019-01-261-6/+6
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* clusters/halo: Fold _merger_idx() into _merger_event()Aaron LI2019-01-261-18/+11
| | | | Update _merger_time() accordingly.
* clusters/halo: Move and rename _velocity_turb() to _velocity_turb()Aaron LI2019-01-261-57/+57
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* clusters/halo: Rename _merger() to _merger_event()Aaron LI2019-01-261-4/+4
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* clusters/halo: Remove *_avg and *_fraction methodsAaron LI2019-01-262-54/+0
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* clusters/halo: Use t_merger for duration_turb() and mach_turb()Aaron LI2019-01-261-4/+6
| | | | Rename mach_turbulence() to mach_turb().
* clusters/halo: Simplify tau_acceleration() methodAaron LI2019-01-261-45/+14
| | | | Move the turbulence activity check into the fp_diffusion() method.
* clusters/halo: Some cleanupsAaron LI2019-01-261-28/+15
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* clusters/halo: Use t_merger to be more explicitAaron LI2019-01-261-13/+25
| | | | | Add _validate_t_merger() method to validate the given time to be an merger time.
* clusters/halo: Rename time_turbulence() to duration_turb()Aaron LI2019-01-262-11/+10
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* clusters/halo: Fold _rho_gas_f() into _velocity_turb()Aaron LI2019-01-251-20/+8
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* clusters/halo: Account for mass scaling in tau_acceleration()Aaron LI2019-01-251-0/+18
| | | | Add configuration option "mass_index" to specify the scaling index.
* clusters/halo: Fold parameter "zeta_ins" into "f_acc"Aaron LI2019-01-251-3/+2
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* clusters/halo: Clean up tau_acceleration() methodAaron LI2019-01-251-14/+13
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* clusters: Assume equipartition between B field and CRAaron LI2019-01-252-3/+15
| | | | | | Equipartition between the magnetic fields and cosmic rays is assumed, i.e., eta_b == x_cr. Therefore remove "extragalactic/clusters/eta_b" configuration option.
* clusters/helper: Add plasma_beta() functionAaron LI2019-01-231-0/+26
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* clusters/helper: Do not pass the whole configs to functionsAaron LI2019-01-232-14/+40
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* clusters/helper: Fix a variable error in density_gas()Aaron LI2019-01-221-1/+1
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* clusters/helper: Add radius_overdensity() functionAaron LI2019-01-211-4/+29
| | | | e.g., to calculate R200, R500.
* clusters/helper: Improve density_energy_electron() calculationAaron LI2019-01-211-4/+4
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* clusters/helper: Add density_gas() functionAaron LI2019-01-211-0/+8
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* clusters/halo: Minor cleanupAaron LI2019-01-191-4/+1
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* clusters/halo: Update turbulence velocity dispersion calcuationAaron LI2019-01-181-7/+6
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* clusters/halo: Update time_turbulence() calculationAaron LI2019-01-181-8/+9
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* clusters/helper: Pass beta to helper.radius_stripping()Aaron LI2019-01-182-7/+9
| | | | | * Add 'beta' parameter to radius_stripping() * Pass 'f_rc' and 'beta' to calc_gas_density_profile()
* Minor tweaksAaron LI2019-01-182-4/+5
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* clusters/halo: Update the estimation of radius_turbulence()Aaron LI2019-01-171-4/+8
| | | | | The radius_turbulence is estimated as the stripping radius (r_s) if r_s is larger than the core radius (r_c) of the main cluster, otherwise, r_c.
* clusters/main: Account for baryon fraction in _simulate_mergers()Aaron LI2019-01-171-3/+4
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* clusters/main: Account for baryon fraction in _simulate_catalog()Aaron LI2019-01-172-6/+11
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* clusters/main: Fix _calc_cluster_info()Aaron LI2019-01-171-1/+1
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* clusters/halo: Refactor calc_radius_turb()Aaron LI2019-01-111-14/+37
| | | | | Keep all the calculated properties that can be used to tweak the parameters or to help debug.
* clusters/halo: Implement calc_radius_turb()Aaron LI2019-01-111-0/+36
| | | | | Determine the effective radius of the turbulence region along the whole merging process (i.e., multiple merger events).
* clusters/halo: Add new "RadioHalo" to wrap over RadioHaloAMAaron LI2019-01-101-0/+33
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* clusters/halo: Renamed "RadioHalo" to "RadioHalo1M"Aaron LI2019-01-101-3/+4
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* clusters/halo: Rewrite is_geniune() methodAaron LI2019-01-101-0/+30
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* clusters/main: Update _calc_halos_emission()Aaron LI2019-01-101-2/+2
| | | | Match the updated variable names.
* Bump copyright yearAaron LI2019-01-102-2/+2
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* clusters/main: Update _simulate_halo1()Aaron LI2019-01-101-23/+15
| | | | | Directly merge in the cluster information into the halo information dictionary.
* clusters/main: Rename 'theta' to 'Rvir_angular'Aaron LI2019-01-101-2/+2
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* clusters/halo: Change radius attribute to calc_radius()Aaron LI2019-01-101-20/+1
| | | | Meanwhile remove the angular_radius and volume attributes.
* clusters/main: Calculate DA and theta in _calc_cluster_info()Aaron LI2019-01-101-6/+13
| | | | | Calculate angular diameter distance and angular radius in _calc_cluster_info().
* clusters/halo: Remove is_geniune()Aaron LI2019-01-101-32/+0
| | | | The similar functionality will be implemented in another wrapper class.
* clusters/main: Add _calc_cluster_info()Aaron LI2019-01-102-29/+23
| | | | Move the calculation of Rvir, kT, and B from halo.py to main.py.
* clusters/main: Minor cleanupsAaron LI2019-01-101-3/+3
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* clusters/halo: Set fixed radius for RadioHaloAMAaron LI2018-12-231-2/+14
| | | | | | | Since the halo radius is related to the turbulence injection region size which is further related to the stripping radius, it varies along the cluster growth as mergers happen. Therefore, the finally radio halo radius is determined otherwise and just specified here.
* clusters/halo: Minor tweaksAaron LI2018-12-221-12/+10
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* clusters/halo: Update is_genuine() to return flux factor alsoAaron LI2018-12-221-1/+5
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* clusters/main: Split out _simulate_halo1()Aaron LI2018-12-221-42/+56
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