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* clusters/halo: Add time argument to radius_turbulence()Aaron LI2018-10-311-10/+8
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* clusters/halo: Add time argument to _velocity_turb()Aaron LI2018-10-311-10/+10
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* clusters/halo: Add time argument to _gas_density_profile_t()Aaron LI2018-10-311-4/+6
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* clusters/halo: Rename 'injection_radius' to 'radius_turbulence'Aaron LI2018-10-301-16/+16
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* clusters/halo: Update time_turbulence() calculationAaron LI2018-10-302-28/+10
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* clusters/helper: Remove the obsolete fmass_nfw()Aaron LI2018-10-301-26/+0
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* clusters/halo: Update turbulence velocity calculationAaron LI2018-10-301-26/+40
| | | | | | | | Adopt the same beta-model for the gas density profile to calculate the gas/baryon mass within the turbulence region (<R_turb). Meanwhile, change the '_velocity_turb()` method to a property without depending on the time, to further simplify the model a bit.
* clusters/halo: Update calculations of injection and halo radiusAaron LI2018-10-302-36/+13
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* Deprecate the pointsource component (2)Aaron LI2018-10-301-2/+1
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* clusters/help: Add radius_stripping()Aaron LI2018-10-261-6/+73
| | | | | This function calculates the stripping radius of the sub-cluster when it falling through the main cluster.
* clusters/halo: Improve descriptions and commentsAaron LI2018-10-252-20/+16
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* clusters/halo: Change _merger() to accept time to simplify its usageAaron LI2018-10-251-12/+12
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* clusters/halo: Simplify the code a bitAaron LI2018-10-251-18/+8
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* clusters/halo: Fix a wrong variable in a logging messageAaron LI2018-10-251-6/+4
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* clusters/main: Minor improvementsAaron LI2018-10-241-13/+11
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* clusters: Add parameter felong_minAaron LI2018-05-221-3/+3
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* clusters: Fix cluster distribution calculation about massAaron LI2018-05-121-14/+8
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* cluster/formation: Fix merger tree simulation about cluster massAaron LI2018-05-111-24/+22
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* cluster/formation: update zmax default valueAaron LI2018-03-081-2/+2
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* cluster/formation: merger tree simulation should use dark matter massesAaron LI2018-03-031-41/+34
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* clusters: Fix dropout handlingAaron LI2018-02-031-8/+7
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* clusters: improve dropout handlingAaron LI2018-01-281-10/+26
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* clusters: calculate/save cosmic (~cluster) age to catalog & halos dataAaron LI2018-01-221-1/+6
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* clusters: coerce to plain list for concatenationAaron LI2018-01-221-4/+8
| | | | | The "merger_mass1", "merger_mass2", "merger_z", and "merger_age" may be NumPy arrays, e.g., the catalog data are manually modified.
* clusters/halo: most consistent turbulent acceleration and time calculationsAaron LI2018-01-212-3/+3
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* clusters/halo: simplify energy loss calculationsAaron LI2018-01-211-27/+14
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* clusters/emission: improve description symbols :-)Aaron LI2018-01-211-4/+4
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* clusters: minor updatesAaron LI2018-01-161-5/+4
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* clusters/main: minor cleanupsAaron LI2018-01-111-10/+8
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* clusters/halo: fix _is_turb_active() bool conditionAaron LI2018-01-061-2/+2
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* clusters: fix string formatting in _simulate_halos()Aaron LI2018-01-051-1/+1
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* clusters: small cleanupsAaron LI2018-01-052-12/+18
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* clusters/halo: fix self.time_step errorAaron LI2018-01-051-4/+4
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* clusters/halo: fix _merger_time() error when t < age_beginAaron LI2018-01-051-2/+7
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* clusters: update _simulate_halos() with new halo propertiesAaron LI2018-01-051-11/+9
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* clusters/halo: calculate several time-averaged propertiesAaron LI2018-01-051-0/+54
| | | | | | | * time_turbulence_avg * mach_turbulence_avg * tau_acceleration_avg * time_acceleration_fraction
* clusters/halo: move tau_max and time dependence to tau_acceleration()Aaron LI2018-01-051-27/+27
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* clusters/halo: add _is_turb_active(), update _velocity_turb() etc.Aaron LI2018-01-051-12/+29
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* clusters/halo: update turbulence acceleration calc. with _merger_time()Aaron LI2018-01-051-28/+20
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* clusters/halo: add _merger_time() and mass_sub() methodsAaron LI2018-01-051-0/+31
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* clusters/halo: refactor tau_acceleration() to help RadioHaloAMAaron LI2018-01-042-25/+39
| | | | | Change "tau_acceleration" from a attribute to a method with the time parameter, and then simplify "fp_diffusion()" method.
* clusters/halo: Add preliminary RadioHaloAM based on RadioHaloAaron LI2018-01-042-12/+115
| | | | | The RadioHaloAM class is intended to account for all merger events, and there are a lot of methods to be implemented.
* clusters/halo: small updates and some cleanupsAaron LI2018-01-042-60/+45
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* clusters/halo: minor cleanupsAaron LI2018-01-031-14/+15
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* clusters/halo: change "age_merger" to "age_begin"Aaron LI2018-01-031-23/+26
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* clusters/halo: update radius_halo() calculationAaron LI2018-01-032-15/+7
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* clusters/halo: delete radius_virial_{main,sub} and kT_sub propertiesAaron LI2018-01-032-20/+0
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* clusters: Fix catalog data to CSV saveAaron LI2018-01-031-1/+3
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* clusters: update to to use the new HaloEmission in _calc_halos_emission()Aaron LI2018-01-031-13/+9
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* clusters/halo: split emissivity/power/flux calculations into HaloEmissionAaron LI2018-01-032-175/+200
| | | | | Add emission.HaloEmission class to calculate halo emissivity, power, flux, brightness etc.
Copyright © 2017-2018 Aaron LI. All Rights Reserved.