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* clusters/main: Adjust log level for _simulate_halo1()Aaron LI2019-02-161-2/+2
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* clusters/main: Minor cleanupsAaron LI2019-02-011-2/+8
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* clusters/helper: Some cleanupsAaron LI2019-01-311-32/+13
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* clusters: Use radius_cluster() accordinglyAaron LI2019-01-313-17/+14
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* clusters/helper: Remove obsolete time_crossing()Aaron LI2019-01-311-31/+0
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* clusters/helper: Add radius_cluster()Aaron LI2019-01-311-0/+19
| | | | Ignore the cosmic evolution, keeping the radio halo modeling simple.
* clusters/main: Skip drawing ingenuine halosAaron LI2019-01-301-3/+3
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* clusters/main: Also calculate spectral index and acceleration factorAaron LI2019-01-301-7/+22
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* clusters/main: Add 'genuine' property for halosAaron LI2019-01-302-1/+13
| | | | Configuration option 'genuine_threshold' is added together.
* clusters: Minor cleanups (rename 'comp' to 'sec')Aaron LI2019-01-303-47/+49
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* clusters/main: Improve keys handling in _save_halos_data()Aaron LI2019-01-301-3/+2
| | | | This also fixes the issue when try to remove a non-existent key.
* utils/analyze: Add countdist() functionAaron LI2019-01-301-8/+16
| | | | Modified from the original countdist_integrated().
* clusters/psformalism: Count for dark matter fraction for M_minAaron LI2019-01-292-6/+8
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* clusters/halo: Add options bolo_freq_{min,max,num}Aaron LI2019-01-293-3/+18
| | | | Update the default bolometric frequency band to: 10 MHz -- 100 GHz.
* clusters/helper: Get rid of CONFIGSAaron LI2019-01-291-37/+7
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* clusters/formation: Add show() methodAaron LI2019-01-291-1/+9
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* clusters/formation: Move history() to mergertree.get_history()Aaron LI2019-01-292-30/+46
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* clusters/main: Do not require "age" in _simulate_mergers()Aaron LI2019-01-291-4/+3
| | | | Thus _simulate_mergers() can be called without _process_catalog().
* utils/healpix: Minor cleanupsAaron LI2019-01-291-22/+36
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* Use UTC time instead of local timeAaron LI2019-01-293-22/+17
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* clusters/formation: Implement history() methodAaron LI2019-01-291-16/+36
| | | | | | | Compared to the original mergers() method, this method extracts all formation history (i.e., both mergers and accretions). The mergers() method is now simply wraps on the history() method.
* clusters/mergertree: Tweak format of show_mtree() a bitAaron LI2019-01-281-3/+3
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* clusters/megertree: Minor cleanupsAaron LI2019-01-281-7/+9
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* clusters/halo: Do not rescale density in _adjust_spectrum()Aaron LI2019-01-281-5/+0
| | | | | | Since there is continuous electron injection, the electron density may keep increasing. Therefore, it's bad to rescale the density to match the beginning value.
* configs/manager: Minor cleanupsAaron LI2019-01-281-23/+15
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* clusters/main: Minor cleanupsAaron LI2019-01-281-11/+11
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* clusters/main: Fix column names due to previous renamingAaron LI2019-01-281-3/+2
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* clusters/main: Fix calling of magnetic_field() and kT_cluster()Aaron LI2019-01-281-3/+9
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* utils/analyze: Add logfit()Aaron LI2019-01-281-2/+27
| | | | This function helps fit the index of a scaling relation.
* clusters/main: Update spectrum fields and factor_acc calculationAaron LI2019-01-281-3/+5
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* clusters/halo: calc_acc_factor() accepts the fiducial spectrumAaron LI2019-01-281-3/+7
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* clusters/halo: Fix minor errors along the refactoringAaron LI2019-01-271-5/+4
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* configs/spec: Tweak gamma_max and gamma_npAaron LI2019-01-271-3/+3
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* clusters/halo: Tweak radius_turb() calculationAaron LI2019-01-271-4/+3
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* clusters/main: Calculate acceleration factorAaron LI2019-01-271-0/+2
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* clusters/halo: Rewrite is_genuine() to be calc_acc_factor()Aaron LI2019-01-272-23/+10
| | | | | | | 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".
* clusters/emission: Add calc_emissivity_bolo()Aaron LI2019-01-271-6/+33
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* clusters/halo: Delete the RadioHalo wrapper classAaron LI2019-01-271-92/+0
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* clusters/halo: Implement calc_electron_spectrum() for multiple mergersAaron LI2019-01-271-0/+118
| | | | | | | For a cluster with multiple mergers, each merger has a different turbulence radius, so the accelerated spectrum needs appropriate adjustment to take the (may be significant) variation of turbulence radius into account.
* clusters/helper: Add simple density_number_electron()Aaron LI2019-01-271-0/+8
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* clusters/halo: Implement radius_turb_eff() methodAaron LI2019-01-271-0/+27
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* clusters/halo: Add 'radius_turb_max' propertyAaron LI2019-01-271-2/+10
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* clusters/halo: Tweak {duration,velocity}_turb()Aaron LI2019-01-261-8/+7
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* clusters/main: Adjust against halo radiusAaron LI2019-01-261-4/+3
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* clusters/halo: Reimplement the 'radius' propertyAaron LI2019-01-261-6/+11
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* clusters/halo: Reorder radius_{strip,turb}()Aaron LI2019-01-261-35/+35
| | | | | Rename radius_stripping() to radius_strip() and radius_turbulence() to radius_turb().
* clusters/halo: Clean up mass_main() methodAaron LI2019-01-261-12/+3
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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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