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* clusters/halo: Add radius_stripping() methodAaron LI2018-11-081-3/+13
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* README: Clean up and improve the installationAaron LI2018-11-081-14/+10
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* README: Fix style and clean up a bitAaron LI2018-11-081-15/+7
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* docs/guide: Remove the old outdated test configAaron LI2018-11-082-46/+0
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* docs/guide: Update to refer to the right config.specAaron LI2018-11-082-496/+2
| | | | Delete the old outdated one.
* clusters/halo: Apply option 'f_radius' to derive halo radiusAaron LI2018-11-082-6/+5
| | | | The config option 'f_radius' is renamed from the old 'f_lturb'.
* clusters/halo: New formula for radius_turbulence()Aaron LI2018-11-081-6/+12
| | | | | | | | Calculate the radius of the turbulence region as the mean of the stripping radius of the in-falling sub-cluster and the core radius of the main cluster. Also make the 't' parameter mandatory.
* clusters/halo: Add and use 'f_rc' and 'beta' optionsAaron LI2018-11-082-1/+11
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* clusters/helper: Add f_rc and beta parameters to calc_gas_density_profile()Aaron LI2018-11-081-3/+11
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* clusters/halo: Fix time argument in _velocity_turb()Aaron LI2018-11-021-5/+4
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* clusters/halo: Improve cluster temperature calculationAaron LI2018-11-011-8/+6
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* clusters/halo: Support to check whether halo is genuineAaron LI2018-11-012-0/+40
| | | | | | | 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.
* clusters/halo: Fix the 'lru_cache' usageAaron LI2018-10-311-2/+2
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* PEP8 fixAaron LI2018-10-3110-26/+31
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* bin/get-healpix-path: Check outfile existence earlyAaron LI2018-10-311-6/+13
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* configs/manager: Fix the loading of config specAaron LI2018-10-311-2/+1
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* bin/get-healpix-patch: Get HEALPix ordering for reprojectionAaron LI2018-10-311-2/+9
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* clusters/halo: Support to calculate the fiducial electron spectrumAaron LI2018-10-311-7/+20
| | | | | | | The fiducial electron spectrum is the one that is derived with the turbulent acceleration turned off. It can be used to determine whether the acceleration is indeed effective for one cluster and then further determine whether the radio halo is formed/observable.
* Remove the empty testsAaron LI2018-10-315-78/+4
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* clusters/halo: Simplify calc_electron_spectrum()Aaron LI2018-10-311-49/+6
| | | | | | | | Get rid of the 'electron_spec' property and the set_electron_spectrum() function. Simplify the calc_electron_spectrum() by removing the step adjustment. Other minor cleanups.
* clusters/halo: Rework the way to disable turbulent accelerationAaron LI2018-10-311-16/+13
| | | | | | Introduce a new property '_acceleration_disabled' to control whether the turbulent acceleration is disabled. With this new property, improve the code to derive the initial electron spectrum.
* clusters/halo: Use _is_turb_active() in fp_advection()Aaron LI2018-10-311-14/+6
| | | | Some other minor cleanups.
* 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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* doc: Update template data informationAaron LI2018-10-311-15/+15
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* data: Update manifestAaron LI2018-10-312-32/+32
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* data: Bundle the template data with this repoAaron LI2018-10-315-0/+307
| | | | | | | | * GalacticSNRs_Green2014.csv * Halpha_fwhm06_ns1024.fits.xz * SFD_i100_ns1024.fits.xz * haslam408_dsds_Remazeilles2014_ns512.fits.xz * synchrotron_specind2_ns512.fits.xz
* Enable LFS for .fits and .fits.xzAaron LI2018-10-311-0/+2
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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 LI2018-10-303-41/+17
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* Deprecate the pointsource component (2)Aaron LI2018-10-302-51/+1
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* Deprecate the pointsource componentAaron LI2018-10-302-15/+1
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* configs: Merge config specs into one single fileAaron LI2018-10-305-264/+235
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* README: Tweak the installation steps a bitAaron LI2018-10-301-4/+5
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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.
* utils/units: Add J2erg and erg2JAaron LI2018-10-261-0/+2
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* 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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* docs/guide: Explain the sim_interferometer config fileAaron LI2018-08-161-0/+3
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* docs/guide: Add data analysis sectionAaron LI2018-08-161-1/+19
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* docs/guide: Improve observation simulationAaron LI2018-08-161-10/+58
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* Update docs/guide with observation simulation infoAaron LI2018-08-161-0/+26
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* Update docs/guide with sky patch extraction and point sources simulationAaron LI2018-08-161-0/+31
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Copyright © 2017-2018 Aaron LI. All Rights Reserved.