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* configs: Clean up importsAaron LI2017-08-012-3/+2
| | | | Signed-off-by: Aaron LI <aly@aaronly.me>
* configs: Default logging to INFO; remove a obsolete config optionAaron LI2017-08-012-6/+1
| | | | Signed-off-by: Aaron LI <aly@aaronly.me>
* clusters: Add config "halos_dumpfile" and dump simulate halos dataAaron LI2017-08-012-1/+12
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* utils/io.py: Add functions "pickle_dump()" and "pickle_load()"Aaron LI2017-08-011-0/+31
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* utils/io.py: Split out "_create_dir()" and "_check_existence()"Aaron LI2017-08-011-12/+31
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* clusters/halo.py: Finished brief simulation descriptionAaron LI2017-08-011-3/+13
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* clusters: Fix several small issues on wrong variable namesAaron LI2017-07-313-7/+8
| | | | | | Also update logging message for RadioHalo a bit. Signed-off-by: Aaron LI <aly@aaronly.me>
* Fix several small issues; Also update PSFormalism a bitAaron LI2017-07-312-5/+11
| | | | Signed-off-by: Aaron LI <aly@aaronly.me>
* docs: Add example NumPy document fileAaron LI2017-07-311-0/+323
| | | | Signed-off-by: Aaron LI <aly@aaronly.me>
* docs: Add sample Makefile and conf.pyAaron LI2017-07-312-0/+395
| | | | Signed-off-by: Aaron LI <aly@aaronly.me>
* clusters/main.py: Use PSFormalism to simulate cluster catalogAaron LI2017-07-311-13/+11
| | | | Signed-off-by: Aaron LI <aly@aaronly.me>
* clusters: Add psformalism.py to simulate cluster catalogAaron LI2017-07-312-2/+241
| | | | | | Also updated configuration options. Signed-off-by: Aaron LI <aly@aaronly.me>
* utils/cosmology.py: Add "dVc()": differential comoving volumeAaron LI2017-07-311-0/+8
| | | | Signed-off-by: Aaron LI <aly@aaronly.me>
* utils: Add interpolate.py with "bilinear()" functionAaron LI2017-07-311-0/+42
| | | | Signed-off-by: Aaron LI <aly@aaronly.me>
* cosmology: Avoid the circular importing issueAaron LI2017-07-313-8/+2
| | | | Signed-off-by: Aaron LI <aly@aaronly.me>
* Add the new module `fg21sim.share` missing from the last commit!Aaron LI2017-07-311-0/+32
| | | | Signed-off-by: Aaron LI <aly@aaronly.me>
* Add `fg21sim.share` module to hold globally shared "CONFIGS" & "COSMO"Aaron LI2017-07-3117-23/+16
| | | | Signed-off-by: Aaron LI <aly@aaronly.me>
* clusters/main.py: Add method "_simulate_halos()"Aaron LI2017-07-311-0/+43
| | | | | | | This method simulates the radio halo properties for each cluster with a recent major merger. Signed-off-by: Aaron LI <aly@aaronly.me>
* clusters/halo.py: Add description for "time_crossing" propertyAaron LI2017-07-311-0/+6
| | | | Signed-off-by: Aaron LI <aly@aaronly.me>
* Update references a bitAaron LI2017-07-312-38/+34
| | | | Signed-off-by: Aaron LI <aly@aaronly.me>
* cluster/halo.py: Add method "calc_brightness_mean()"Aaron LI2017-07-301-0/+48
| | | | Signed-off-by: Aaron LI <aly@aaronly.me>
* clusters/halo.py: Add property "angular_radius" (unit: [arcsec])Aaron LI2017-07-302-0/+12
| | | | Signed-off-by: Aaron LI <aly@aaronly.me>
* clusters/emission.py: Remove methods and clean up parametersAaron LI2017-07-291-78/+2
| | | | | | | | * Methods "power()", "flux()" already moved to "halo.py"; * Method "brightness()" will also be moved over there; * Clean up thus unused parameters "z" and "radius", as well as imports. Signed-off-by: Aaron LI <aly@aaronly.me>
* clusters/halo.py: Add methods "calc_power()" and "calc_flux()"Aaron LI2017-07-291-0/+50
| | | | | | | Calculate the synchrotron power (a.k.a. specific luminosity) and flux density from the emissivity for the halo. Signed-off-by: Aaron LI <aly@aaronly.me>
* clusters/halo.py: Add method "calc_emissivity()"Aaron LI2017-07-291-6/+37
| | | | | | | This method invokes ``SynchrotronEmission`` to calculate the synchrotron emissivity at specified frequencies for the derived electron spectrum. Signed-off-by: Aaron LI <aly@aaronly.me>
* clusters/halo.py: Add property "volume" (unit: [cm^3])Aaron LI2017-07-291-0/+9
| | | | Signed-off-by: Aaron LI <aly@aaronly.me>
* utils/units.py: Add several units conversionsAaron LI2017-07-291-0/+4
| | | | Signed-off-by: Aaron LI <aly@aaronly.me>
* clusters/emission.py: support calc emissivity at multiple frequenciesAaron LI2017-07-291-17/+27
| | | | Signed-off-by: Aaron LI <aly@aaronly.me>
* clusters/emission.py: Add property "B_gauss"Aaron LI2017-07-291-7/+11
| | | | Signed-off-by: Aaron LI <aly@aaronly.me>
* galactic/freefree: Add "dust_fraction" and "halpha_abs_th" configsAaron LI2017-07-292-10/+18
| | | | Signed-off-by: Aaron LI <aly@aaronly.me>
* galactic/freefree.py: Add method "_calc_halpha_to_freefree()"Aaron LI2017-07-291-14/+24
| | | | Signed-off-by: Aaron LI <aly@aaronly.me>
* galactic/freefree.py: Some cleanupsAaron LI2017-07-291-33/+33
| | | | Signed-off-by: Aaron LI <aly@aaronly.me>
* galactic/freefree: Add config "electron_temperature"Aaron LI2017-07-292-10/+28
| | | | | | Update method "_calc_ratio_a()" to "_calc_factor_a()" Signed-off-by: Aaron LI <aly@aaronly.me>
* clusters/emission.py: Cache kernel function interpolation resultsAaron LI2017-07-271-22/+22
| | | | Signed-off-by: Aaron LI <aly@aaronly.me>
* clusters/configs: Update "beta_turb" default to 1.0Aaron LI2017-07-271-1/+1
| | | | | | | This makes the simulation agree better with observations, e.g., <Jsyn> ~ 1e-42 [erg/s/cm^3/Hz] Signed-off-by: Aaron LI <aly@aaronly.me>
* utils/cosmology.py: age() and redshift() accepts numpy arraysAaron LI2017-07-271-7/+10
| | | | Signed-off-by: Aaron LI <aly@aaronly.me>
* utils/cosmology.py: Update references and commentsAaron LI2017-07-271-36/+66
| | | | Signed-off-by: Aaron LI <aly@aaronly.me>
* clusters/emission.py: Fix units/dimensions problemAaron LI2017-07-261-1/+2
| | | | | | | | | | | NOTE: Since we just substitute ``p`` (electron momentum) for ``γ`` (electron Lorentz factor), i.e., N = int_p n(p) dp = int_γ n(γ) dγ , therefore the coefficient ``sqrt(3) e^3 B / (m c^2)`` does NOT need modification (e.g., multiply an extra ``m c``)! Signed-off-by: Aaron LI <aly@aaronly.me>
* clusters/emission.py: explain more on Larmor frequencyAaron LI2017-07-261-4/+12
| | | | Signed-off-by: Aaron LI <aly@aaronly.me>
* clusters/emission.py: Fix the calling to F(x)Aaron LI2017-07-261-9/+6
| | | | Signed-off-by: Aaron LI <aly@aaronly.me>
* clusters/emission.py: Rewrite emissivity calculationAaron LI2017-07-261-15/+24
| | | | | | | | | | Use 2D grid of (discrete) samples to optimize integration speed, avoiding the more complicated integration w.r.t. functions. WARNING: Current calculation results seems wrong! Signed-off-by: Aaron LI <aly@aaronly.me>
* clusters/emission.py: Update argumentsAaron LI2017-07-261-28/+28
| | | | Signed-off-by: Aaron LI <aly@aaronly.me>
* clusters/emission.py: Rewrite Synchrotron kernel function calculationAaron LI2017-07-261-3/+41
| | | | | | | Use interpolation to optimize the speed as well as to vectorize the function to ease calling. Signed-off-by: Aaron LI <aly@aaronly.me>
* clusters/halo.py: Add property "magnetic_field"Aaron LI2017-07-261-0/+11
| | | | Signed-off-by: Aaron LI <aly@aaronly.me>
* clusters/solver.py: Use multiple data points to fit the power-lawAaron LI2017-07-251-17/+19
| | | | Signed-off-by: Aaron LI <aly@aaronly.me>
* configs: Update [[halos]] sections a bitAaron LI2017-07-251-5/+6
| | | | Signed-off-by: Aaron LI <aly@aaronly.me>
* clusters/halo: Change config "eta_turb" to "beta_turb"Aaron LI2017-07-252-6/+5
| | | | | | | | | | This configuration option "beta_turb" has different meaning as "eta_turb" in [Cassano & Brunetti 2005], though they can both be an indicator for the turbulence acceleration efficiency. Rename this configuration option to make the difference more clear. Signed-off-by: Aaron LI <aly@aaronly.me>
* clusters/helper.py: Fix and replace R_halo vs. R_vir relationAaron LI2017-07-231-11/+12
| | | | Signed-off-by: Aaron LI <aly@aaronly.me>
* clusters/helper.py: Fix a bug in "mass_to_kT()"Aaron LI2017-07-231-2/+2
| | | | Signed-off-by: Aaron LI <aly@aaronly.me>
* clusters/helper.py: Add "density_energy_electron()" functionAaron LI2017-07-231-2/+27
| | | | Signed-off-by: Aaron LI <aly@aaronly.me>
Copyright © 2017-2018 Aaron LI. All Rights Reserved.