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* | utils/units.py: add "rad2arcmin" and some cleanup/simplifications | Aaron LI | 2017-10-18 | 1 | -16/+20 | |
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* | utils/analyze.py: countdist_integrated(): Add xmin and xmax param. | Aaron LI | 2017-10-18 | 1 | -2/+15 | |
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* | clusters: More regular shape for radio halos | Aaron LI | 2017-10-16 | 1 | -6/+5 | |
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* | configs: remove "filemode" option | Aaron LI | 2017-10-16 | 2 | -6/+2 | |
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* | clusters: Update the documents/comments a b it | Aaron LI | 2017-10-14 | 2 | -11/+6 | |
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* | clusters/solver.py: Add FokkerPlanckTests with 3 cases | Aaron LI | 2017-10-12 | 1 | -9/+158 | |
| | | | | | | | | The FokkerPlanckSolver is validated with all the 3 test cases! References: * Park & Petrosian 1996, ApJS, 103, 255 * Donnert & Brunetti 2014, MNRAS, 443, 3564 | |||||
* | clusters/solver.py: significantly improve fix_boundary() | Aaron LI | 2017-10-12 | 1 | -10/+30 | |
| | | | | Also suggest that ``buffer_np`` be specified to 5%-10% of ``x_np``. | |||||
* | clusters/solver.py: Small tweaks | Aaron LI | 2017-10-07 | 1 | -8/+6 | |
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* | clusters/solver.py: Adjust parameter tc,uc orders | Aaron LI | 2017-10-06 | 1 | -10/+7 | |
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* | clusters/solver.py: Stop calc. at "tstop" by adding "tstep" parameter | Aaron LI | 2017-10-06 | 1 | -12/+19 | |
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* | clusters/solver.py: Update comments/references/descriptions etc. | Aaron LI | 2017-10-06 | 1 | -25/+31 | |
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* | clusters/psformalism.py: Rewrite sample_z_m() method | Aaron LI | 2017-10-04 | 2 | -38/+54 | |
| | | | | | Also update clusters/main.py to calculate the halo mass distributions before sampling the mass and redshifts for clusters. | |||||
* | clusters: Use "hmf" to calculate halo mass functions/distributions | Aaron LI | 2017-10-04 | 6 | -82/+230 | |
| | | | | | | | | | | | | * New dependency "hmf" (halo mass functions) module * Calculate halo mass distributions/functions (dndlnm) with respect to masses and redshifts, instead of use the previous data file ("ps_data") * New section "[extragalactic][psformalism]" in configurations * New functions to write and read the dndlnm data TODO: * update the method to sample (mass, redshift) for clusters from the dndlnm data | |||||
* | configs/manager.py: Add missing cosmology parameters | Aaron LI | 2017-10-04 | 1 | -0/+2 | |
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* | utils/cosmology.py: Add parameter Tcmb0 [K] | Aaron LI | 2017-10-04 | 2 | -6/+13 | |
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* | utils/units.py: Add "K2eV" and "K2keV" | Aaron LI | 2017-10-04 | 1 | -0/+2 | |
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* | configs: Use lower case for logging levels | Aaron LI | 2017-10-04 | 7 | -24/+18 | |
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* | bin/fg21sim-download-data: Update description | Aaron LI | 2017-10-04 | 1 | -2/+3 | |
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* | utils/cosmology: Add scalar spectral index "ns" | Aaron LI | 2017-10-04 | 2 | -4/+8 | |
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* | configs: Clean up some comments | Aaron LI | 2017-10-03 | 2 | -14/+0 | |
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* | utils/cosmology.py: Add methods Dc() and Dc_to_redshift() | Aaron LI | 2017-10-02 | 1 | -0/+48 | |
| | | | | | | * Dc(): simple wrapper on astropy cosmology's comoving_distance() * Dc_to_redshift(): determine the redshift w.r.t. the input comoving distances using interpolation. | |||||
* | clusters/psformalism.py: Improve catalog comments | Aaron LI | 2017-10-02 | 1 | -4/+7 | |
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* | Bump version to 0.6.1v0.6.1 | Aaron LI | 2017-09-26 | 1 | -1/+1 | |
| | | | | | | Component "extragalactic/clusters" is tuned and tested to work. Start working on radio relics from galaxy clusters. | |||||
* | utils/units.py: Add eV and keV to temperature conversions | Aaron LI | 2017-09-26 | 1 | -0/+3 | |
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* | clusters/emission: Assume electron pitch angle be pi/2 | Aaron LI | 2017-09-20 | 1 | -23/+17 | |
| | | | | And some cleanup and small changes | |||||
* | clusters/emission: Rewrite synchrotron kernel function | Aaron LI | 2017-09-20 | 1 | -9/+38 | |
| | | | | | | | | | | | Add asymptotic functions to calculate the values beyond the interpolation bounds (e.g., <1e-3 and >10), otherwise, the calculated synchrotron emissivity is overestimated at the higher frequencies. By rewrite this synchrotron kernel function, the calculated results is consistent with the theoretical/analytical results, e.g., the synchrotron radiation of a population of electrons of power-law index n is also a power-law with index (n-1)/2. | |||||
* | clusters: Add option "use_output_catalog" to continue halo simulation | Aaron LI | 2017-09-03 | 3 | -4/+36 | |
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* | configs: Update option descriptions; also tweak checkers a bit | Aaron LI | 2017-09-03 | 2 | -7/+12 | |
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* | utils/io.py: Add function "csv_to_dataframe()" to support CSV comments | Aaron LI | 2017-09-03 | 1 | -2/+35 | |
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* | clusters: Add config option "boost" | Aaron LI | 2017-09-01 | 2 | -2/+10 | |
| | | | | | | | NOTE: The cluster number (especially the bright ones) may be rather small within a sky patch. This ``boost`` config option increase the expected cluster number by a specified times, for better testing purpose. | |||||
* | configs/logging: print time only, without date | Aaron LI | 2017-09-01 | 1 | -1/+1 | |
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* | Update time cost report; Also fix a variable name error | Aaron LI | 2017-09-01 | 2 | -6/+6 | |
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* | Update "Fnu_to_Tb_fast()" to "Fnu_to_Tb()" | Aaron LI | 2017-09-01 | 7 | -11/+11 | |
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* | utils/convert.py: Remove the slow, astropy.units based functions | Aaron LI | 2017-09-01 | 1 | -64/+24 | |
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* | utils/draw.py: Replace "ellipse()" with the `skiimage' version | Aaron LI | 2017-08-31 | 1 | -27/+96 | |
| | | | | | | | Also do not use Numba JIT here. Credit: scikit-image - skimage/draw/draw.py https://github.com/scikit-image/scikit-image/blob/master/skimage/draw/draw.py | |||||
* | configs: Update clusters simulation parameters | Aaron LI | 2017-08-31 | 1 | -4/+4 | |
| | | | | | | | Carried many simulation tests to determine the best parameters, by comparing with the integrated counts distribution (i.e., halo luminosity function) reported in previous works (Cassano2006, Cassano2012, and Ensslin2002). | |||||
* | utils: Add analyze.py with function "countsdist_integrate()" | Aaron LI | 2017-08-30 | 1 | -0/+66 | |
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* | clusters/psformalism: Remove config "f_darkmatter" | Aaron LI | 2017-08-29 | 3 | -6/+12 | |
| | | | | Use "1 - baryon_fraction = 1 - Ob0/Om0" to replace "f_darkmatter". | |||||
* | configs: Fix checker for "extragalactic/clusters" section | Aaron LI | 2017-08-29 | 1 | -1/+1 | |
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* | convert.py: do not use Numba JIT | Aaron LI | 2017-08-29 | 1 | -14/+8 | |
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* | configs: update "frequencies" property to be a numpy array | Aaron LI | 2017-08-28 | 1 | -6/+7 | |
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* | Delete obsolete script: bin/fg21sim-download-cluster-data | Aaron LI | 2017-08-27 | 1 | -163/+0 | |
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* | Bump version to 0.6.0, prepare for a new releasev0.6.0 | Aaron LI | 2017-08-27 | 1 | -5/+5 | |
| | | | | | | | Since last release (0.4.2), too many things have changed ... so skip 0.5.x to emphasis the big update ... Also update the URL to the GitHub one. | |||||
* | configs: Update default values of some options | Aaron LI | 2017-08-27 | 2 | -7/+9 | |
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* | Update README.rst | Aaron LI | 2017-08-27 | 1 | -11/+10 | |
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* | configs: Use "utf-8" encoding to allow unicode in config files | Aaron LI | 2017-08-27 | 1 | -6/+11 | |
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* | freefree.py: Fix bug: "comp" -> "compID" | Aaron LI | 2017-08-27 | 1 | -1/+1 | |
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* | configs: Delete obsolete checks on "{halphamap,dustmap}_unit" | Aaron LI | 2017-08-27 | 1 | -4/+0 | |
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* | configs: synchrotron: default to not add smallscales | Aaron LI | 2017-08-27 | 1 | -3/+5 | |
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* | freefree.py: Remove units of "halphamap" and "dustmap" | Aaron LI | 2017-08-27 | 2 | -19/+4 | |
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