aboutsummaryrefslogtreecommitdiffstats
Commit message (Collapse)AuthorAgeFilesLines
* halo.py: Fix wrong cosmo.age() usageAaron LI2017-06-251-1/+1
|
* solver.py: Fix coefficients calculation w.r.t. escape termAaron LI2017-06-251-5/+6
|
* solver.py: Add example for TDMAsolver()Aaron LI2017-06-251-0/+16
|
* clusters/solver.py: Split methods bound_w/Wplus/WminusAaron LI2017-06-251-14/+36
| | | | Also change an INFO message to be DEBUG level.
* clusters/solver.py: Fix "fix_boundary()" and remove a warningAaron LI2017-06-251-6/+5
|
* clusters/solver.py: Support escape termAaron LI2017-06-251-5/+12
|
* halo.py: Add argument "n0_e" to method "calc_electron_spectrum()"Aaron LI2017-06-241-4/+10
|
* halo.py: Split out property "_chi_data"Aaron LI2017-06-241-31/+31
|
* halo.py: Add property "pgrid" as same as it is in slover.pyAaron LI2017-06-241-0/+10
|
* halo.py: use age at cluster redshift z0 instead of present dayAaron LI2017-06-241-6/+12
|
* halo.py: Add property "zgrid" as well as config option "zbinsize"Aaron LI2017-06-242-1/+11
|
* Revert "utils/convert.py: Use 'utils.units' module"Aaron LI2017-06-241-7/+6
| | | | | | This reverts commit eb660ae70db40d36418f1e4eb886fd9bb02af1a7. Numba cannot recognize AUC/AC classes, or needs further updates
* clusters/halo.py: calculate electron density default end at z0Aaron LI2017-06-231-10/+12
|
* mergertree.py: axes.hold() is deprecated and it is True by defaultAaron LI2017-06-231-1/+0
|
* halo.py: calculate magnetic field using a scaling relationAaron LI2017-06-232-11/+29
|
* halo.py + formation.py: Add argument z0Aaron LI2017-06-232-7/+18
|
* cosmology: Use default parameters from configurationsAaron LI2017-06-232-1/+7
| | | | Also add configuration option "cosmology/Omegab0".
* emission.py: Add power(), flux(), brightness() methodsAaron LI2017-06-231-25/+111
|
* utils/convert.py: Use 'utils.units' moduleAaron LI2017-06-231-6/+7
|
* utils/units.py: Add "rad2deg" and "k_B"Aaron LI2017-06-231-1/+5
|
* utils/cosmology: Add methods DL() and DA()Aaron LI2017-06-191-0/+14
|
* sky.py: Write PIXELSIZE, RA0, and DEC0 to header for patch skyAaron LI2017-06-191-0/+3
|
* Use keyword "BUNIT" and unit "K"Aaron LI2017-06-135-5/+5
|
* Fix GalaxyClusters importAaron LI2017-06-131-2/+2
|
* configs: Default to disable all foregroundsAaron LI2017-06-131-4/+4
|
* bin/get-healpix-patch: Add argument --smooth and write historyAaron LI2017-06-121-0/+13
|
* sky.py: Fix mkdir when the directory name is emptyAaron LI2017-06-121-2/+2
|
* clusters.py: Fix calculation on size_{major,minor}Aaron LI2017-06-111-15/+20
| | | | | | | | The size_{major,minor} should be the major and minor (not semi-) axes of the cluster halo; but I originally calculated them as the semi-major and semi-minor axes. Also change the units of size_{major,minor} from [deg] to [arcmin].
* galactic/snr.py: Explain size_{major,minor} are diameter valuesAaron LI2017-06-111-4/+6
|
* configs: extragalactic/halos: change "radius_halo" to "radius"Aaron LI2017-06-012-10/+9
|
* clusters: Move units.py and cosmology.py to utilsAaron LI2017-06-015-4/+6
|
* extragalactic/clusters/clusters.py: Trim unused importsAaron LI2017-06-011-2/+0
|
* fg21sim/clusters: Save progress on halo simulationAaron LI2017-06-015-4/+30
|
* clusters/halo.py: Add zbegin & zend parametersAaron LI2017-06-011-3/+37
| | | | | * Add "zbegin" and "zend" parameters to "calculate_electron_spectrum()" * Add more detail docstrings
* Add clusters/emission.py: Calculate synchrotron emissivityAaron LI2017-06-012-0/+123
| | | | | | | Calculate the synchrotron emissivity from the given electron spectrum at specified frequency. Add the electron charge to units.Constants
* halo.py: Rewrite "_coef_acceleration()" methodAaron LI2017-06-011-15/+44
|
* Bind ClusterFormation to HaloSingleAaron LI2017-06-012-1/+7
| | | | Also add logging messages to simulate_mergertree()
* cosmology.py: Optimize the speed of overdensity_crit()Aaron LI2017-06-011-2/+11
|
* Update to use custom units.py instead of astropy'sAaron LI2017-06-013-52/+36
| | | | Also fix a parameter error in "formation.py"
* Add units.py: Commonly used units and conversions and constantsAaron LI2017-06-011-0/+66
| | | | | Astropy's unit conversions is too slow, thus store the used units conversions to avoid astropy's slow conversions.
* mergertree.py: Implement function "plot_mtree()"Aaron LI2017-06-011-2/+52
|
* halo.py: Update to match MergerTree structuresAaron LI2017-06-011-8/+8
|
* configs: Add sigma8 to specificationsAaron LI2017-06-011-0/+2
|
* Add clusters/formation.py: Simulate cluster merging historyAaron LI2017-06-012-0/+234
|
* mergertree.py: Remove "merged" parameterAaron LI2017-06-011-5/+1
|
* solver.py: Avoid possible overflow when w is too largeAaron LI2017-06-011-0/+10
|
* halo.py: Force a minimal value on acceleration coefficientAaron LI2017-06-013-3/+27
| | | | | | | To avoid the too small (or zero) values for the diffusion coefficient of the Fokker-Planck equation. Also change config "extragalactic/halo/pmax" from 1e4 to 1e5
* cosmology.py: Greatly optimize the speed!Aaron LI2017-06-011-26/+57
|
* cosmology.py: Only support flat ΛCDM cosmological modelAaron LI2017-06-011-93/+25
|
* clusters/halo: Add missing config "buffer_np"Aaron LI2017-06-012-0/+7
|
Copyright © 2017-2018 Aaron LI. All Rights Reserved.