aboutsummaryrefslogtreecommitdiffstats
Commit message (Collapse)AuthorAgeFilesLines
* 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
|
* clusters/solver.py: Extrapolate the x grid to avoid NaN'sAaron LI2017-06-011-5/+15
|
* clusters/solver.py: Disable a RuntimeWarningAaron LI2017-06-011-2/+4
|
* clusters/clusters.py: Fix import pathAaron LI2017-06-011-6/+6
|
* Add "[extragalactic/halos]" configurationsAaron LI2017-06-011-0/+44
|
* Add clusters/halo.py: simulate single halo for clusterAaron LI2017-06-011-0/+698
| | | | | Simulate (giant) radio halos following the "statistical magneto-turbulent model" proposed by Cassano & Brunetti (2005).
* cosmology.py: Change name to "Cosmology"; Add "age0" and "Ob0"Aaron LI2017-06-011-3/+18
|
* Add clusters/solver.py to solve the Fokker-Planck equationAaron LI2017-06-011-0/+276
| | | | | Adopt the finite difference scheme to solve the Fokker-Planck equation, following Park & Petrosian (1996, ApJS, 103, 255).
* Add clusters/mergertree.pyAaron LI2017-06-011-0/+77
| | | | | The merger tree is a binary tree that represents the merging (or formation) history of a cluster.
* Add clusters/cosmology.py with common cosmological modelsAaron LI2017-06-011-0/+230
| | | | | | Mainly the "flat LambdaCDM" and "EdS" cosmological models. With some useful utility functions.
* Make separate directory for clusters, prepare for halo simulationsAaron LI2017-06-013-4/+4
|
* uvsim/telescope.py: Add "plot_stations()" and "plot_telescope()"Aaron LI2017-06-012-8/+85
|
* Add uvsim/ska1low.layout.txt: SKA1-low layout v2.0 2016-05-31Aaron LI2017-05-311-0/+538
| | | | | | Reference: SKA-TEL-SKO-0000422, revision 02, 2016-05-31, Table 1 http://astronomers.skatelescope.org/wp-content/uploads/2016/09/SKA-TEL-SKO-0000422_02_SKA1_LowConfigurationCoordinates-1.pdf
* Add uvsim/telescope.py and bin/make-ska1low-modelAaron LI2017-05-313-0/+283
| | | | | The `bin/make-ska1low-model` executable uses `telescope.py` to generate the SKA1-low telescope model for OSKAR simulation usage.
* setup.py: Use `os.listdir("bin/")` to obtain all executablesAaron LI2017-05-311-10/+1
|
* Add uvsim/wgs84.py: Convert WGS84 to ECEF/ENU coordinatesAaron LI2017-05-311-0/+97
|
* Add bin/get-healpix-patch: extract patch from HEALPix mapv0.4.2Aaron LI2017-05-272-3/+94
|
* sky.py: Fix FITS header writeAaron LI2017-05-271-4/+8
|
* extragalactic/clusters: Update to use sky.pyAaron LI2017-05-262-78/+91
|