Commit message (Collapse) | Author | Age | Files | Lines | |
---|---|---|---|---|---|
* | 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 |
| | |||||
* | clusters/solver.py: Adjust parameter tc,uc orders | Aaron LI | 2017-10-06 | 1 | -10/+7 |
| | |||||
* | clusters/solver.py: Stop calc. at "tstop" by adding "tstep" parameter | Aaron LI | 2017-10-06 | 1 | -12/+19 |
| | |||||
* | clusters/solver.py: Update comments/references/descriptions etc. | Aaron LI | 2017-10-06 | 1 | -25/+31 |
| | |||||
* | 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 | 1 | -69/+136 |
| | | | | | | | | | | | | * 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 | ||||
* | clusters/psformalism.py: Improve catalog comments | Aaron LI | 2017-10-02 | 1 | -4/+7 |
| | |||||
* | 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 | 1 | -4/+19 |
| | |||||
* | clusters: Add config option "boost" | Aaron LI | 2017-09-01 | 1 | -2/+5 |
| | | | | | | | 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. | ||||
* | Update "Fnu_to_Tb_fast()" to "Fnu_to_Tb()" | Aaron LI | 2017-09-01 | 6 | -9/+9 |
| | |||||
* | clusters/psformalism: Remove config "f_darkmatter" | Aaron LI | 2017-08-29 | 1 | -3/+2 |
| | | | | Use "1 - baryon_fraction = 1 - Ob0/Om0" to replace "f_darkmatter". | ||||
* | clusters/halo.py: Update injection rate calculation | Aaron LI | 2017-08-26 | 1 | -10/+5 |
| | | | | | The electrons are assumed to be injected throughout the whole cluster ICM/volume. | ||||
* | Return the list of filepath to the written sky files | Aaron LI | 2017-08-26 | 1 | -0/+8 |
| | |||||
* | clusters/main.py: Update sky header; update comments etc. | Aaron LI | 2017-08-26 | 1 | -5/+7 |
| | |||||
* | configs: Remove option "save"; all enabled components will be saved | Aaron LI | 2017-08-26 | 1 | -1/+0 |
| | |||||
* | clusters/halo.py: Rewrite electron acceleration coefficient calc | Aaron LI | 2017-08-14 | 2 | -26/+53 |
| | | | | | | | | | | * Adopt the electron acceleration coefficient formula from [cassano2005] * Rename method "_tau_acceleration()" to "_chi_acceleration()", and rewrite * Add property "kT_merger" * Also save "kT_merger" and "chi" into halos data Signed-off-by: Aaron LI <aly@aaronly.me> | ||||
* | clusters/main.py: Use OrderedDict to easy keys manipulation | Aaron LI | 2017-08-14 | 1 | -29/+31 |
| | | | | | | | Also avoid forgetting to add the newly added item for DataFrame conversion. Signed-off-by: Aaron LI <aly@aaronly.me> | ||||
* | clusters/halo.py: Simplify two coefficients usage | Aaron LI | 2017-08-14 | 1 | -7/+5 |
| | | | | Signed-off-by: Aaron LI <aly@aaronly.me> | ||||
* | clusters: Rename property "injection_rate" and save into halos data | Aaron LI | 2017-08-14 | 2 | -37/+38 |
| | | | | Signed-off-by: Aaron LI <aly@aaronly.me> | ||||
* | Use "GalaxyClusters" from main.py, and remove clusters.py | Aaron LI | 2017-08-14 | 2 | -734/+2 |
| | | | | Signed-off-by: Aaron LI <aly@aaronly.me> | ||||
* | Fix several bugs | Aaron LI | 2017-08-13 | 1 | -11/+3 |
| | | | | | | | | | * Brought back "clobber" property * Delete the wrong "self.halos=[]" * Fix the wrong assignment of "cimax0" * Assign default values for {c,r}i{min,max}1 Signed-off-by: Aaron LI <aly@aaronly.me> | ||||
* | clusters/main.py: Implement "simulate_frequency()" and "simulate()" | Aaron LI | 2017-08-13 | 1 | -0/+46 |
| | | | | Signed-off-by: Aaron LI <aly@aaronly.me> | ||||
* | clusters: Halo templates are normalized to have mean of 1 | Aaron LI | 2017-08-13 | 2 | -4/+12 |
| | | | | | | Also update the documents of "draw_halo()" function Signed-off-by: Aaron LI <aly@aaronly.me> | ||||
* | clusters/main.py: Add method "_outfilepath()" | Aaron LI | 2017-08-13 | 1 | -0/+21 |
| | | | | Signed-off-by: Aaron LI <aly@aaronly.me> | ||||
* | clusters/main.py: Set sky header properties | Aaron LI | 2017-08-13 | 1 | -4/+5 |
| | | | | | | | * Clean up the unused configurations * Add "FREQ" keyword to the sky FITS header Signed-off-by: Aaron LI <aly@aaronly.me> | ||||
* | clusters/main.py: Implement "_draw_halos()" method | Aaron LI | 2017-08-12 | 2 | -2/+89 |
| | | | | | | New functions "halo_rprofile()" and "draw_halo()" added to helper.py Signed-off-by: Aaron LI <aly@aaronly.me> | ||||
* | clusters/main.py: Inherent cluster catalog info to halos data | Aaron LI | 2017-08-12 | 1 | -4/+9 |
| | | | | | | Also rename "frequencies" to "frequency" Signed-off-by: Aaron LI <aly@aaronly.me> | ||||
* | clusters/main.py: Add missing columns to DataFrame conversion | Aaron LI | 2017-08-12 | 1 | -2/+2 |
| | | | | Signed-off-by: Aaron LI <aly@aaronly.me> | ||||
* | clusters: Implement calc_{power,flux,brightness_mean} in helper | Aaron LI | 2017-08-11 | 2 | -40/+116 |
| | | | | | | Help development & debug ... Signed-off-by: Aaron LI <aly@aaronly.me> | ||||
* | clusters/halo: "volume" use unit "kpc^3" instead of "cm^3" | Aaron LI | 2017-08-11 | 2 | -4/+7 |
| | | | | Signed-off-by: Aaron LI <aly@aaronly.me> | ||||
* | clusters/main.py: Calculate and cache more halo data | Aaron LI | 2017-08-06 | 1 | -4/+9 |
| | | | | Signed-off-by: Aaron LI <aly@aaronly.me> | ||||
* | Fix a bug in clusters/halo.py; Add a comment to utils/io/_create_dir() | Aaron LI | 2017-08-06 | 1 | -1/+1 |
| | | | | Signed-off-by: Aaron LI <aly@aaronly.me> | ||||
* | Update against "Fnu_to_Tb_fast()" unit changes | Aaron LI | 2017-08-03 | 6 | -28/+36 |
| | | | | Signed-off-by: Aaron LI <aly@aaronly.me> | ||||
* | clusters/main.py: Convert halos data to be a DataFrame and dump | Aaron LI | 2017-08-03 | 1 | -0/+19 |
| | | | | Signed-off-by: Aaron LI <aly@aaronly.me> | ||||
* | clusters/emission.py: Make "F()" be class method, fixing memory hole! | Aaron LI | 2017-08-01 | 1 | -22/+35 |
| | | | | | | | | | | | For unknown reason! Each instance of "SynchrotronEmission" will cost ~5 MiB memory when interpolating the kernel function cached as "self._F_interp", which won't be collected/freed by GC, for UNKNOWN reason! Therefore, make the method "F()" be class-wide, to avoid the memory hole! Signed-off-by: Aaron LI <aly@aaronly.me> | ||||
* | Improve logging messages | Aaron LI | 2017-08-01 | 2 | -4/+9 |
| | | | | Signed-off-by: Aaron LI <aly@aaronly.me> | ||||
* | clusters/emission.py: Fix bug in "F()" | Aaron LI | 2017-08-01 | 1 | -13/+14 |
| | | | | Signed-off-by: Aaron LI <aly@aaronly.me> | ||||
* | clusters: Add config "halos_dumpfile" and dump simulate halos data | Aaron LI | 2017-08-01 | 1 | -1/+8 |
| | |||||
* | clusters/halo.py: Finished brief simulation description | Aaron LI | 2017-08-01 | 1 | -3/+13 |
| | |||||
* | clusters: Fix several small issues on wrong variable names | Aaron LI | 2017-07-31 | 3 | -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 bit | Aaron LI | 2017-07-31 | 1 | -4/+10 |
| | | | | Signed-off-by: Aaron LI <aly@aaronly.me> | ||||
* | clusters/main.py: Use PSFormalism to simulate cluster catalog | Aaron LI | 2017-07-31 | 1 | -13/+11 |
| | | | | Signed-off-by: Aaron LI <aly@aaronly.me> | ||||
* | clusters: Add psformalism.py to simulate cluster catalog | Aaron LI | 2017-07-31 | 1 | -0/+230 |
| | | | | | | Also updated configuration options. Signed-off-by: Aaron LI <aly@aaronly.me> | ||||
* | Add `fg21sim.share` module to hold globally shared "CONFIGS" & "COSMO" | Aaron LI | 2017-07-31 | 4 | -7/+4 |
| | | | | Signed-off-by: Aaron LI <aly@aaronly.me> | ||||
* | clusters/main.py: Add method "_simulate_halos()" | Aaron LI | 2017-07-31 | 1 | -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" property | Aaron LI | 2017-07-31 | 1 | -0/+6 |
| | | | | Signed-off-by: Aaron LI <aly@aaronly.me> | ||||
* | Update references a bit | Aaron LI | 2017-07-31 | 1 | -19/+15 |
| | | | | Signed-off-by: Aaron LI <aly@aaronly.me> |