pysm
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galsci
PySM 3: Sky emission simulations for Cosmic Microwave Background experiments
> I'd like to propose a sanity regression test for this. The middle CMB band is usually chosen to balance the power of the radio and CIB foreground components. Thus,...
It would be useful to have an implementation of the CMB Dipole as a separate component in PySM. I have a simple implementation here: https://github.com/CMB-S4/s4mapbasedsims/blob/master/202102_design_tool_input/utils/create_cmb_solar_dipole.ipynb However it would be nice...
Current sky models at high resolution are very expensive to run, especially memory-wise. A complete sky model with CMB, foregrounds and extragalactic can have 8-9 components, each needs to load...
In the course of using the d9 and d10 models, it has been noted that these models have more B-mode power at ell~80 in the Southern Hole than is measured...
This is an effort to validate the PySM3 synchrotron models by comparing with Planck LFI 30 GHz (NPIPE Full, A and B splits) and WMAP 23 GHz (9year) maps. For...
I am failing test_d10_vs_d11 when passing the parameters for `seeds` and `synalm_lmax` in test_dust_pysm3.py; however, when I followed the instructions to modify data/presets.cfg and I commented out the parameters `seeds`...
I had unit testing working on Github Actions for Mac OS. However, after I added the requirement on `pixell`, `numba` stopped working. I tried playing with `NUMBA_DISABLE_JIT`, I got most...
Based on the slides emailed on Oct. 19, @delabrou recommends we, "[m]ultiply dust template maps by 0.92 to get a template at 353 GHz rather than integrated in the Planck...
MSS-001 production run * 700 nodes * 10 nodes/group * 70 groups * 8 MPI processes/node * ~ 7 observation per group * 2580 channels * 1/20th year * TOD...