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galsci
PySM 3: Sky emission simulations for Cosmic Microwave Background experiments
I'm working with @brandonshensley to quantify decorrelation in the new models. Here is a first [notebook + plot](https://gist.github.com/myra-norton/8edcde151758a5898b0653aadc037d84)!
We should implement a generic component that can take a list of coordinates and flux from an input file and generate a map already smoothed with the instrument beam. This...
I am describing here an issue that I ran into while trying to return a CAR map using `pysm3.apply_smoothing_and_coord_transform` I find specifically the error originates when _template.py_ tries to import...
## Problem PySM needs to store the templates at very different resolutions, we want people to be able to do maps at low nside without the need of downloading and...
I checked models d9, d10 and d12 at 100µm (one of IRAS frequencies), these are smoothed to the IRIS resolution (4.3arcmin):    This is the IRIS map: ...
Hello team, I'm running the following example script on a compute node that does not have internet access: ``` import os os.environ['PYSM_LOCAL_DATA']='/scratch/gpfs/ip8725/pysm-data/' import numpy as np import healpy as hp...
I just realized that `rg1` doesn't have polarization. although this goes into the direction of having a low complexity model, i think neglecting the blazar polarization is not realistic. I...
Functionality exported from #116 - smooth directly the small scales - fix: was smoothing the mbb temperature instead of the template - scale also index and mbb temperature - make...
- feat: add ModifiedBlackBodyRealizationGL as a copy of ModifiedBlackBodyRealization - feat: map2alm and alm2map for Gauss Legendre with test - utils - feat: first running implementation of dx11-style realization in...
I did the comparison between the PySM bandpass integrated dust models d9, d10, d11 and d12 with Planck's 3rd data release at 353 GHz and nside 2048. Bandpass used: HFI_RIMO_R3.00.fits...