Comments (2)
from pysm_public.
Hi, Thanks.
And I have another question (forgive me not to open a new issue in order to keep it clean for the issue board).
I read the document, and in the introduction section, I noticed
This code generates full-sky simulations of Galactic foregrounds in intensity and polarization relevant for CMB experiments.
Does it mean your code generate maps following the CMB polarization convention (i.e., the healpix convention), rather than the IAU convention?
The two polarization conventions
from pysm_public.
Related Issues (18)
- code license HOT 1
- Modifications for partial sky HOT 3
- Run tests with runtests HOT 2
- Tag a release HOT 3
- Units of noise levels in Instrument HOT 2
- Upgrading foreground templates to ~arcmin resolution
- Reduce PySM package size HOT 4
- How to calculate the E and B mode signal from Q and U map? HOT 2
- Nosetests failing HOT 1
- units of sky maps
- Integration for unit conversion
- `pysm.Instrument` seems not working properly in some cases HOT 1
- `instrument.observe` returns different maps according to the value of the flag `write_outputs`
- error in the `pysm.Instrument` documentation HOT 2
- Dust temperature can't be scalar HOT 1
- Unit tests
- K_RJ bandpass unit conversion
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