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DC-0 Validation spectra: Synchrotron #29
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hello, not sure what it might cause this honestly . |
@giuspugl I agree, it also simplifies the dust models. Alternatively what if we apply just a tiny bit of smoothing to the real data to smooth out pixel effects? Is it confirmed that the problem is It would be good to have feedback from @seclark and @brandonshensley. |
well, this seems to me a bit as an epicycle approach. We need to convolve the template by a beam of ~5' to avoid that spectra explodes at ell=2000. Although it seems totally feasible , it 's true that few users would look at the ell=2000 power spectrum of Gal. plane... |
Recording that we discussed this on the PanEx call today and plan to not make the change for now, but to note it as a caveat to the models in the current paper. We do not expect that this will affect typical use cases since these models are not designed to reproduce the power spectrum of the Galactic center, and we will address this in the future as we update our treatment of small scale structure in bright regions anyway. |
documented in PySM, see the linked issues. |
@giuspugl the other issue I noted, also in simonsobs/map_based_simulations#44 (comment) is spikes at high-ell in the Synchrotron maps.
Should check if they are still there when masking.
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