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poltens full sky power spectra #100
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can you please share the code? |
I just use Namaster with following masks to calculate the power spectra of the IQU maps transfromed from polten maps with small scales. The Namaster code and the maps are exactly from this notebook . |
@yaojian95 I'd rather see the actual notebook you ran, in particular with all the intermediate outputs. it would be useful to compare spectra to the original map and/or to the large-scales-only map. |
Thank you @yaojian95 and @NicolettaK for checking this! This is something we were aware as for testing and for the implementation we didn't considered the full sky case but always the GAL080 one. From the plot above |
@giuspugl What do you mean by "neglecting any leakage effect due to the Galactic cut" ? |
To address this issue we agreed on including the real observed data (without any small scale ) within the region inside the GAL097 HFI mask see this post . I think this version of the maps benefits of the high SNR and high resolution at 21.8', notice how we transition more gradually from the observed small scales (at ell>400) to the artificial ones as we go from fsky = 1 to fsky~0.90 . Thanks @yaojian95 and @NicolettaK for spotting this !! |
@giuspugl can you please share the notebook implementing this fix and generating those plots? I'd like to use it as reference for my implementation and then merge it into the docs. |
implementation of the galactic plane fix was not too bad. |
Hi,
@yaojian95 has been working a bit on poltens dust maps produced by @giuspugl in #97, in order to estimate non-Gaussianity. He has computed power spectra for different fsky. In particular, power spectra on full sky look a bit weird, with bumps around \ell~100 (see below). Have you already discussed this point? I'm not sure whether this is critical or not, as spectra look ok once we move away from the Galactic plane, but we just want to make sure that you are aware of this features.
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