We calculate the cross-correlations between CMB lensing reconstructions and a (correlated) galaxy density field. The lensing reconstructions currently account for (stacked) foregrounds and the LSST survey mask based on a depth-limited LSST footprint, while the correlated galaxy density field accounts for the LSST survey mask and modulation seen due to the systematics induced by the depth non-uniformities (with, without MW dust).
[Need to be written out, once finalized]
- The
code
folder contains the working code. Thenotebooks
folder contains some helper notebooks. - The
legacy
folder contains code/docs from initial analyses/exploration. Specifically, inlegacy-recent
:- The main code is in two scripts:
code/save_needed_alms.py
calculates the various alms and saves them, whilecode/get_spectra.py
reads in the saved alms to calculate and plot the spectra. These scripts which use the rest of the files in that folder. scripts/run_analysis.sh
runs the python scripts with specific inputs.- The code needed orphics, pixell, and falafel; all these have changed though.
- The main code is in two scripts:
The code needs basic packages: healpy
, numpy
, matplotlib
.