The code used to create these maps is publicly available: https://github.com/jcolinhill/pyilc.

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data_products
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All publicly available maps are produced on the sky area left unmasked by the Planck 40% galactic plane mask. However, it can be more optimal to compute the covariance only on the area of sky that you are interested in. We provide sample code that can use pyilc to do this below.
pyilc_examples
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email me: fiona dot mccarthy 0 at gmail dot com
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