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This paper presents a maximum-likelihood algorithm for combining sky maps with disparate sky coverage, angular resolution and spatially varying anisotropic noise into a single map of the sky.
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Barentsen, G., et al. 2014, Monthly Notices of the Royal Astronomical Society, 444, 3230–3257, The second data release of the INT Photometric H α \alpha Survey of the Northern Galactic Plane (IPHAS DR2)
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Meisner, A. M., Lang, D., & Schlegel, D. J. 2017, The Astronomical Journal, 154, 161, Deep Full-sky Coadds from Three Years of WISE and NEOWISE Observations
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Dey, A., et al. 2019, The Astronomical Journal, 157, 168, Overview of the DESI Legacy Imaging Surveys
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Aiola, S., Calabrese, E., Loic, M., & Naess, S. 2020, ApJS, The Atacama Cosmology Telescope: DR4 Maps and Cosmological Results
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Hilton, M., ACT, DES, & HSC. 2020, in preparation, The Atacama Cosmology Telescope: A Catalog of > 4000 >4000 Sunyaev-Zel’dovich Galaxy Clusters
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