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Filtering in CMB data analysis with application to ACT DR4 and Planck observations

Erik Rosenberg ^1,2,3,*, Steven Gratton^4,2,3, and Anthony Challinor ^2,3,4

¹Jodrell Bank Centre for Astrophysics, University of Manchester, Oxford Road, Manchester, M13 9PL, United Kingdom
²Institute of Astronomy, Madingley Road, Cambridge, CB3 0HA, United Kingdom
³Kavli Institute for Cosmology, Cambridge, Madingley Road, Cambridge, CB3 0HA, United Kingdom
⁴DAMTP, Centre for Mathematical Sciences, Wilberforce Road, Cambridge, CB3 0WA, United Kingdom

^*Contact author: erik.rosenberg@manchester.ac.uk

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Physical Review D

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Articles Citing

Filtering in CMB data analysis with application to ACT DR4 and Planck observations

SPT-3G D1: CMB temperature and polarization power spectra and cosmology from 2019 and 2020 observations of the SPT-3G main field

Atacama Cosmology Telescope: B -mode delensing with DR6 data and external tracers of large-scale structure

Mitigating point-source contamination in CMB polarization: a Generalized Point Spread Function fitting approach

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