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Published February 2021 | Accepted Version + Published
Journal Article Open

DAYENU: a simple filter of smooth foregrounds for intensity mapping power spectra

Abstract

We introduce DPSS Approximate lazY filtEriNg of foregroUnds (DAYENU), a linear, spectral filter for H I intensity mapping that achieves the desirable foreground mitigation and error minimization properties of inverse co-variance weighting with minimal modelling of the underlying data. Beyond 21-cm power-spectrum estimation, our filter is suitable for any analysis where high dynamic-range removal of spectrally smooth foregrounds in irregularly (or regularly) sampled data is required, something required by many other intensity mapping techniques. Our filtering matrix is diagonalized by Discrete Prolate Spheroidal Sequences which are an optimal basis to model band-limited foregrounds in 21-cm intensity mapping experiments in the sense that they maximally concentrate power within a finite region of Fourier space. We show that DAYENU enables the access of large-scale line-of-sight modes that are inaccessible to tapered discrete Fourier transform estimators. Since these modes have the largest SNRs,DAYENU significantly increases the sensitivity of 21-cm analyses over tapered Fourier transforms. Slight modifications allow us to use DAYENU as a linear replacement for iterative delay CLEAN ing (DAYENUREST). We refer readers to the Code section at the end of this paper for links to examples and code.

Additional Information

© 2020 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. This article is published and distributed under the terms of the Oxford University Press, Standard Journals Publication Model (https://academic.oup.com/journals/pages/open_access/funder_policies/chorus/standard_publication_model). Accepted 2020 October 20. Received 2020 October 5; in original form 2020 May 5. Published: 23 October 2020. We thank Jacqueline Hewitt, Honggeun Kim, Kevin Bandura, Miguel Morales, Bobby Pascua, Bryna Hazelton, and Ue-Li Pen for helpful discussions. AEW and acknowledges support from the NASA Postdoctoral Program and the Berkeley Center of Cosmological Physics. JSD gratefully acknowledges the support of the NSF AAPF award #1701536. A portion of this work was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration. AL acknowledges support from the New Frontiers in Research Fund Exploration grant program, a Natural Sciences and Engineering Research Council of Canada (NSERC) Discovery Grant and a Discovery Launch Supplement, the Sloan Research Fellowship, as well as the Canadian Institute for Advanced Research (CIFAR) Azrieli Global Scholars program. This material is based upon work supported by the National Science Foundation under grants #1636646 and #1836019 and institutional support from the HERA collaboration partners. This research is funded in part by the Gordon and Betty Moore Foundation. HERA is hosted by the South African Radio Astronomy Observatory, which is a facility of the National Research Foundation, an agency of the Department of Science and Innovation. Code: An interactive jupyter tutorial on using dayenu can be found at https://github.com/HERA-Team/uvtools/blob/master/examples/linear_clean_demo.ipynb. dayenu's source code can be found at https://github.com/HERA-Team/uvtools/blob/master/uvtools/dspec.py This work made use of the numpy (Virtanen et al. 2020), scipy (Virtanen et al. 2020), matplotlib (Hunter 2007), aipy https://github.com/HERA-Team/aipy, and astropy https://www.astropy.org/ and jupyter https://github.com/jupyter/jupyter python libraries along with pyuvdata (Hazelton et al. 2017) and healvis (Lanman & Kern 2019) python packages.

Attached Files

Published - staa3293.pdf

Accepted Version - 2004.11397.pdf

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Additional details

Created:
August 20, 2023
Modified:
October 20, 2023