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dc.contributor.authorLiu, Adrian Chi-Yan
dc.contributor.authorTegmark, Max Erik
dc.contributor.authorBowman, Judd D.
dc.contributor.authorHewitt, Jacqueline N.
dc.contributor.authorZaldarriaga, Matias, 1971-
dc.date.accessioned2013-01-30T21:38:51Z
dc.date.available2013-01-30T21:38:51Z
dc.date.issued2009-09
dc.date.submitted2009-05
dc.identifier.issn0035-8711
dc.identifier.issn1365-8711
dc.identifier.urihttp://hdl.handle.net/1721.1/76695
dc.description.abstract21-cm tomography is expected to be difficult in part because of serious foreground contamination. Previous studies have found that line-of-sight approaches are capable of cleaning foregrounds to an acceptable level on large spatial scales, but not on small spatial scales. In this paper, we introduce a Fourier space formalism for describing the line-of-sight methods, and use it to introduce an improved new method for 21-cm foreground cleaning. Heuristically, this method involves fitting foregrounds in Fourier space using weighted polynomial fits, with each pixel weighted according to its information content. We show that the new method reproduces the old one on large angular scales, and gives marked improvements on small scales at essentially no extra computational cost.en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (Grant AST-0134999)en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (Grant AST-05-06556)en_US
dc.description.sponsorshipDavid & Lucile Packard Foundationen_US
dc.description.sponsorshipResearch Corporationen_US
dc.language.isoen_US
dc.publisherOxford University Pressen_US
dc.relation.isversionofhttp://dx.doi.org/10.1111/j.1365-2966.2009.15156.xen_US
dc.rightsCreative Commons Attribution-Noncommercial-Share Alike 3.0en_US
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/3.0/en_US
dc.sourcearXiven_US
dc.titleAn Improved Method for 21cm Foreground Removalen_US
dc.typeArticleen_US
dc.identifier.citationLiu, Adrian et al. “An Improved Method for 21-cm Foreground Removal.” Monthly Notices of the Royal Astronomical Society 398.1 (2009): 401–406.en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.contributor.departmentMIT Kavli Institute for Astrophysics and Space Researchen_US
dc.contributor.mitauthorLiu, Adrian Chi-Yan
dc.contributor.mitauthorTegmark, Max Erik
dc.contributor.mitauthorHewitt, Jacqueline N.
dc.relation.journalMonthly Notices of the Royal Astronomical Societyen_US
dc.eprint.versionAuthor's final manuscripten_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dspace.orderedauthorsLiu, Adrian; Tegmark, Max; Bowman, Judd; Hewitt, Jacqueline; Zaldarriaga, Matiasen
dc.identifier.orcidhttps://orcid.org/0000-0002-4117-570X
dc.identifier.orcidhttps://orcid.org/0000-0001-7670-7190
dc.identifier.orcidhttps://orcid.org/0000-0001-6876-0928
dspace.mitauthor.errortrue
mit.licenseOPEN_ACCESS_POLICYen_US
mit.metadata.statusComplete


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