| dc.contributor.author | Liu, Adrian Chi-Yan | |
| dc.contributor.author | Tegmark, Max Erik | |
| dc.contributor.author | Bowman, Judd D. | |
| dc.contributor.author | Hewitt, Jacqueline N. | |
| dc.contributor.author | Zaldarriaga, Matias, 1971- | |
| dc.date.accessioned | 2013-01-30T21:38:51Z | |
| dc.date.available | 2013-01-30T21:38:51Z | |
| dc.date.issued | 2009-09 | |
| dc.date.submitted | 2009-05 | |
| dc.identifier.issn | 0035-8711 | |
| dc.identifier.issn | 1365-8711 | |
| dc.identifier.uri | http://hdl.handle.net/1721.1/76695 | |
| dc.description.abstract | 21-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.sponsorship | National Science Foundation (U.S.) (Grant AST-0134999) | en_US |
| dc.description.sponsorship | National Science Foundation (U.S.) (Grant AST-05-06556) | en_US |
| dc.description.sponsorship | David & Lucile Packard Foundation | en_US |
| dc.description.sponsorship | Research Corporation | en_US |
| dc.language.iso | en_US | |
| dc.publisher | Oxford University Press | en_US |
| dc.relation.isversionof | http://dx.doi.org/10.1111/j.1365-2966.2009.15156.x | en_US |
| dc.rights | Creative Commons Attribution-Noncommercial-Share Alike 3.0 | en_US |
| dc.rights.uri | http://creativecommons.org/licenses/by-nc-sa/3.0/ | en_US |
| dc.source | arXiv | en_US |
| dc.title | An Improved Method for 21cm Foreground Removal | en_US |
| dc.type | Article | en_US |
| dc.identifier.citation | Liu, 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.department | Massachusetts Institute of Technology. Department of Physics | en_US |
| dc.contributor.department | MIT Kavli Institute for Astrophysics and Space Research | en_US |
| dc.contributor.mitauthor | Liu, Adrian Chi-Yan | |
| dc.contributor.mitauthor | Tegmark, Max Erik | |
| dc.contributor.mitauthor | Hewitt, Jacqueline N. | |
| dc.relation.journal | Monthly Notices of the Royal Astronomical Society | en_US |
| dc.eprint.version | Author's final manuscript | en_US |
| dc.type.uri | http://purl.org/eprint/type/JournalArticle | en_US |
| eprint.status | http://purl.org/eprint/status/PeerReviewed | en_US |
| dspace.orderedauthors | Liu, Adrian; Tegmark, Max; Bowman, Judd; Hewitt, Jacqueline; Zaldarriaga, Matias | en |
| dc.identifier.orcid | https://orcid.org/0000-0002-4117-570X | |
| dc.identifier.orcid | https://orcid.org/0000-0001-7670-7190 | |
| dc.identifier.orcid | https://orcid.org/0000-0001-6876-0928 | |
| dspace.mitauthor.error | true | |
| mit.license | OPEN_ACCESS_POLICY | en_US |
| mit.metadata.status | Complete | |