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dc.contributor.authorTegmark, Max Erik
dc.contributor.authorBuza, Victor
dc.contributor.authorDillon, Joshua Shane
dc.contributor.authorGharibyan, Hrant
dc.contributor.authorKunz, Eben A.
dc.contributor.authorLiu, Adrian Chi-Yan
dc.contributor.authorLosh, Jonathan L.
dc.contributor.authorLutomirksi, Andy
dc.contributor.authorMorrison, Scott D.
dc.contributor.authorNarayanan, Sruthi A.
dc.contributor.authorPerko, Ashley
dc.contributor.authorRosner, Devon
dc.contributor.authorSanchez, Nevada
dc.contributor.authorSchutz, Katelin
dc.contributor.authorTribiano, Shana
dc.contributor.authorValdez, Michael
dc.contributor.authorZelko, Ioana
dc.contributor.authorZheng, Kevin
dc.contributor.authorEwall-Wice, Aaron Michael
dc.contributor.authorMatejek, Michael Scott
dc.contributor.authorMorgan, Edward H.
dc.contributor.authorNeben, Abraham Richard
dc.contributor.authorPan, Qinxuan
dc.contributor.authorPenna, Robert
dc.contributor.authorSu, Meng
dc.contributor.authorVillasenor, Joel
dc.contributor.authorWilliams, Christopher Leigh
dc.contributor.authorYang, Hung-I
dc.contributor.authorZhu, Yan
dc.contributor.authorZheng, Haoxuan, Ph. D. Massachusetts Institute of Technology
dc.date.accessioned2014-09-05T17:19:13Z
dc.date.available2014-09-05T17:19:13Z
dc.date.issued2013-10
dc.identifier.isbn978-1-4673-1127-4
dc.identifier.isbn978-1-4673-1126-7
dc.identifier.urihttp://hdl.handle.net/1721.1/89207
dc.description.abstractMapping our universe in 3D by imaging the redshifted 21 cm line from neutral hydrogen has the potential to overtake the cosmic microwave background as our most powerful cosmological probe, because it can map a much larger volume of our Universe, shedding new light on the epoch of reionization, inflation, dark matter, dark energy, and neutrino masses. We report on MITEoR, a pathfinder low-frequency radio interferometer whose goal is to test technologies that greatly reduce the cost of such 3D mapping for a given sensitivity. MITEoR accomplishes this by using massive baseline redundancy both to enable automated precision calibration and to cut the correlator cost scaling from N[superscript 2] to N log N, where N is the number of antennas. The success of MITEoR with its 64 dual-polarization elements bodes well for the more ambitious HERA project, which incorporates many identical or similar technologies using an order of magnitude more antennas, each with dramatically larger collecting area.en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (Grant AST-0908848)en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (Grant AST-1105835)en_US
dc.description.sponsorshipMIT Kavli Instrumentation Funden_US
dc.description.sponsorshipMassachusetts Institute of Technology. Undergraduate Research Opportunities Programen_US
dc.language.isoen_US
dc.publisherInstitute of Electrical and Electronics Engineers (IEEE)en_US
dc.relation.isversionofhttp://dx.doi.org/10.1109/ARRAY.2013.6731928en_US
dc.rightsCreative Commons Attribution-Noncommercial-Share Alikeen_US
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/4.0/en_US
dc.sourcearXiven_US
dc.titleMapping our universe in 3D with MITEoRen_US
dc.typeArticleen_US
dc.identifier.citationZheng, Haoxuan, Max Tegmark, Victor Buza, Josh Dillon, Hrant Gharibyan, Jack Hickish, Eben Kunz, et al. “Mapping Our Universe in 3D with MITEoR.” 2013 IEEE International Symposium on Phased Array Systems and Technology (October 2013).en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Mathematicsen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.contributor.departmentMIT Kavli Institute for Astrophysics and Space Researchen_US
dc.contributor.mitauthorZheng, Haoxuanen_US
dc.contributor.mitauthorTegmark, Max Eriken_US
dc.contributor.mitauthorBuza, Victoren_US
dc.contributor.mitauthorDillon, Joshua Shaneen_US
dc.contributor.mitauthorGharibyan, Hranten_US
dc.contributor.mitauthorKunz, Eben A.en_US
dc.contributor.mitauthorLiu, Adrian Chi-Yanen_US
dc.contributor.mitauthorLosh, Jonathan L.en_US
dc.contributor.mitauthorLutomirksi, Andyen_US
dc.contributor.mitauthorMorrison, Scott D.en_US
dc.contributor.mitauthorNarayanan, Sruthi A.en_US
dc.contributor.mitauthorPerko, Ashleyen_US
dc.contributor.mitauthorRosner, Devonen_US
dc.contributor.mitauthorSanchez, Nevadaen_US
dc.contributor.mitauthorSchutz, Katelinen_US
dc.contributor.mitauthorTribiano, Shanaen_US
dc.contributor.mitauthorValdez, Michaelen_US
dc.contributor.mitauthorZelko, Ioanaen_US
dc.contributor.mitauthorZheng, Kevinen_US
dc.contributor.mitauthorEwall-Wice, Aaron Michaelen_US
dc.contributor.mitauthorMatejek, Michael Scotten_US
dc.contributor.mitauthorMorgan, Edward H.en_US
dc.contributor.mitauthorNeben, Abraham Richarden_US
dc.contributor.mitauthorPan, Qinxuanen_US
dc.contributor.mitauthorPenna, Roberten_US
dc.contributor.mitauthorSu, Mengen_US
dc.contributor.mitauthorVillasenor, Joelen_US
dc.contributor.mitauthorWilliams, Christopher Leighen_US
dc.contributor.mitauthorYang, Hung-Ien_US
dc.contributor.mitauthorZhu, Yanen_US
dc.relation.journalProceedings of the 2013 IEEE International Symposium on Phased Array Systems and Technologyen_US
dc.eprint.versionOriginal manuscripten_US
dc.type.urihttp://purl.org/eprint/type/ConferencePaperen_US
eprint.statushttp://purl.org/eprint/status/NonPeerRevieweden_US
dspace.orderedauthorsZheng, Haoxuan; Tegmark, Max; Buza, Victor; Dillon, Josh; Gharibyan, Hrant; Hickish, Jack; Kunz, Eben; Liu, Adrian; Losh, Jon; Lutomirski, Andy; Morrison, Scott; Narayanan, Sruthi; Perko, Ashley; Rosner, Devon; Sanchez, Nevada; Schutz, Katelin; Tribiano, Shana; Valdez, Michael; Zaldarriaga, Matias; Zarb-Adami, Kris; Zelko, Ioana; Zheng, Kevin; Armstrong, Richard; Bradley, Richard; Dexter, Matt; Ewall-Wice, Aaron; Magro, Alessio; Mateiek, Michael; Moraan, Edward; Neben, Abraham; Pan, Qinxuan; Peterson, Courtney; Penna, Robert F.; Su, Meng; Villasenor, Joel; Williams, Christopher L.; Yang, Hung-I; Zhu, Yanen_US
dc.identifier.orcidhttps://orcid.org/0000-0001-7776-7240
dc.identifier.orcidhttps://orcid.org/0000-0002-0086-7363
dc.identifier.orcidhttps://orcid.org/0000-0001-7130-208X
dc.identifier.orcidhttps://orcid.org/0000-0003-3336-9958
dc.identifier.orcidhttps://orcid.org/0000-0001-7670-7190
dc.identifier.orcidhttps://orcid.org/0000-0001-8412-8287
dc.identifier.orcidhttps://orcid.org/0000-0001-8267-3425
dc.identifier.orcidhttps://orcid.org/0000-0003-3932-6174
dc.identifier.orcidhttps://orcid.org/0000-0001-6876-0928
dspace.mitauthor.errortrue
mit.licenseOPEN_ACCESS_POLICYen_US
mit.metadata.statusComplete


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