Show simple item record

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.authorLutomirski, Andrew Michael
dc.contributor.authorMorrison, Scott D.
dc.contributor.authorNarayanan, Siddharth Madhavan
dc.contributor.authorPerko, Ashley
dc.contributor.authorRosner, Devin
dc.contributor.authorSanchez, N.
dc.contributor.authorSchutz, Katharine
dc.contributor.authorTribiano, Shana M.
dc.contributor.authorValdez, M.
dc.contributor.authorYang, H.
dc.contributor.authorZelko, Ioana
dc.contributor.authorZheng, K.
dc.contributor.authorArmstrong, R. P.
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, Jesus Noel Samonte
dc.contributor.authorWilliams, Christopher Leigh
dc.contributor.authorZhu, Y.
dc.contributor.authorZheng, Haoxuan, Ph. D. Massachusetts Institute of Technology
dc.date.accessioned2015-09-10T12:19:10Z
dc.date.available2015-09-10T12:19:10Z
dc.date.issued2014-10
dc.date.submitted2014-08
dc.identifier.issn0035-8711
dc.identifier.issn1365-2966
dc.identifier.urihttp://hdl.handle.net/1721.1/98426
dc.description.abstractWe report on the MIT Epoch of Reionization (MITEoR) experiment, a pathfinder low-frequency radio interferometer whose goal is to test technologies that improve the calibration precision and reduce the cost of the high-sensitivity 3D mapping required for 21 cm cosmology. MITEoR accomplishes this by using massive baseline redundancy, which enables both automated precision calibration and correlator cost reduction. We demonstrate and quantify the power and robustness of redundancy for scalability and precision. We find that the calibration parameters precisely describe the effect of the instrument upon our measurements, allowing us to form a model that is consistent with χ[superscript 2] per degree of freedom <1.2 for as much as 80 per cent of the observations. We use these results to develop an optimal estimator of calibration parameters using Wiener filtering, and explore the question of how often and how finely in frequency visibilities must be reliably measured to solve for calibration coefficients. The success of MITEoR with its 64 dual-polarization elements bodes well for the more ambitious Hydrogen Epoch of Reionization Array project and other next-generation instruments, which would incorporate many identical or similar technologies.en_US
dc.language.isoen_US
dc.publisherOxford University Pressen_US
dc.relation.isversionofhttp://dx.doi.org/10.1093/mnras/stu1773en_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.titleMITEoR: a scalable interferometer for precision 21 cm cosmologyen_US
dc.typeArticleen_US
dc.identifier.citationZheng, H., M. Tegmark, V. Buza, J. S. Dillon, H. Gharibyan, J. Hickish, E. Kunz, et al. “MITEoR: a Scalable Interferometer for Precision 21 Cm Cosmology.” Monthly Notices of the Royal Astronomical Society 445, no. 2 (October 8, 2014): 1084–1103.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.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.mitauthorLutomirski, Andrew Michaelen_US
dc.contributor.mitauthorMorrison, Scott D.en_US
dc.contributor.mitauthorNarayanan, Siddharth Madhavanen_US
dc.contributor.mitauthorPerko, Ashleyen_US
dc.contributor.mitauthorRosner, Devinen_US
dc.contributor.mitauthorSanchez, N.en_US
dc.contributor.mitauthorSchutz, Katharineen_US
dc.contributor.mitauthorTribiano, Shana M.en_US
dc.contributor.mitauthorValdez, M.en_US
dc.contributor.mitauthorYang, H.en_US
dc.contributor.mitauthorZelko, Ioanaen_US
dc.contributor.mitauthorZheng, K.en_US
dc.contributor.mitauthorArmstrong, R. P.en_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, Jesus Noel Samonteen_US
dc.contributor.mitauthorWilliams, Christopher Leighen_US
dc.contributor.mitauthorZhu, Y.en_US
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.orderedauthorsZheng, H.; Tegmark, M.; Buza, V.; Dillon, J. S.; Gharibyan, H.; Hickish, J.; Kunz, E.; Liu, A.; Losh, J.; Lutomirski, A.; Morrison, S.; Narayanan, S.; Perko, A.; Rosner, D.; Sanchez, N.; Schutz, K.; Tribiano, S. M.; Valdez, M.; Yang, H.; Adami, K. Z.; Zelko, I.; Zheng, K.; Armstrong, R. P.; Bradley, R. F.; Dexter, M. R.; Ewall-Wice, A.; Magro, A.; Matejek, M.; Morgan, E.; Neben, A. R.; Pan, Q.; Penna, R. F.; Peterson, C. M.; Su, M.; Villasenor, J.; Williams, C. L.; Zhu, Y.en_US
dc.identifier.orcidhttps://orcid.org/0000-0001-7776-7240
dc.identifier.orcidhttps://orcid.org/0000-0001-7130-208X
dc.identifier.orcidhttps://orcid.org/0000-0002-0086-7363
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/0000-0003-2723-3560
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


Files in this item

Thumbnail

This item appears in the following Collection(s)

Show simple item record