Please use this identifier to cite or link to this item: https://www.um.edu.mt/library/oar/handle/123456789/88561
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dc.contributor.authorZheng, Haoxuan-
dc.contributor.authorTegmark, Max-
dc.contributor.authorBuza, Victor-
dc.contributor.authorDillon, Josh-
dc.contributor.authorGharibyan, Hrant-
dc.contributor.authorHickish, Jack-
dc.contributor.authorKunz, Eben-
dc.contributor.authorLiu, Adrian-
dc.contributor.authorLosh, Jon-
dc.contributor.authorLutomirski, Andy-
dc.contributor.authorMorrison, Scott-
dc.contributor.authorNarayanan, Sruthi-
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.authorZaldarriaga, Matias-
dc.contributor.authorZarb Adami, Kristian-
dc.contributor.authorZelko, Ioana-
dc.contributor.authorZheng, Kevin-
dc.contributor.authorArmstrong, Richard-
dc.contributor.authorBradley, Richard-
dc.contributor.authorDexter, Matt-
dc.contributor.authorEwall-Wice, Aaron-
dc.contributor.authorMagro, Alessio-
dc.contributor.authorMatejek, Michael-
dc.contributor.authorMorgan, Edward-
dc.contributor.authorNeben, Abraham-
dc.contributor.authorPan, Qinxuan-
dc.contributor.authorPeterson, Courtney-
dc.contributor.authorPenna, Robert F.-
dc.contributor.authorSu, Meng-
dc.contributor.authorVillasenor, Joel-
dc.contributor.authorWilliams, Christopher L.-
dc.contributor.authorYang, Hung-I-
dc.contributor.authorZhu, Yan-
dc.date.accessioned2022-02-08T10:50:47Z-
dc.date.available2022-02-08T10:50:47Z-
dc.date.issued2013-
dc.identifier.citationZheng, H., Tegmark, M., Buza, V., Dillon, J., Gharibyan, H., Hickish, J., ... & Zhu, Y. (2013). Mapping our Universe in 3D with MITEoR. In 2013 IEEE International Symposium on Phased Array Systems and Technology (pp. 784-791). IEEE.en_GB
dc.identifier.isbn9781467311274-
dc.identifier.urihttps://www.um.edu.mt/library/oar/handle/123456789/88561-
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 N2 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_GB
dc.language.isoenen_GB
dc.publisherIEEEen_GB
dc.rightsinfo:eu-repo/semantics/restrictedAccessen_GB
dc.subjectThree-dimensional modelingen_GB
dc.subjectAstrophysicsen_GB
dc.subjectAstronautical instruments -- Design and constructionen_GB
dc.titleMapping our Universe in 3D with MITEoRen_GB
dc.typeconferenceObjecten_GB
dc.rights.holderThe copyright of this work belongs to the author(s)/publisher. The rights of this work are as defined by the appropriate Copyright Legislation or as modified by any successive legislation. Users may access this work and can make use of the information contained in accordance with the Copyright Legislation provided that the author must be properly acknowledged. Further distribution or reproduction in any format is prohibited without the prior permission of the copyright holder.en_GB
dc.bibliographicCitation.conferencename2013 IEEE International Symposium on Phased Array Systems and Technologyen_GB
dc.description.reviewedpeer-revieweden_GB
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