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dc.contributor.authorHewitt, Jacqueline N
dc.date.accessioned2022-04-15T14:01:13Z
dc.date.available2022-04-15T14:01:13Z
dc.date.issued2021
dc.identifier.urihttps://hdl.handle.net/1721.1/141908
dc.description.abstractAs current- and next-generation astronomical instruments come online, they will generate an unprecedented deluge of data. Analyzing these data in real time presents unique conceptual and computational challenges, and their long-term storage and archiving is scientifically essential for generating reliable, reproducible results. We present here the real-time processing (RTP) system for the Hydrogen Epoch of Reionization Array (HERA), a radio interferometer endeavoring to provide the first detection of the highly redshifted 21 cm signal from Cosmic Dawn and the Epoch of Reionization by an interferometer. The RTP system consists of analysis routines run on raw data shortly after they are acquired, such as calibration and detection of radio-frequency interference (RFI) events. RTP works closely with the Librarian, the HERA data storage and transfer manager which automatically ingests data and transfers copies to other clusters for post-processing analysis. Both the RTP system and the Librarian are public and open source software, which allows for them to be modified for use in other scientific collaborations. When fully constructed, HERA is projected to generate over 50 terabytes (TB) of data each night, and the RTP system enables the successful scientific analysis of these data.en_US
dc.language.isoen
dc.publisherElsevier BVen_US
dc.relation.isversionof10.1016/J.ASCOM.2021.100489en_US
dc.rightsCreative Commons Attribution 4.0 International licenseen_US
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_US
dc.sourceElsevieren_US
dc.titleA Real Time Processing system for big data in astronomy: Applications to HERAen_US
dc.typeArticleen_US
dc.identifier.citationHewitt, Jacqueline N. 2021. "A Real Time Processing system for big data in astronomy: Applications to HERA." Astronomy and Computing, 36.
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physics
dc.relation.journalAstronomy and Computingen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2022-04-15T13:01:46Z
dspace.orderedauthorsLa Plante, P; Williams, PKG; Kolopanis, M; Dillon, JS; Beardsley, AP; Kern, NS; Wilensky, M; Ali, ZS; Abdurashidova, Z; Aguirre, JE; Alexander, P; Balfour, Y; Bernardi, G; Billings, TS; Bowman, JD; Bradley, RF; Bull, P; Burba, J; Carey, S; Carilli, CL; Cheng, C; DeBoer, DR; Dexter, M; de Lera Acedo, E; Ely, J; Ewall-Wice, A; Fagnoni, N; Fritz, R; Furlanetto, SR; Gale-Sides, K; Glendenning, B; Gorthi, D; Greig, B; Grobbelaar, J; Halday, Z; Hazelton, BJ; Hewitt, JN; Hickish, J; Jacobs, DC; Julius, A; Kerrigan, J; Kittiwisit, P; Kohn, SA; Lanman, A; Lekalake, T; Lewis, D; Liu, A; MacMahon, D; Malan, L; Malgas, C; Maree, M; Martinot, ZE; Matsetela, E; Mesinger, A; Molewa, M; Morales, MF; Mosiane, T; Murray, S; Neben, AR; Nikolic, B; Parsons, AR; Pascua, R; Patra, N; Pieterse, S; Pober, JC; Razavi-Ghods, N; Ringuette, J; Robnett, J; Rosie, K; Santos, MG; Sims, P; Smith, C; Syce, A; Thyagarajan, N; Zheng, Hen_US
dspace.date.submission2022-04-15T13:01:47Z
mit.journal.volume36en_US
mit.licensePUBLISHER_CC
mit.metadata.statusAuthority Work and Publication Information Neededen_US


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