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dc.date.accessioned2022-08-25T17:22:44Z
dc.date.available2022-08-25T17:22:44Z
dc.date.created2022-08-22T11:33:16Z
dc.date.issued2022
dc.identifier.citationLamb, James W. Cleary, Kieran A. Woody, David P. Catha, Morgan Chung, Dongwoo T. Gundersen, Joshua Ott Harper, Stuart E. Harris, Andrew I. Hobbs, Richard Ihle, Håvard Tveit Kocz, Jonathon Pearson, Timothy J. Philip, Liju Powell, Travis W. Basoalto, Lilian Bond, J. Richard Borowska, Jowita Breysse, Patrick C. Church, Sarah E. Dickinson, Clive Dunne, Delaney A. Eriksen, Hans Kristian Kamfjord Foss, Marie Kristine Gaier, Todd Kim, Junhan Lawrence, Charles R. Lunde, Jonas Gahr Sturtzel Padmanabhan, Hamsa Rasmussen, Maren S. Readhead, Anthony C. S. Reeves, Rodrigo Rennie, Thomas J. Stutzer, Nils-Ole Viero, Marco P. Watts, Duncan Wehus, Ingunn Kathrine . COMAP Early Science. II. Pathfinder Instrument. The Astrophysical Journal (ApJ). 2022, 933(2)
dc.identifier.urihttp://hdl.handle.net/10852/95716
dc.description.abstractLine intensity mapping (LIM) is a new technique for tracing the global properties of galaxies over cosmic time. Detection of the very faint signals from redshifted carbon monoxide (CO), a tracer of star formation, pushes the limits of what is feasible with a total-power instrument. The CO Mapping Project Pathfinder is a first-generation instrument aiming to prove the concept and develop the technology for future experiments, as well as delivering early science products. With 19 receiver channels in a hexagonal focal plane arrangement on a 10.4 m antenna and an instantaneous 26–34 GHz frequency range with 2 MHz resolution, it is ideally suited to measuring CO (J = 1–0) from z ∼ 3. In this paper we discuss strategies for designing and building the Pathfinder and the challenges that were encountered. The design of the instrument prioritized LIM requirements over those of ancillary science. After a couple of years of operation, the instrument is well understood, and the first year of data is already yielding useful science results. Experience with this Pathfinder will guide the design of the next generations of experiments.
dc.languageEN
dc.rightsAttribution 4.0 International
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.titleCOMAP Early Science. II. Pathfinder Instrument
dc.title.alternativeENEngelskEnglishCOMAP Early Science. II. Pathfinder Instrument
dc.typeJournal article
dc.creator.authorLamb, James W.
dc.creator.authorCleary, Kieran A.
dc.creator.authorWoody, David P.
dc.creator.authorCatha, Morgan
dc.creator.authorChung, Dongwoo T.
dc.creator.authorGundersen, Joshua Ott
dc.creator.authorHarper, Stuart E.
dc.creator.authorHarris, Andrew I.
dc.creator.authorHobbs, Richard
dc.creator.authorIhle, Håvard Tveit
dc.creator.authorKocz, Jonathon
dc.creator.authorPearson, Timothy J.
dc.creator.authorPhilip, Liju
dc.creator.authorPowell, Travis W.
dc.creator.authorBasoalto, Lilian
dc.creator.authorBond, J. Richard
dc.creator.authorBorowska, Jowita
dc.creator.authorBreysse, Patrick C.
dc.creator.authorChurch, Sarah E.
dc.creator.authorDickinson, Clive
dc.creator.authorDunne, Delaney A.
dc.creator.authorEriksen, Hans Kristian Kamfjord
dc.creator.authorFoss, Marie Kristine
dc.creator.authorGaier, Todd
dc.creator.authorKim, Junhan
dc.creator.authorLawrence, Charles R.
dc.creator.authorLunde, Jonas Gahr Sturtzel
dc.creator.authorPadmanabhan, Hamsa
dc.creator.authorRasmussen, Maren S.
dc.creator.authorReadhead, Anthony C. S.
dc.creator.authorReeves, Rodrigo
dc.creator.authorRennie, Thomas J.
dc.creator.authorStutzer, Nils-Ole
dc.creator.authorViero, Marco P.
dc.creator.authorWatts, Duncan
dc.creator.authorWehus, Ingunn Kathrine
cristin.unitcode185,15,3,0
cristin.unitnameInstitutt for teoretisk astrofysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode2
dc.identifier.cristin2044903
dc.identifier.bibliographiccitationinfo:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=The Astrophysical Journal (ApJ)&rft.volume=933&rft.spage=&rft.date=2022
dc.identifier.jtitleThe Astrophysical Journal (ApJ)
dc.identifier.volume933
dc.identifier.issue2
dc.identifier.pagecount22
dc.identifier.doihttps://doi.org/10.3847/1538-4357/ac63c6
dc.identifier.urnURN:NBN:no-98242
dc.subject.nviVDP::Astrofysikk, astronomi: 438
dc.type.documentTidsskriftartikkel
dc.type.peerreviewedPeer reviewed
dc.source.issn0004-637X
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/95716/1/Lamb_2022_ApJ_933_183.pdf
dc.type.versionPublishedVersion
cristin.articleid183


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