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Article: The yuan-tseh lee array for microwave background anisotropy

TitleThe yuan-tseh lee array for microwave background anisotropy
Authors
Ho, PTPAltamirano, PChang, CHChang, SHChang, SWChen, CCChen, KJChen, MTHan, CCHo, WMHuang, YDHwang, YJIbãezRomano, FJiang, HKoch, PMKubo, DYLi, CTLim, JLin, KYLiu, GCLo, KYMa, CJMartin, RNMartinCocher, PMolnar, SMNg, KWNishioka, HO'connell, KEOshiro, PPatt, FRaffin, PUmetsu, KWei, TWu, JHPChiueh, TDChiueh, TChu, THHuang, CWLHwang, WYPLiao, YWLien, CHWang, FCWang, HWei, RMYang, CHKesteven, MKingsley, JSinclair, MMWilson, WBirkinshaw, MLiang, HLancaster, KPark, CGPen, ULPeterson, JB
KeywordsCosmic Microwave Background
Instrumentation: Interferometers
Telescopes
Issue Date2009
PublisherInstitute of Physics Publishing Ltd. The Journal's web site is located at http://iopscience.iop.org/2041-8205
Citation
Astrophysical Journal Letters, 2009, v. 694 n. 2, p. 1610-1618 How to Cite?
DOI: http://dx.doi.org/10.1088/0004-637X/694/2/1610
AbstractThe Yuan-Tseh Lee Array for microwave background anisotropy is the first interferometer dedicated to study the cosmic microwave background radiation at 3 mm wavelength. The choice of 3 mm is to minimize the contributions from foreground synchrotron radiation and Galactic dust emission. The initial configuration of seven 0.6 m telescopes mounted on a 6 m hexapod platform was dedicated in 2006 October on Mauna Loa, Hawaii. Scientific operations began with the detection of a number of clusters of galaxies via the thermal Sunyaev-Zel'dovich effect. We compare our data with Subaru weak-lensing data to study the structure of dark matter. We also compare our data with X-ray data to derive the Hubble constant. © 2009. The American Astronomical Society. All rights reserved.
Persistent Identifierhttp://hdl.handle.net/10722/175170
ISSN
2041-8205
2023 Impact Factor: 8.8
2023 SCImago Journal Rankings: 2.766
ISI Accession Number ID
WOS:000264538900073
References
References in Scopus

 

DC FieldValueLanguage
dc.contributor.authorHo, PTPen_US
dc.contributor.authorAltamirano, Pen_US
dc.contributor.authorChang, CHen_US
dc.contributor.authorChang, SHen_US
dc.contributor.authorChang, SWen_US
dc.contributor.authorChen, CCen_US
dc.contributor.authorChen, KJen_US
dc.contributor.authorChen, MTen_US
dc.contributor.authorHan, CCen_US
dc.contributor.authorHo, WMen_US
dc.contributor.authorHuang, YDen_US
dc.contributor.authorHwang, YJen_US
dc.contributor.authorIbãezRomano, Fen_US
dc.contributor.authorJiang, Hen_US
dc.contributor.authorKoch, PMen_US
dc.contributor.authorKubo, DYen_US
dc.contributor.authorLi, CTen_US
dc.contributor.authorLim, Jen_US
dc.contributor.authorLin, KYen_US
dc.contributor.authorLiu, GCen_US
dc.contributor.authorLo, KYen_US
dc.contributor.authorMa, CJen_US
dc.contributor.authorMartin, RNen_US
dc.contributor.authorMartinCocher, Pen_US
dc.contributor.authorMolnar, SMen_US
dc.contributor.authorNg, KWen_US
dc.contributor.authorNishioka, Hen_US
dc.contributor.authorO'connell, KEen_US
dc.contributor.authorOshiro, Pen_US
dc.contributor.authorPatt, Fen_US
dc.contributor.authorRaffin, Pen_US
dc.contributor.authorUmetsu, Ken_US
dc.contributor.authorWei, Ten_US
dc.contributor.authorWu, JHPen_US
dc.contributor.authorChiueh, TDen_US
dc.contributor.authorChiueh, Ten_US
dc.contributor.authorChu, THen_US
dc.contributor.authorHuang, CWLen_US
dc.contributor.authorHwang, WYPen_US
dc.contributor.authorLiao, YWen_US
dc.contributor.authorLien, CHen_US
dc.contributor.authorWang, FCen_US
dc.contributor.authorWang, Hen_US
dc.contributor.authorWei, RMen_US
dc.contributor.authorYang, CHen_US
dc.contributor.authorKesteven, Men_US
dc.contributor.authorKingsley, Jen_US
dc.contributor.authorSinclair, MMen_US
dc.contributor.authorWilson, Wen_US
dc.contributor.authorBirkinshaw, Men_US
dc.contributor.authorLiang, Hen_US
dc.contributor.authorLancaster, Ken_US
dc.contributor.authorPark, CGen_US
dc.contributor.authorPen, ULen_US
dc.contributor.authorPeterson, JBen_US
dc.date.accessioned2012-11-26T08:49:35Z-
dc.date.available2012-11-26T08:49:35Z-
dc.date.issued2009en_US
dc.identifier.citationAstrophysical Journal Letters, 2009, v. 694 n. 2, p. 1610-1618en_US
dc.identifier.issn2041-8205en_US
dc.identifier.urihttp://hdl.handle.net/10722/175170-
dc.description.abstractThe Yuan-Tseh Lee Array for microwave background anisotropy is the first interferometer dedicated to study the cosmic microwave background radiation at 3 mm wavelength. The choice of 3 mm is to minimize the contributions from foreground synchrotron radiation and Galactic dust emission. The initial configuration of seven 0.6 m telescopes mounted on a 6 m hexapod platform was dedicated in 2006 October on Mauna Loa, Hawaii. Scientific operations began with the detection of a number of clusters of galaxies via the thermal Sunyaev-Zel'dovich effect. We compare our data with Subaru weak-lensing data to study the structure of dark matter. We also compare our data with X-ray data to derive the Hubble constant. © 2009. The American Astronomical Society. All rights reserved.en_US
dc.languageengen_US
dc.publisherInstitute of Physics Publishing Ltd. The Journal's web site is located at http://iopscience.iop.org/2041-8205en_US
dc.relation.ispartofAstrophysical Journal Lettersen_US
dc.subjectCosmic Microwave Backgrounden_US
dc.subjectInstrumentation: Interferometersen_US
dc.subjectTelescopesen_US
dc.titleThe yuan-tseh lee array for microwave background anisotropyen_US
dc.typeArticleen_US
dc.identifier.emailLim, J: jjlim@hku.hken_US
dc.identifier.authorityLim, J=rp00745en_US
dc.description.naturelink_to_subscribed_fulltexten_US
dc.identifier.doi10.1088/0004-637X/694/2/1610en_US
dc.identifier.scopuseid_2-s2.0-75149155205en_US
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-75149155205&selection=ref&src=s&origin=recordpageen_US
dc.identifier.volume694en_US
dc.identifier.issue2en_US
dc.identifier.spage1610en_US
dc.identifier.epage1618en_US
dc.identifier.isiWOS:000264538900073-
dc.publisher.placeUnited Kingdomen_US
dc.identifier.scopusauthoridHo, PTP=7402211489en_US
dc.identifier.scopusauthoridAltamirano, P=25647163300en_US
dc.identifier.scopusauthoridChang, CH=43361001800en_US
dc.identifier.scopusauthoridChang, SH=35329046100en_US
dc.identifier.scopusauthoridChang, SW=14832199200en_US
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dc.identifier.scopusauthoridChen, KJ=43361012100en_US
dc.identifier.scopusauthoridChen, MT=25722966100en_US
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dc.identifier.scopusauthoridIbãezRomano, F=43361354600en_US
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dc.identifier.scopusauthoridKoch, PM=7202929125en_US
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dc.identifier.scopusauthoridLi, CT=7501686171en_US
dc.identifier.scopusauthoridLim, J=7403453870en_US
dc.identifier.scopusauthoridLin, KY=43361314500en_US
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dc.identifier.scopusauthoridLo, KY=7402101550en_US
dc.identifier.scopusauthoridMa, CJ=16432796100en_US
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dc.identifier.scopusauthoridNg, KW=7403178527en_US
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dc.identifier.scopusauthoridO'Connell, KE=43361572800en_US
dc.identifier.scopusauthoridOshiro, P=25823175800en_US
dc.identifier.scopusauthoridPatt, F=6701686651en_US
dc.identifier.scopusauthoridRaffin, P=6602270674en_US
dc.identifier.scopusauthoridUmetsu, K=7006622321en_US
dc.identifier.scopusauthoridWei, T=43361943300en_US
dc.identifier.scopusauthoridWu, JHP=7409251963en_US
dc.identifier.scopusauthoridChiueh, TD=7102713137en_US
dc.identifier.scopusauthoridChiueh, T=35373583000en_US
dc.identifier.scopusauthoridChu, TH=7401775911en_US
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dc.identifier.scopusauthoridHwang, WYP=25939793300en_US
dc.identifier.scopusauthoridLiao, YW=14822253900en_US
dc.identifier.scopusauthoridLien, CH=27167735500en_US
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dc.identifier.scopusauthoridWei, RM=35331089700en_US
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dc.identifier.scopusauthoridPeterson, JB=54790597800en_US
dc.identifier.issnl2041-8205-

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