File Download

There are no files associated with this item.

  Links for fulltext
     (May Require Subscription)
Supplementary

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

TitleThe yuan-tseh lee array for microwave background anisotropy
Authors
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?
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
2015 Impact Factor: 5.487
2015 SCImago Journal Rankings: 3.369
ISI Accession Number ID
References

 

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
dc.identifier.scopusauthoridChen, CC=7501950054en_US
dc.identifier.scopusauthoridChen, KJ=43361012100en_US
dc.identifier.scopusauthoridChen, MT=25722966100en_US
dc.identifier.scopusauthoridHan, CC=7403379491en_US
dc.identifier.scopusauthoridHo, WM=35329501200en_US
dc.identifier.scopusauthoridHuang, YD=7501580011en_US
dc.identifier.scopusauthoridHwang, YJ=7402311428en_US
dc.identifier.scopusauthoridIbãezRomano, F=43361354600en_US
dc.identifier.scopusauthoridJiang, H=35177706000en_US
dc.identifier.scopusauthoridKoch, PM=7202929125en_US
dc.identifier.scopusauthoridKubo, DY=24474502900en_US
dc.identifier.scopusauthoridLi, CT=7501686171en_US
dc.identifier.scopusauthoridLim, J=7403453870en_US
dc.identifier.scopusauthoridLin, KY=43361314500en_US
dc.identifier.scopusauthoridLiu, GC=26643238900en_US
dc.identifier.scopusauthoridLo, KY=7402101550en_US
dc.identifier.scopusauthoridMa, CJ=16432796100en_US
dc.identifier.scopusauthoridMartin, RN=35474579900en_US
dc.identifier.scopusauthoridMartinCocher, P=6506130985en_US
dc.identifier.scopusauthoridMolnar, SM=7102411479en_US
dc.identifier.scopusauthoridNg, KW=7403178527en_US
dc.identifier.scopusauthoridNishioka, H=7102469161en_US
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
dc.identifier.scopusauthoridHuang, CWL=36080193900en_US
dc.identifier.scopusauthoridHwang, WYP=25939793300en_US
dc.identifier.scopusauthoridLiao, YW=14822253900en_US
dc.identifier.scopusauthoridLien, CH=27167735500en_US
dc.identifier.scopusauthoridWang, FC=7501312852en_US
dc.identifier.scopusauthoridWang, H=7501731867en_US
dc.identifier.scopusauthoridWei, RM=35331089700en_US
dc.identifier.scopusauthoridYang, CH=9534061100en_US
dc.identifier.scopusauthoridKesteven, M=7004146312en_US
dc.identifier.scopusauthoridKingsley, J=7003840294en_US
dc.identifier.scopusauthoridSinclair, MM=35588969500en_US
dc.identifier.scopusauthoridWilson, W=7404032342en_US
dc.identifier.scopusauthoridBirkinshaw, M=7005755208en_US
dc.identifier.scopusauthoridLiang, H=7402854000en_US
dc.identifier.scopusauthoridLancaster, K=16506552900en_US
dc.identifier.scopusauthoridPark, CG=43361710800en_US
dc.identifier.scopusauthoridPen, UL=7005890052en_US
dc.identifier.scopusauthoridPeterson, JB=54790597800en_US

Export via OAI-PMH Interface in XML Formats


OR


Export to Other Non-XML Formats