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Conference Paper: The Yuan Tseh Lee AMiBA project
Title | The Yuan Tseh Lee AMiBA project |
---|---|
Authors | Ho, PTPAltimirano, PBirkinshaw, MChang, SWChang, CHChen, KJChen, MChiueh, TDChiueh, TChu, THHan, CCHuang, CWHuang, YDHwang, WYPHwang, YJJiang, HKesteven, MKoch, PKubo, DLancaster, KLi, CTLiang, HLiao, YWLim, JLin, YSLin, KYLiu, GCLo, KYMa, CJMartinCocher, PMartin, RNMolnar, SNg, KWNishioka, HPark, CGPatt, FPeterson, JBRaffin, PRomano, FWang, HUmetsu, KWang, FCWu, JHP |
Keywords | Cosmic Microwave Background Cosmology Interferometry |
Issue Date | 2008 |
Publisher | World Scientific Publishing Co Pte Ltd. The Journal's web site is located at http://www.worldscinet.com/mpla/mpla.shtml |
Citation | Modern Physics Letters A, 2008, v. 23 n. 17-20, p. 1243-1251 How to Cite? |
Abstract | The Array for Microwave Background Anisotropy is a 7-element interferometer sited on Mauna Loa, Hawaii. The seven 60cm telescopes are mounted on a 6-meter platform, and operates at 3mm wavelength. In October 2006, the telescope was officially dedicated and renamed as the Y. T. Lee AMiBA. During 2007, scientific operations have begun, after a long process of calibration and testing. At the time of this meeting, six clusters of galaxies have been detected and mapped via the inverse Compton scattering of the Cosmic Microwave Background radiation, also known as the Sunyaev-Zel'dovich Effect. © 2008 World Scientific Publishing Company. |
Persistent Identifier | http://hdl.handle.net/10722/176194 |
ISSN | 2023 Impact Factor: 1.5 2023 SCImago Journal Rankings: 0.404 |
ISI Accession Number ID | |
References |
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Ho, PTP | en_US |
dc.contributor.author | Altimirano, P | en_US |
dc.contributor.author | Birkinshaw, M | en_US |
dc.contributor.author | Chang, SW | en_US |
dc.contributor.author | Chang, CH | en_US |
dc.contributor.author | Chen, KJ | en_US |
dc.contributor.author | Chen, M | en_US |
dc.contributor.author | Chiueh, TD | en_US |
dc.contributor.author | Chiueh, T | en_US |
dc.contributor.author | Chu, TH | en_US |
dc.contributor.author | Han, CC | en_US |
dc.contributor.author | Huang, CW | en_US |
dc.contributor.author | Huang, YD | en_US |
dc.contributor.author | Hwang, WYP | en_US |
dc.contributor.author | Hwang, YJ | en_US |
dc.contributor.author | Jiang, H | en_US |
dc.contributor.author | Kesteven, M | en_US |
dc.contributor.author | Koch, P | en_US |
dc.contributor.author | Kubo, D | en_US |
dc.contributor.author | Lancaster, K | en_US |
dc.contributor.author | Li, CT | en_US |
dc.contributor.author | Liang, H | en_US |
dc.contributor.author | Liao, YW | en_US |
dc.contributor.author | Lim, J | en_US |
dc.contributor.author | Lin, YS | en_US |
dc.contributor.author | Lin, KY | en_US |
dc.contributor.author | Liu, GC | en_US |
dc.contributor.author | Lo, KY | en_US |
dc.contributor.author | Ma, CJ | en_US |
dc.contributor.author | MartinCocher, P | en_US |
dc.contributor.author | Martin, RN | en_US |
dc.contributor.author | Molnar, S | en_US |
dc.contributor.author | Ng, KW | en_US |
dc.contributor.author | Nishioka, H | en_US |
dc.contributor.author | Park, CG | en_US |
dc.contributor.author | Patt, F | en_US |
dc.contributor.author | Peterson, JB | en_US |
dc.contributor.author | Raffin, P | en_US |
dc.contributor.author | Romano, F | en_US |
dc.contributor.author | Wang, H | en_US |
dc.contributor.author | Umetsu, K | en_US |
dc.contributor.author | Wang, FC | en_US |
dc.contributor.author | Wu, JHP | en_US |
dc.date.accessioned | 2012-11-26T09:06:46Z | - |
dc.date.available | 2012-11-26T09:06:46Z | - |
dc.date.issued | 2008 | en_US |
dc.identifier.citation | Modern Physics Letters A, 2008, v. 23 n. 17-20, p. 1243-1251 | en_US |
dc.identifier.issn | 0217-7323 | en_US |
dc.identifier.uri | http://hdl.handle.net/10722/176194 | - |
dc.description.abstract | The Array for Microwave Background Anisotropy is a 7-element interferometer sited on Mauna Loa, Hawaii. The seven 60cm telescopes are mounted on a 6-meter platform, and operates at 3mm wavelength. In October 2006, the telescope was officially dedicated and renamed as the Y. T. Lee AMiBA. During 2007, scientific operations have begun, after a long process of calibration and testing. At the time of this meeting, six clusters of galaxies have been detected and mapped via the inverse Compton scattering of the Cosmic Microwave Background radiation, also known as the Sunyaev-Zel'dovich Effect. © 2008 World Scientific Publishing Company. | en_US |
dc.language | eng | en_US |
dc.publisher | World Scientific Publishing Co Pte Ltd. The Journal's web site is located at http://www.worldscinet.com/mpla/mpla.shtml | en_US |
dc.relation.ispartof | Modern Physics Letters A | en_US |
dc.subject | Cosmic Microwave Background | en_US |
dc.subject | Cosmology | en_US |
dc.subject | Interferometry | en_US |
dc.title | The Yuan Tseh Lee AMiBA project | en_US |
dc.type | Conference_Paper | en_US |
dc.identifier.email | Lim, J: jjlim@hku.hk | en_US |
dc.identifier.authority | Lim, J=rp00745 | en_US |
dc.description.nature | link_to_subscribed_fulltext | en_US |
dc.identifier.scopus | eid_2-s2.0-47749116867 | en_US |
dc.relation.references | http://www.scopus.com/mlt/select.url?eid=2-s2.0-47749116867&selection=ref&src=s&origin=recordpage | en_US |
dc.identifier.volume | 23 | en_US |
dc.identifier.issue | 17-20 | en_US |
dc.identifier.spage | 1243 | en_US |
dc.identifier.epage | 1251 | en_US |
dc.identifier.isi | WOS:000258297100011 | - |
dc.publisher.place | Singapore | en_US |
dc.identifier.scopusauthorid | Ho, PTP=7402211489 | en_US |
dc.identifier.scopusauthorid | Altimirano, P=24474358900 | en_US |
dc.identifier.scopusauthorid | Birkinshaw, M=7005755208 | en_US |
dc.identifier.scopusauthorid | Chang, SW=14832199200 | en_US |
dc.identifier.scopusauthorid | Chang, CH=24474100600 | en_US |
dc.identifier.scopusauthorid | Chen, KJ=24474443700 | en_US |
dc.identifier.scopusauthorid | Chen, M=25722966100 | en_US |
dc.identifier.scopusauthorid | Chiueh, TD=7102713137 | en_US |
dc.identifier.scopusauthorid | Chiueh, T=35373583000 | en_US |
dc.identifier.scopusauthorid | Chu, TH=7401775911 | en_US |
dc.identifier.scopusauthorid | Han, CC=7403379491 | en_US |
dc.identifier.scopusauthorid | Huang, CW=15822173300 | en_US |
dc.identifier.scopusauthorid | Huang, YD=24474561100 | en_US |
dc.identifier.scopusauthorid | Hwang, WYP=25939793300 | en_US |
dc.identifier.scopusauthorid | Hwang, YJ=7402311428 | en_US |
dc.identifier.scopusauthorid | Jiang, H=35177706000 | en_US |
dc.identifier.scopusauthorid | Kesteven, M=7004146312 | en_US |
dc.identifier.scopusauthorid | Koch, P=7202929125 | en_US |
dc.identifier.scopusauthorid | Kubo, D=24474502900 | en_US |
dc.identifier.scopusauthorid | Lancaster, K=16506552900 | en_US |
dc.identifier.scopusauthorid | Li, CT=7501686171 | en_US |
dc.identifier.scopusauthorid | Liang, H=7402854000 | en_US |
dc.identifier.scopusauthorid | Liao, YW=24474776700 | en_US |
dc.identifier.scopusauthorid | Lim, J=7403453870 | en_US |
dc.identifier.scopusauthorid | Lin, YS=8216516900 | en_US |
dc.identifier.scopusauthorid | Lin, KY=43361314500 | en_US |
dc.identifier.scopusauthorid | Liu, GC=26643238900 | en_US |
dc.identifier.scopusauthorid | Lo, KY=7402101550 | en_US |
dc.identifier.scopusauthorid | Ma, CJ=16432796100 | en_US |
dc.identifier.scopusauthorid | MartinCocher, P=6506130985 | en_US |
dc.identifier.scopusauthorid | Martin, RN=35474579900 | en_US |
dc.identifier.scopusauthorid | Molnar, S=7102411479 | en_US |
dc.identifier.scopusauthorid | Ng, KW=7403178527 | en_US |
dc.identifier.scopusauthorid | Nishioka, H=7102469161 | en_US |
dc.identifier.scopusauthorid | Park, CG=43361710800 | en_US |
dc.identifier.scopusauthorid | Patt, F=6701686651 | en_US |
dc.identifier.scopusauthorid | Peterson, JB=54790597800 | en_US |
dc.identifier.scopusauthorid | Raffin, P=6602270674 | en_US |
dc.identifier.scopusauthorid | Romano, F=24475506800 | en_US |
dc.identifier.scopusauthorid | Wang, H=7501731867 | en_US |
dc.identifier.scopusauthorid | Umetsu, K=7006622321 | en_US |
dc.identifier.scopusauthorid | Wang, FC=7501312852 | en_US |
dc.identifier.scopusauthorid | Wu, JHP=7409251963 | en_US |
dc.identifier.issnl | 0217-7323 | - |