Abstract
The 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.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 1610-1618 |
| Number of pages | 9 |
| Journal | Astrophysical Journal |
| Volume | 694 |
| Issue number | 2 |
| DOIs | |
| State | Published - 2009 |
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Keywords
- Cosmic microwave background
- Instrumentation: interferometers
- Telescopes
ASJC Scopus subject areas
- Space and Planetary Science
- Astronomy and Astrophysics
Cite this
The yuan-tseh lee array for microwave background anisotropy. / Ho, Paul T P; Altamirano, Pablo; Chang, Chia Hao; Chang, Shu Hao; Chang, Su Wei; Chen, Chung Cheng; Chen, Ke Jung; Chen, Ming Tang; Han, Chih Chiang; Ho, West M.; Huang, Yau De; Hwang, Yuh Jing; Ibãez-Romano, Fabiola; Jiang, Homin; Koch, Patrick M.; Kubo, Derek Y.; Li, Chao Te; Lim, Jeremy; Lin, Kai Yang; Liu, Guo Chin; Lo, Kwok Yung; Ma, Cheng Jiun; Martin, Robert N.; Martin-Cocher, Pierre; Molnar, Sandor M.; Ng, Kin Wang; Nishioka, Hiroaki; O'Connell, Kevin E.; Oshiro, Peter; Patt, Ferdinand; Raffin, Philippe; Umetsu, Keiichi; Wei, Tashun; Wu, Jiun Huei Proty; Chiueh, Tzi Dar; Chiueh, Tzihong; Chu, Tah Hsiung; Huang, Chih Wei Locutus; Hwang, W. Y Pauchy; Liao, Yu Wei; Lien, Chun Hsien; Wang, Fu Cheng; Wang, Huei; Wei, Ray Ming; Yang, Chia Hsiang; Kesteven, Michael; Kingsley, Jeffrey S; Sinclair, Malcolm M.; Wilson, Warwick; Birkinshaw, Mark; Liang, Haida; Lancaster, Katy; Park, Chan Gyung; Pen, Ue Li; Peterson, Jeffrey B.
In: Astrophysical Journal, Vol. 694, No. 2, 2009, p. 1610-1618.Research output: Contribution to journal › Article
}
TY - JOUR
T1 - The yuan-tseh lee array for microwave background anisotropy
AU - Ho, Paul T P
AU - Altamirano, Pablo
AU - Chang, Chia Hao
AU - Chang, Shu Hao
AU - Chang, Su Wei
AU - Chen, Chung Cheng
AU - Chen, Ke Jung
AU - Chen, Ming Tang
AU - Han, Chih Chiang
AU - Ho, West M.
AU - Huang, Yau De
AU - Hwang, Yuh Jing
AU - Ibãez-Romano, Fabiola
AU - Jiang, Homin
AU - Koch, Patrick M.
AU - Kubo, Derek Y.
AU - Li, Chao Te
AU - Lim, Jeremy
AU - Lin, Kai Yang
AU - Liu, Guo Chin
AU - Lo, Kwok Yung
AU - Ma, Cheng Jiun
AU - Martin, Robert N.
AU - Martin-Cocher, Pierre
AU - Molnar, Sandor M.
AU - Ng, Kin Wang
AU - Nishioka, Hiroaki
AU - O'Connell, Kevin E.
AU - Oshiro, Peter
AU - Patt, Ferdinand
AU - Raffin, Philippe
AU - Umetsu, Keiichi
AU - Wei, Tashun
AU - Wu, Jiun Huei Proty
AU - Chiueh, Tzi Dar
AU - Chiueh, Tzihong
AU - Chu, Tah Hsiung
AU - Huang, Chih Wei Locutus
AU - Hwang, W. Y Pauchy
AU - Liao, Yu Wei
AU - Lien, Chun Hsien
AU - Wang, Fu Cheng
AU - Wang, Huei
AU - Wei, Ray Ming
AU - Yang, Chia Hsiang
AU - Kesteven, Michael
AU - Kingsley, Jeffrey S
AU - Sinclair, Malcolm M.
AU - Wilson, Warwick
AU - Birkinshaw, Mark
AU - Liang, Haida
AU - Lancaster, Katy
AU - Park, Chan Gyung
AU - Pen, Ue Li
AU - Peterson, Jeffrey B.
PY - 2009
Y1 - 2009
N2 - The 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.
AB - The 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.
KW - Cosmic microwave background
KW - Instrumentation: interferometers
KW - Telescopes
UR - http://www.scopus.com/inward/record.url?scp=75149155205&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=75149155205&partnerID=8YFLogxK
U2 - 10.1088/0004-637X/694/2/1610
DO - 10.1088/0004-637X/694/2/1610
M3 - Article
AN - SCOPUS:75149155205
VL - 694
SP - 1610
EP - 1618
JO - Astrophysical Journal
JF - Astrophysical Journal
SN - 0004-637X
IS - 2
ER -