S
Shu-Hao Chang
Researcher at Academia Sinica
Publications - 31
Citations - 549
Shu-Hao Chang is an academic researcher from Academia Sinica. The author has contributed to research in topics: Galaxy cluster & Cosmic microwave background. The author has an hindex of 10, co-authored 30 publications receiving 525 citations. Previous affiliations of Shu-Hao Chang include Academia Sinica Institute of Astronomy and Astrophysics.
Papers
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Journal ArticleDOI
MASS AND HOT BARYONS IN MASSIVE GALAXY CLUSTERS FROM SUBARU WEAK-LENSING AND AMiBA SUNYAEV-ZEL'DOVICH EFFECT OBSERVATIONS*
Keiichi Umetsu,Keiichi Umetsu,Mark Birkinshaw,Guo-Chin Liu,Guo-Chin Liu,Jiun-Huei Proty Wu,Elinor Medezinski,Tom Broadhurst,Doron Lemze,Adi Zitrin,Paul T. P. Ho,Paul T. P. Ho,Chih-Wei Locutus Huang,Patrick M. Koch,Yu-Wei Liao,Kai-Yang Lin,Kai-Yang Lin,Sandor M. Molnar,Hiroaki Nishioka,Fu-Cheng Wang,Pablo Altamirano,Chia-Hao Chang,Shu-Hao Chang,Su-Wei Chang,Ming-Tang Chen,Chih-Chiang Han,Yau-De Huang,Yuh-Jing Hwang,Homin Jiang,Michael Kesteven,Derek Kubo,Chao-Te Li,Pierre Martin-Cocher,Peter Oshiro,Philippe Raffin,Tashun Wei,Warwick Wilson +36 more
TL;DR: In this article, a multwavelength analysis of a sample of four hot (TX > 8 keV) X-ray galaxy clusters (A1689, A2261, A2142, and A2390) using joint AMiBA Sunyaev-Zel'dovich effect (SZE) and Subaru weak-lensing observations was presented.
Journal ArticleDOI
Mass and Hot Baryons in Massive Galaxy Clusters from Subaru Weak Lensing and AMiBA SZE Observations
Keiichi Umetsu,Mark Birkinshaw,Guo-Chin Liu,Jiun-Huei Proty Wu,Elinor Medezinski,Tom Broadhurst,Doron Lemze,Adi Zitrin,Paul T. P. Ho,Chih-Wei Locutus Huang,Patrick M. Koch,Yu-Wei Liao,Kai-Yang Lin,Sandor M. Molnar,Hiroaki Nishioka,Fu-Cheng Wang,Pablo Altamirano,Chia-Hao Chang,Shu-Hao Chang,Su-Wei Chang,Ming-Tang Chen,Chih-Chiang Han,Yau-De Huang,Yuh-Jing Hwang,Homin Jiang,Michael Kesteven,Derek Kubo,Chao-Te Li,Pierre Martin-Cocher,Peter Oshiro,Philippe Raffin,Ta-Shun Wei,Warwick Wilson +32 more
TL;DR: In this paper, a multi-wavelength analysis of a sample of four hot (T_X>8keV) X-ray galaxy clusters (A1689, A2261, A2142, and A2390) using joint AMiBA Sunyaev-Zel'dovich effect (SZE) and Subaru weak lensing observations was presented.
Journal ArticleDOI
The Yuan-Tseh Lee Array for microwave background anisotropy
Paul T. P. Ho,Paul T. P. Ho,Pablo Altamirano,Chia-Hao Chang,Shu-Hao Chang,Su-Wei Chang,Chung-Cheng Chen,Ke-Jung Chen,Ming-Tang Chen,Chih-Chiang Han,West M. Ho,Yau-De Huang,Yuh-Jing Hwang,Fabiola Ibanez-Romano,Homin Jiang,Patrick M. Koch,Derek Kubo,Chao-Te Li,Jeremy Lim,Kai-Yang Lin,Guo-Chin Liu,Guo-Chin Liu,K. Y. Lo,K. Y. Lo,Cheng-Jiun Ma,Cheng-Jiun Ma,Robert N. Martin,Pierre Martin-Cocher,Sandor M. Molnar,Kin-Wang Ng,Hiroaki Nishioka,Kevin E. O'Connell,Peter Oshiro,F. Patt,Philippe Raffin,Keiichi Umetsu,Keiichi Umetsu,Tashun Wei,Jiun-Huei Proty Wu,Tzi-Dar Chiueh,Tzihong Chiueh,Tah-Hsiung Chu,Chih-Wei Locutus Huang,W. Y. Pauchy Hwang,Yu-Wei Liao,Chun-Hsien Lien,Fu-Cheng Wang,Huei Wang,Ray-Ming Wei,Chia-Hsiang Yang,Michael Kesteven,J. S. Kingsley,Malcolm Sinclair,Warwick Wilson,Mark Birkinshaw,Haida Liang,Haida Liang,Katy Lancaster,Chan-Gyung Park,Ue-Li Pen,Jeffrey B. Peterson +60 more
TL;DR: 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 as discussed by the authors, where the choice of 3 mm is to minimize the contributions from foreground synchrotron radiation and Galactic dust emission.
Journal ArticleDOI
Array for microwave background anisotropy: Observations, data analysis, and results for sunyaev-zel'dovich effects
Jiun-Huei Proty Wu,Paul T. P. Ho,Paul T. P. Ho,Chih-Wei Locutus Huang,Patrick M. Koch,Yu-Wei Liao,Kai-Yang Lin,Kai-Yang Lin,Guo-Chin Liu,Guo-Chin Liu,Sandor M. Molnar,Hiroaki Nishioka,Keiichi Umetsu,Keiichi Umetsu,Fu-Cheng Wang,Pablo Altamirano,Mark Birkinshaw,Chia-Hao Chang,Shu-Hao Chang,Su-Wei Chang,Ming-Tang Chen,Tzihong Chiueh,Chih Chiang Han,Yau De Huang,Yuh-Jing Hwang,Homin Jiang,Michael Kesteven,Derek Kubo,Katy Lancaster,Chao-Te Li,Pierre Martin-Cocher,Peter Oshiro,Philippe Raffin,Tashun Wei,Warwick Wilson +34 more
TL;DR: In this article, the authors present observations, analysis, and results for the first-year operation of AMiBA, an interferometric experiment designed to study cosmology via the measurement of cosmic microwave background (CMB).
Journal ArticleDOI
AMiBA: Broadband Heterodyne CMB Interferometry
Ming-Tang Chen,Chao-Te Li,Yuh-Jing Hwang,Homin Jiang,Pablo Altamirano,Chia-Hao Chang,Shu-Hao Chang,Su-Wei Chang,Tzi-Dar Chiueh,Tah-Hsiung Chu,Chih-Chiang Han,Yau-De Huang,Michael Kesteven,Derek Kubo,Pierre Martin-Cocher,Peter Oshiro,Philippe Raffin,Ta-Shun Wei,Huei Wang,Warwick Wilson,Paul T. P. Ho,Chih-Wei Huang,Patrick M. Koch,Yu-Wei Liao,Kai-Yang Lin,Guo-Chin Liu,Sandor M. Molnar,Hiroaki Nishioka,Keiichi Umetsu,Fu-Cheng Wang,Jiun-Huei Proty Wu +30 more
TL;DR: The Y. T. Lee Array for Microwave Background (AMiBA) as mentioned in this paper was designed for the best sensitivity by utilizing the maximum possible continuum bandwidth matched to the atmospheric window at 86-102GHz, with dual polarizations.