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Research > Cosmology

Cosmology

Direct measurement of the CMB angular power spectrum. From WMAP V band map we choose patches with σ < 98 μK (after eliminating bright point sources), and we take the cross-power spectra of patches between WMAP V and W band. After deconvolution of the window functions, the power spectra of the 47 patches are shown in black dot and the mean power spectrum is in big blue dot. For comparison we plot in big orange dot the power spectrum binned (⊿l = 15) from that by the WMAP science team. The best-fit CDM model is in solid line.
Direct measurement of the angular power spectrum of cosmic microwave background temperature anisotropies in the WMAP Data
Three-dimensional cross power spectrum of the 21cm emission measured at the Green Bank Telescope and the optical density field traced by the WiggleZ redshift survey. Negative points are shown with reversed sign and a thin line. The solid line is the mean of simulations based on the empirical non-linear model of Blake et al. (2011) processed by the same pipeline. The overall amplitude is consistent with a measurement of Omega_HI~4*10^(-4) at z=0.8, similar to the value measured at z=0.
21cm brightness fluctuation at z=0.8 in cross-correlation
A cross-correlation measurement of 21-cm emission measured by the Green Bank Telescope, and the optical galaxies measured by the DEEP2 galaxy survey.
An intensity map of hydrogen 21-cm emission at redshift z ≈ 0.8
Average power spectrum in units of K 2 of all combinations of days, excluding December 11, as a function of the multipole moment l. Each point is shown with a 2σ upper limit derived from a bootstrap error analysis, which is in most cases smaller than the size of the point. The points are logarithmically spaced as described in the text, from left to right covering the ranges 377 < l < 578, 578 < l < 899 and 899 < l < 1414. Triangles are the power before subtracting foregrounds, diamonds are after 8 MHz mean subtraction, squares are after 2 MHz mean subtraction and circles are after 0.5 MHz subtraction. The curved solid line is the theoretical EoR signal from Jelic et al. (2008), and the dashed line is the theoretical EoR signal ´ with a cold absorbing IGM as described in the text.
The GMRT Epoch of Reionization experiment: a new upper limit on the neutral hydrogen power spectrum at z ≈ 8.6
Model-free direct reconstruction of full mass profiles for five massive galaxy clusters, A1689, A1703, A370, Cl0024+17, and RXJ1347-11, from combined weak and strong gravitational lensing.
Full mass profiles of five massive galaxy clusters
The figure represents the three-dimensional galaxy distribution for about 1/10 field of view of the RCS photometric redshift catalog (Hsieh et al. 2005, ApJS, 158, 161; Gladders and Yee 2005, ApJS, 157, 1) with the Earth at the origin. Each red dot indicate
Three-dimensional galaxy distribution for about 1/10 field of view of the RCS photometric redshift catalog
A Subaru Suprime-Cam image of one of the clusters used in the analysis, A2390, (2.7 billion light years from the Earth). The purple hue shows the dark matter distribution measured by the gravitational lensing effect on distant galaxies (typically 8 billion light years from the Earth), where the darker color indicates the denser dark matter concentration. It shows that the dark matter distribution is elongated along the northwest-southeast direction.
Direct measurement of dark matter halo ellipticity of massive clusters
Maps of the large-scale structure of galaxies (purple) and gas temperature distributions within the cluster (pink). Brighter pink indicates higher temperature. The filamentary structure is found outside the cluster in the top-left direction, in contact with the hotter gas realm. The other fields in which there are few galaxies (black) contact the cooler realm. The white line represents 10 million light-years.
Correlation between the temperature of the intra-cluster medium of galaxy cluster A1689 and its surrounding environment of the large-scale-structure.
Joint constraints on the dark-matter halo structure parameters of the galaxy cluster CL0024+1654 (z=0.395) from full lensing analysis of Subaru weak lensing and ACS strong lensing data (Umetsu et al. 2010, ApJ, in press; arXiv:0908.0069).
Joint constraints on the DM halo structure parameters from full lensing analysis (CL0024+1654)
The Sunyaev-Zel'dovich effect as a probe for large structures in the Universe. Top: integrated pressure contour map showing a signature of merger. Left: comparison between thermal and non-thermal spectral functions in a merger event. (Koch 2004, JKAS, 37,
Sunyaev-Zel'dovich effect as a probe for large structures in the Universe
Quadrupole power spectra for the 2dF QSO redshift survey measured with our algorithm. Anisotropic nature due to the redshift-space distortions can be seen although it is noisy (Yamamoto, Nakamichi, Kamino, Bassett & Nishioka 2006, PASJ 58, 93). The best-f
Quadrupole power spectra for the 2dF QSO redshift survey

Cosmology is the study of the large-scale properties of the universe as a whole. Our goal in cosmological studies is to understand the nature, origin, and evolution of the whole universe. The universe is the sum of all matter and energies, space and time, and the laws of nature. Cosmology involves the formation of theoretical models to describe our universe, which then provide us with specific predictions for physical phenomena that can be tested with astronomical experiments.

The research of the cosmology group at IAA has been focusing on the measurement analysis of the cosmic microwave background (CMB) and using multiwavelength observation and analysis on galaxy formation at high redshift and galaxy clusters in order to understand their properties and place constraints on the properties of dark energy (DE) and dark matter (DM).

Research Members (17)

Umetsu, Keiichi 梅津敬一 cv Associate Research Fellow (Tenure)
Research Interest: Observational Cosmology, Gravitational Lensing, Galaxy Clusters, Large Scale Structure in the Universe
Chang, Tzu-Ching 張慈錦 cv Assistant Research Fellow
Research Interest: 21-cm Cosmology; Cosmic Reionization; Gravitational Lensing; Large-scale Structure
Chiang, Lung-Yih 蔣龍毅 cv Assistant Research Fellow
Research Interest: Cosmology, Cosmic microwave background, Large-scale Structure of the Universe
Koch, Patrick 高培邁 cv Assistant Research Fellow
Research Interest: Structure Formation, Clusters of galaxies, Molecular Clouds
Lin, Li-Hwai 林俐暉 cv Assistant Research Fellow
Research Interest: Galaxy Evolution; Interacting Galaxies; Optical/Infrared Astronomy
Lin, Yen-Ting 林彥廷 cv Assistant Research Fellow
Research Interest: cosmological models constrained by cluster mass function
Wang, Wei-Hao 王為豪 cv Assistant Research Fellow
Research Interest: Multiwavelength observational studies of galaxy formation and evolution at high redshift
Chiueh, Tzi-Hong 闕志鴻 cv Joint Research Fellow; Dept. Physics, NTU
Research Interest: Theoretical Physics
Ng, Kin-Wang 吳建宏 cv Joint Research Fellow; Inst. of Physics, AS
Research Interest: Cosmology & Particle Astrophysics
Hsieh, Bau-Ching 謝寶慶 cv Support Scientist
Research Interest: High-z Galaxies, Large Scale Structure, Galaxy and Galaxy Cluster, Near Infrared/ Optical Astronomy
Huang, Chih-Wei Locutus 黃智威 cv Postdoc Fellow
Research Interest: Cosmic Microwave Background, Galaxy Clusters, Observational Cosmology
Liao, Yu-Wei 廖祐葳 cv Postdoc Fellow
Research Interest: Observation and theoratical analysis of cosmic microwave background; Observation of 21 CM emission at the epoch of reionization.
Lin, Kai-Yang 林凱揚 cv Project Scientist
Research Interest: Observational Cosmology, Galaxy Cluster; Radio Interferometry
Liu, Hau-Yu 呂浩宇 cv Postdoc Fellow
Research Interest: OB cluster formation; SMBH accretion; YSO jet variability; radio astrophysics
Nishioka, Hiroaki 西岡宏朗 cv Support Scientist
Research Interest: Observational Cosmology, Structure Formation in the Universe, Statistics of the Galaxy Distribution, Telescope Testing/Commissioning, Telescope Control Software
Okabe, Nobuhiro 岡部信広 cv Postdoc Fellow
Research Interest: Galaxy clusters, Weak lensing, X-ray & optical analyses, Plasma physics.
Yan, Chi-Hung 顏吉鴻 cv Technical Staff - OIR
Research Interest: OIR Image Pipeline, Radio Astronomy

Journal Papers (231)

  1. Coupon J; Broadhurst T; Umetsu K, "Cluster Lensing Profiles Derived from a Redshift Enhancement of Magnified BOSS-Survey Galaxie" , ApJ, 2013, Submitted [SCI] ( ADS | Fulltext )
  2. Koch PM; Ho PTP; ...; Lin KY; ...; Molnar SM; Nishioka H; Umetsu K; et al., "AMiBA 94 GHz SZE Observations: An Initial Measurement of H_0" , ApJ, 2013, Submitted [SCI] ( ADS | Fulltext )
  3. Koch PM;Chang Y-Y, "How significantly affect lage-scale filaments cluster SZE observations?" , ApJ, 2013, Submitted [SCI] ( ADS | Fulltext )
  4. Kuo CY; Braatz JA; Reid MJ; Lo FKY; et al., "The Megamaser Cosmology Project. V. An Angular Diameter Distance to NGC 6264 at 140 Mpc" , ApJ: 767(2), 155, April, 2013 [SCI] ( ADS | Fulltext )
  5. Liao Y-W; Lin K-Y; Huang Y-D; Wu JHP; Ho PTP; Chen M-T; Huang CWL; Koch PM; Nishioka H; Cheng T-A; Fu S-Y; Liu G-C; Molnar SM; Umetsu K; Wang F-C; Chang Y-Y; Han C-C; Li C-T; Martin-Cocher P; Oshiro P, "Platform Deformation Phase Correction for the AMiBA-13 Co-planar Interferometer" , ApJ: 769(1), 71, May, 2013 [SCI] ( ADS | Fulltext )
  6. Okabe N, "A Joint Weak-lensing, X-ray, Optical and Radio Study of Cold Front Cluster A2319: Gravitational Wake Triggers Cold Front and Radio Halo?" , ApJ, 2013, Submitted [SCI] ( ADS | Fulltext )
  7. Okabe N; Smith GP; Umetsu K; et al., "LoCuSS: The Mass Density Profile of Massive Galaxy Clusters at z=0.2" , ApJL: 769(2), L35, May 17, 2013 [SCI] ( ADS | Fulltext )
  8. Suyu SH; Auger MW; Hilbert S; et al., "Two Accurate Time-delay Distances from Strong Lensing: Implications for Cosmology" , ApJ: 766(2), 70, April 1, 2013 [SCI] ( ADS | Fulltext )
  9. Umetsu K, "Model-Free Multi-Probe Lensing Reconstruction of Cluster Mass Profiles" , ApJ: 769(2), 13, May, 2013 [SCI] ( ADS | Fulltext )
  10. Chang Y-Y; Chao R; Wang W-H; Chen P, "A Principle Component Analysis of Galaxy Properties from a Large, Gas-Selected Sample" , Advances in Astronomy: 2012, Article ID 208901, 2012 ( ADS | Fulltext )
  11. Chiang L-Y; Chen FF, "Direct measurement of the angular power spectrum of cosmic microwave background temperature anisotropies in the WMAP Data" , ApJ: 751(1), 43, May 20, 2012 [SCI] ( ADS | Fulltext )
  12. Coupon J; et al., "Galaxy clustering in the CFHTLS-Wide: the changing relationship between galaxies and haloes since z ~ 1.2" , A&A: 542, A5, June, 2012 [SCI] ( ADS | Fulltext )
  13. Hsieh B-C; Wang W-H; Hsieh C-C; Lin L; Yan H; Lim J; Ho PTP, "The Taiwan ECDFS Near-Infrared Survey: Ultra-Deep J and Ks Imaging in the Extended Chandra Deep Field-South" , ApJS: 203(2), 23-46, Dec, 2012 [SCI] ( ADS | Fulltext )
  14. Hsieh BC; Wang W-H; ...; Lin L; ...; Ho PTP; et al., "The Taiwan ECDFS Near-Infrared Survey: Very Bright End of the Luminosity Function at z>7" , ApJ: 749(1), 88-100, April 10, 2012 [SCI] ( ADS | Fulltext )
  15. Keenan RC; Barger AJ; Cowie LL; Wang W-H; et al., "Testing for a Large Local Void by Investigating the Normalization of the Near-Infrared Galaxy Luminosity Function at z ~ 0.1-0.3" , ApJ: 754(2), 131, Aug 1, 2012 [SCI] ( ADS | Fulltext )
  16. Lin Y-T; et al., "Baryon Content of Massive Galaxy Clusters at z=0-0.6" , ApJL: 745(1), L3, Jan 20, 2012 [SCI] ( ADS | Fulltext )
  17. Umetsu K; ...; Koch PM; Lin KY; Molnar SM; et al, "CLASH: Mass Distribution in and around MACS J1206.2-0847 from a Full Cluster Lensing Analysis" , ApJ: 755(1), 56, Aug 10, 2012 [SCI] ( ADS | Fulltext )
  18. Wang W-H; Barger AJ; Cowie LL, "A Ks and IRAC Selection of High-Redshift Extremely Red Objects" , ApJ: 744, 155, Jan, 2012 [SCI] ( ADS | Fulltext )
  19. Chiang L-Y; Chen FF, "Cross-power Spectrum and Its Application on Window Functions in the Wilkinson Microwave Anisotropy Probe Data" , ApJ: 738(2), 188, Sept 10, 2011 [SCI] ( ADS | Fulltext )
  20. Hota A*; ...; Ohyama Y; Konar C; ...; Matsushita S, "Discovery of a spiral-host episodic radio galaxy" , MNRAS: 417(1), L36-L40, Oct, 2011 [SCI] ( ADS | Fulltext )
  21. Okabe N; Bourdin H; Mazzotta P; et al., "Subaru Weak-lensing Study of A2163: Bimodal Mass Structure" , ApJ: 741(2), 116, Nov 10, 2011 [SCI] ( ADS | Fulltext )
  22. Umetsu K; Broadhurst T; Zitrin A; et al., "Cluster Mass Profiles from a Bayesian Analysis of Weak Lensing Distortion and Magnification Measurements: Applications to Subaru Data" , ApJ: 729(2), 127-142, Mar 10, 2011 [SCI] ( ADS | Fulltext )
  23. Umetsu K; Broadhurst T; Zitrin A; et al., "A Precise Cluster Mass Profile Averaged from the Highest Quality Lensing Data" , ApJ: 738(1), 41, Sept, 2011 [SCI] ( ADS | Fulltext )
  24. Wang W-H; Cowie LL; Barger AJ; et al., "SMA Observations of GOODS 850-11 and GOODS 850-13 — First Examples of Multiple Submillimeter Sources Resolved by an Interferometer" , ApJ: 726(2), L18, Jan 10, 2011 [SCI] ( ADS | Fulltext )
  25. Chang T-C; Pen UL; Bandura K; Peterson JB, "An intensity map of hydrogen 21-cm emission at redshift z approximate to 0.8" , Nature: 466(7305), 463-465, Jul 22, 2010 [SCI] ( ADS | Fulltext )
  26. Ho I-T; Wang W-H; Morrison G; Miller N, "Dust Obscuration in Lyman Break Galaxies at z~4" , ApJ: 722(2), 1051-1056, Oct 20, 2010 [SCI] ( ADS | Fulltext )
  27. Li CT; Kubo DY;...; Lin KY; Chen MT; Ho PTP; Chen CC; Han CC; Oshiro P; Martin-Cocher P; Chang CH; Chang SH; Altamirano P; Jiang H;...; Wang H; ...; Chang SW; Huang YD; Hwang YJ; ...; Koch P; Liu GC; Nishioka H; Umetsu K; Wei T; Wu JHP, "AMiBA Wideband Analog Correlator" , ApJ: 716(1), 746-757, June 10, 2010 [SCI] ( ADS | Fulltext )
  28. Liao Y-W; Wu J-HP; Ho PTP; Huang C-WL; Koch PM; Lin K-Y; Liu G-C; Molnar SM; Nishioka H; Umetsu K; Wang F-C; Altamirano P; Birkinshaw M; Chang C-H; Chang S-H; Chang S-W; Chen M-T; Chiueh T; Han C-C; Huang Y-D; Hwang Y-J; Jiang H; Kesteven M; Kubo DY; Li C-T; Martin-Cocher P;Oshiro P; Raffin P; Wei T; Wilson W, "AMiBA: Sunyaev-Zeldovich Effect Derived Properties and Scaling Relations of Massive Galaxy Clusters" , ApJ: 713(1), 584-591, APR 10 2010, 2010 [SCI] ( ADS | Fulltext )
  29. Liu G-C; Birkinshaw M; Wu J-HP; Ho PTP; Huang C-WL; Liao Y-W; Lin K-Y; Molnar SM; Nishioka H; Koch PM; Umetsu K; Wang F-C; Altamirano P; Chang C-H; Chang S-H; Chang S-W; Chen M-T; Han C-C; Huang Y-D; Hwang Y-J; Jiang H; Kestevan M; Kubo DY; Li C-T; Martin-Cocher P; Oshiro P; Raffin P; Wei T; Wilson W, "Contamination of the Central Sunyaev-Zel'dovich Decrements in AMiBA Galaxy Cluster Observations" , ApJ: 720(1), 608-613, Sept, 2010 [SCI] ( ADS | Fulltext )
  30. Molnar SM; Chiu I-N; Umetsu K; Chen P; Hearn N; Broadhurst T; Bryan G; Shang C, "Testing Strict Hydrostatic Equilibrium in Simulated Clusters of Galaxies: Implications to Abell 1689" , ApJ: 724(1), L1-L4, Nov 20, 2010 [SCI] ( ADS | Fulltext )
  31. Molnar SM; Umetsu K; ...; Ho PTP; ...; Koch PM; Liao YWV; Lin KY; Liu GC; Nishioka H; et al., "Constraining Intra-Cluster Gas Models with AMiBA13" , ApJ: 723(2), 1272-1285, Nov 10, 2010 [SCI] ( ADS | Fulltext )
  32. Okabe N; Okura Y; Futamase T, "Weak Lensing Mass Measurements of Substructures in COMA Cluster with Subaru/Suprime-Cam" , ApJ: 713(1), 291-303, April 10, 2010 [SCI] ( ADS | Fulltext )
  33. Okabe N; Takada M; Umetsu K; et al., "LoCuSS: Subaru Weak Lensing Study of 30 Galaxy Clusters" , PASJ: 62(3), 811-870, June 25, 2010 [SCI] ( ADS | Fulltext )
  34. Okabe N; Zhang Y-Y; Finoguenov A; Takada M; Smith GP; Umetsu K; Futamase T, "LoCuSS: Calibrating Mass-Observable Scaling Relations for Cluster Cosmology with Subaru Weak Lensing Observations" , ApJ: 721(1), 875-885, Sept, 2010 [SCI] ( ADS | Fulltext )
  35. Umetsu K; ...; Okabe N; Hsieh BC; Molnar SM, "The Mass Structure of the Galaxy Cluster Cl0024+1654 from a Full Lensing Analysis of Joint Subaru and ACS/NIC3 Observations" , ApJ: 714(2), 1470-1496, May 10, 2010 [SCI] ( ADS | Fulltext )
  36. Yamada M; Fujita Y; Matsuo H; Sugiyama N, "Search for the Sunyaev-Zel'dovich Effect in a Giant Radio Galaxy B1358+305" , AJ: 139(6), 2494-2503, June, 2010 [SCI] ( ADS | Fulltext )
  37. Yamazaki DG; Ichiki K; Kajino K; Mathews GJ, "New Constraints on the Primordial Magnetic Field" , Phys Rev D: 81(2), Art. No. 023008, Jan 15, 2010 [SCI] ( ADS | Fulltext )
  38. Yamazaki DG; Ichiki K; Kajino T; Mathews GJ, "Constraints on the neutrino mass and the primordial magnetic field from the matter density fluctuation parameter σ8" , Phys Rev D: 81(10), 103519, May 17, 2010 [SCI] ( ADS | Fulltext )
  39. Yamazaki DG*; Ichiki K; Kajino T; et al., "[Review Article] Primordial Magnetic Field Effects on the CMB and Large Scale Structure" , Advances in Astronomy: 2010(586590), 1-19, Dec, 2010 ( ADS | Fulltext )
  40. Chiang L-Y; Naselsky PD; Coles P, "Cosmic Covariance and the Low Quadrupole Anisotropy of the Wilkinson Microwave Anisotropy Probe (WMAP) Data" , ApJ: 694(1), 339-343, March 20, 2009 [SCI] ( ADS | Fulltext )
  41. Ho PTP; Altamirano P; Chang CH; Chang SH; et al., "The Yuan-Tseh Lee Array for Microwave Background Anisotropy" , ApJ: 694(2), 1610-1618, April 1, 2009 [SCI] ( ADS | Fulltext )
  42. Molnar SM; Hearn N; Haiman Z; Bryan G; et al., "Accretion Shocks in Clusters of Galaxies and Their SZ Signature from Cosmological Simulations" , ApJ: 696(2), 1640-1656, May 10, 2009 [SCI] ( ADS | Fulltext )
  43. Nishioka H; ...; Ho PTP; Koch PM; Lin K-Y; et al., "Tests of AMiBA Data Integrity" , ApJ: 694(2), 1637-1642, Apr 1, 2009 [SCI] ( ADS | Fulltext )
  44. Umetsu K; ...; Liu GC; Ho PTP; Koch PM; et al., "Mass and Hot Baryons in Massive Galaxy Clusters from Subaru Weak Lensing and AMiBA Sunyaev-Zel'dovich Effect Observations" , ApJ: 694(2), 1643-1663, Apr 1, 2009 [SCI] ( ADS | Fulltext )
  45. Chiang LY; Naselsky PD; Coles P, "Cosmic covariance and the low quadrupole anisotropy in the WMAP data" , MPLA: 23(17-20), 1489-1497, Jun 28, 2008 [SCI] ( ADS | Fulltext )
  46. Ho PTP; Altimirano P;...; Chang S-W; Chang C-H; Chen MT; et al., "The Yuan Tseh Lee AMiBA Project" , MPLA: 23(20), 1243-1251, June, 2008 [SCI] ( ADS | Fulltext )
  47. Hsieh BC; Yee HKC; Lin H; Gladders MD;et al., "Pair Analysis of Field Galaxies from the Red-Sequence Cluster Survey" , ApJ: 683(1), 33-44, Aug 10, 2008 [SCI] ( ADS | Fulltext )
  48. Lin L; Patton DR Patton; Koo DC; ...; Hsieh BC; et al., "The Redshift Evolution of Wet, Dry, and Mixed Galaxy Mergers from Close Galaxy Pairs in the DEEP2 Galaxy Redshift Survey" , ApJ: 681(1), 232-243, July 1, 2008 [SCI] ( ADS | Fulltext )
  49. Liu HY; Hsieh BC; Ho PTP; Lin L; et al., "A New Galaxy Group Finding Algorithm: Probability Friends-of-Friends" , ApJ: 681(2), 1046-1057, July 10, 2008 [SCI] ( ADS | Fulltext )
  50. Muller S; Wu S-Y; Hsieh B-C; Gonzalez RA; et al., "Searching for dust in the intracluster medium from reddening of background galaxies" , ApJ: 680(2), 975-980, Jun 20, 2008 [SCI] ( ADS | Fulltext )
  51. Umetsu K; Broadhurst T, "Combining Lens Distortion and Depletion to Map the Mass Distribution of A1689" , ApJ: 684(1), 177-203, September 1, 2008 [SCI] ( ADS | Fulltext )
  52. Umetsu K; Okura Y; Futamase T, "A Moment Method for Measuring the Higher-Order Weak Gravitational Lensing Effects" , MPLA: 23(17-20), 1506-1513, June, 2008 [SCI] ( ADS | Fulltext )
  53. Chiang L-Y; Naselsky PD, "Phase analysis of the cosmic microwave background from an incomplete sky coverage" , MNRAS: 380(1), L71-L74, Sep 1, 2007 [SCI] ( ADS | Fulltext )
  54. Chiang L-Y; Naselsky PD; Coles P, "Departure from Gaussianity of the Cosmic Microwave Background Temperature Anisotropies in the Three-Year WMAP Data" , ApJ: 664(1), 8-13, Jul 20, 2007 [SCI] ( ADS | Fulltext )
  55. Ng KW, "Some issues in CMB polarization observation" , MPLA: 22(25-28), 1901-1910, Sep 14, 2007 [SCI] ( ADS | Fulltext )
  56. Umetsu K; Takada M; Broadhurst T, "Probing the Cluster Mass Distribution using Subaru Weak Lensing Data" , MPLA: 22(25-28), 2099-2106, Sept 14, 2007 [SCI] ( ADS | Fulltext )
  57. Liu G-C; Lee S; Ng K-W, "Effect on Cosmic Microwave Background Polarization of Coupling of Quintessence to Pseudoscalar Formed from the Electromagnetic Field and its Dual" , Phys Rev Lett: 97(16), 161303, Oct 20, 2006 [SCI] ( ADS | Fulltext )
  58. Hsieh BC; Yee HKC; Lin H; et al., "A photometric redshift galaxy catalog from the Red-Sequence Cluster Survey" , ApJS: 158(2), 161-177, Jun, 2005 [SCI] ( ADS | Fulltext )
  59. Liu G-C; da Silva A; Aghanim N, "Primordial Quadrupole-induced Polarization from Filamentary Structures and Galaxy Clusters" , ApJ: 621(1), 15-21, Mar, 2005 [SCI] ( ADS | Fulltext )
  60. Ng KW, "Full-sky correlation functions for CMB experiments with asymmetric window functions" , Phys Rev D: 71(8), 083009, Apr, 2005 [SCI] ( ADS | Fulltext )
  61. Umetsu K; Tanaka M; Kodama T; et al., "Discovery of a Stronglly Lensed Galaxy at z=3.9 behind a z=0.83 Galaxy Cluster" , PASJ: 57(6), 877-880, Dec, 2005 [SCI] ( ADS | Fulltext )
  62. Ho PTP; Chen M-T; ...; Chiueh T; Chu T-H; Jiang H; Koch P; Kubo D; Li C-T; ...; Lin K-Y; Liu G-C; Lo K-Y; Ma C-J; Martin RN; Ng K-W; Nishioka H; Patt F; ...; Wang H; Hwang Y-J; Umetsu K; et al., "The AMiBA Project" , MPLA: 19(13-16), 993-1000, May 30, 2004 [SCI] ( ADS | Fulltext )
  63. Lin K-Y; Woo T-P; Tseng Y-H; Lin L; Chiueh T, "Effects of Preheated Clusters on the Cosmic Microwave Background Spectrum" , ApJ: 608(1), L1-L4, Jun 10, 2004 [SCI] ( ADS | Fulltext )
  64. Lin K-Y; Woo T-P; Tseng Y-H; Lin L; Chiueh T, "Clusters in Preheating Simulation and its Effect on CMB Spectrum" , MPLA: 19(13-16), 1035-1038, May 30, 2004 [SCI] ( ADS | Fulltext )
  65. Umetsu K; Chiueh T; Lin K-Y; Wu J-M; Tseng Y-H, "Simulation of a Combined SZE and Weak Lensing Cluster Survey for AMiBA Experiment" , MPLA: 19(13-16), 1027-1030, May 30, 2004 [SCI] ( ADS | Fulltext )
  66. Chiueh T; Lee J; Lin L, "An analytical approach to the spin distribution of dark halos" , ApJ: 581(2), 794-798, Dec 20, 2002 [SCI] ( ADS | Fulltext )
  67. Chiueh T; Ma CJ, "The annulus-filtered E and B modes in cosmic microwave background radiation polarization" , ApJ: 578(1), 12-24, Oct 10, 2002 [SCI] ( ADS | Fulltext )
  68. Kawasaki W; Totani T, "Positional coincidence between the high-latitude steady unidentified gamma-ray sources and possibly merging clusters of galaxies" , ApJ: 576(2), 679-687, Sep 10, 2002 [SCI] ( ADS | Fulltext )
  69. Lee J; Pen UL, "Detection of galaxy spin alignments in the point source catalog redshift survey shear field" , ApJ: 567(2), L111-L114, Mar 10, 2002 [SCI] ( ADS | Fulltext )
  70. Wu XP; Xue YJ, "The effect of radiative cooling on the scale dependence of the global stellar and gas content of groups and clusters of galaxies" , ApJ: 572(1), L19-L22, Jun 10, 2002 [SCI] ( ADS | Fulltext )
  71. Fan ZH; Chiueh TH, "Determining the geometry and the cosmological parameters of the universe through Sunyaev-Zeldovich effect cluster counts" , ApJ: 550(2), 547-553, Apr 1, 2001 [SCI] ( ADS | Fulltext )
  72. Liu GC; Sugiyama N; Benson AJ; et al, "Polarization of the cosmic microwave background from nonuniform reionization" , ApJ: 561(2), 504-516, Nov 10, 2001 [SCI] ( ADS | Fulltext )
  73. Ng KW, "Complex visibilities of cosmic microwave background anisotropies" , Phys Rev D: 63(12), 123001, Jun 15, 2001 [SCI] ( ADS | Fulltext )
  74. Fan ZH; Chiueh T, "Influence of the environmental dark matter on QSO-cluster associations and on cluster mass estimates" , ApJ: 538(1), 1-10, Jul 20, 2000 [SCI] ( ADS | Fulltext )
  75. Lee J; Pen UL, "Cosmic shear from galaxy spins" , ApJ: 532(1), L5-L8, Mar 20, 2000 [SCI] ( ADS | Fulltext )
  76. Leon S; Meylan G; Combes F, "Tidal tails around 20 Galactic globular clusters - Observational evidence for gravitational disk/bulge shocking" , A&A: 359(3), 907-931, Jul, 2000 [SCI] ( ADS | Fulltext )
  77. Lee J; Shandarin SF, "Comparison of analytical mass functions with numerical simulations" , ApJ: 517(1), L5-L8, May 20, 1999 [SCI] ( ADS | Fulltext )
  78. Ng KW, "Tensor-induced CMB temperature-polarization correlation in reionized universes" , Phys Rev D: 60(4), 047302, Aug 15, 1999 [SCI] ( ADS | Fulltext )
  79. Chen LW; Fabian AC; Gendreau C, "ASCA and ROSAT observations of the QSF3 field: the X-ray background in the 0.1-7 keV band" , MNRAS: 285(3), 449-471, Mar 1, 1997 [SCI] ( ADS | Fulltext )
  80. Benjamin J; Van Waerbeke L; Heymans C; ...; Coupon J; et al., "CFHTLenS tomographic weak lensing: quantifying accurate redshift distributions" , MNRAS: 431(2), 1547-1564, May, 2013 [SCI] ( ADS | Fulltext )
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