Anh Phan
University of Wisconsin-Madison
5 Papers
33 Citations
Anh Phan is an academic researcher from University of Wisconsin-Madison. The author has contributed to research in topics: Hubble's law & Markov chain Monte Carlo. The author has an hindex of 2, co-authored 5 publications. Previous affiliations of Anh Phan include Utah Valley University.
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Papers
The Tianlai Dish Pathfinder Array: design, operation and performance of a prototype transit radio interferometer
Fengquan Wu,Jixia Li,Shifan Zuo,Shifan Zuo,Xuelei Chen,Xuelei Chen,Santanu Das,Santanu Das,John Marriner,Trevor M. Oxholm,Anh Phan,Albert Stebbins,Peter T. Timbie,R. Ansari,Jean-Eric Campagne,Zhiping Chen,Yanping Cong,Qizhi Huang,Juhun Kwak,Yichao Li,Tao Liu,Yingfeng Liu,Chenhui Niu,Calvin Osinga,Olivier Perdereau,Jeffrey B. Peterson,John Podczerwinski,Huli Shi,Gage Siebert,Shijie Sun,Haijun Tian,Gregory S. Tucker,Qunxiong Wang,Rongli Wang,Yougang Wang,Yanlin Wu,Yidong Xu,Kaifeng Yu,Zijie Yu,Jiao Zhang,Juyong Zhang,Jialu Zhu +41 more
TL;DR: The Tianlai Dish Pathfinder Array as mentioned in this paper is a radio interferometer designed to test techniques for 21cm intensity mapping in the post-reionization universe as a means for measuring large-scale cosmic structure.
41
Infrared Surface Brightness Fluctuation Distances for MASSIVE and Type Ia Supernova Host Galaxies
Joseph B. Jensen,John Blakeslee,Chung-Pei Ma,Peter A. Milne,Peter J. Brown,Michele Cantiello,Peter M. Garnavich,Jenny E. Greene,John R. Lucey,Anh Phan,R. Brent Tully,Charlotte M. Wood +11 more
TL;DR: In this paper, the surface brightness fluctuation (SBF) method was used to measure the distances to galaxies with evolved stellar populations out to 100 Mpc and constraining the local value of the Hubble constant.
25
Cosmic Microwave Background Anisotropy numerical solution (CMBAns) I: An introduction to $C_l$ calculation
Santanu Das,Santanu Das,Anh Phan +2 more
TL;DR: CMBAns as mentioned in this paper is a cosmological Boltzmann code that can be used for accurate calculation of the CMB power spectrum, which is mostly written in the C language.
5
Cosmic Microwave Background Anisotropy numerical solution (CMBAns) I: An introduction to $C_l$ calculation.
Santanu Das,Anh Phan +1 more
TL;DR: All the mathematical formulation, approximation schemes, integration methods etc., that are used in CMBAns, a new cosmological Boltzmann code that can be used for accurate calculation of the CMB power spectrum are discussed.
Infrared Surface Brightness Fluctuation Distances for MASSIVE and Type Ia Supernova Host Galaxies
Joseph B. Jensen,John Blakeslee,Chung-Pei Ma,Peter A. Milne,Peter J. Brown,Michele Cantiello,Peter M. Garnavich,Jenny E. Greene,John R. Lucey,Anh Phan,R. Brent Tully,Charlotte M. Wood +11 more
TL;DR: In this article, the surface brightness fluctuation (SBF) method was used to measure the distances to galaxies with evolved stellar populations out to 100 Mpc and constraining the local value of the Hubble constant.