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2013 Yao-Yuan Mao

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, Louis E. Strigari

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, Risa H. Wechsler

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, Hao-Yi Wu, Oliver Hahn

Halo-To-Halo Similarity and Scatter in the Velocity Distribution of Dark Matter

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Hao-Yi Wu, Oliver Hahn, Risa H. Wechsler

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, Peter S. Behroozi

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Rhapsody. I. Structural Properties and Formation History From a Statistical Sample of Re-Simulated Cluster-Size Halos

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2012 Ting-Wai Chiu, Tung-Han Hsieh, Yao-Yuan Mao

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Pseudoscalar meson in two flavors QCD with the optimal domain-wall fermion

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2011 Ting-Wai Chiu, Tung-Han Hsieh, Yao-Yuan Mao

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Topological susceptibility in two flavors lattice QCD with the optimal domain-wall fermion

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Ting-Wai Chiu, Tung-Han Hsieh, Yao-Yuan Mao

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, Kenji Ogawa

GPU-Based Conjugate Gradient Solver for Lattice QCD with Domain-Wall Fermions

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Yu-Chih Chen, Ting-Wai Chiu, Tian-Shin Guu, Tung-Han Hsieh, Chao-Hsi Huang, Yao-Yuan Mao

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Lattice QCD with Optimal Domain-Wall Fermion: Light Meson Spectroscopy

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Tung-Han Hsieh, Ting-Wai Chiu, Yao-Yuan Mao

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Topological Charge in Two Flavors QCD with Optimal Domain-Wall Fermion

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2010 Wei-Shu Hou, Yao-Yuan Mao

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, Chia-Hsien Shen

Leading effect ofCPviolation with four generations

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2009 Yao-Yuan Mao

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, Ting-Wai Chiu

Topological susceptibility to the one-loop order in chiral perturbation theory

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Chin-Fei Lee, Yao-Yuan Mao

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, Bo Reipurth

ERRATUM: “INFALL AND ROTATION MOTIONS IN THE HH 111 PROTOSTELLAR SYSTEM: A FLATTENED ENVELOPE IN TRANSITION TO a DISK” (2009, ApJ, 694, 1395)

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Chin-Fei Lee, Yao-Yuan Mao

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, Bo Reipurth

Infall and Rotation Motions in the Hh 111 Protostellar System: A Flattened Envelope in Transition to a Disk?

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This paper was not found in any repository; the policy of its publisher is unknown or unclear.

1970 Ethan O. Nadler, Risa H. Wechsler

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, Keith Bechtol, Yao-Yuan Mao

ORCID

, Gregory Green

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, Alex Drlica-Wagner, Mitch McNanna, Sidney Mau, Andrew B. Pace, J. D. Simon, Andrey Kravtsov, Scott Dodelson, T. S. Li, Alexander H. Riley, Mei-Yu Wang and 56 other authors

Milky Way Satellite Census -- II. Galaxy-Halo Connection Constraints Including the Impact of the Large Magellanic Cloud

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