| Issue Date | Title | Author(s) | Relation | scopus | WOS | Fulltext/Archive link |
| 2004 | Simulation of a Combined SZE and Weak Lensing Cluster Survey for AMiBA Experiment | Umetsu, K; Chiueh, T; Lin, K-Y; Wu, J-M; Tseng, Y-H | MODERN PHYSICS LETTERS A 19(13-16), 1027-1030 | | | |
| 2011 | Strong-Lensing Analysis of MS 1358.4+6245: New Multiple Images and Implications for the Well-Resolved z=4.92 Galaxy | Zitrin, A; Broaodhurst, T; Coe, D; Liesenborgs, J; Benítez, N; Rephaeli, Y; Ford, Y; Umetsu, K | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (413) 1753-1763 | | | |
| 2008 | Subaru Weak Lensing Study of Seven Merging Clusters of Galaxies: Distributions of Mass and Baryon | Okabe, N; Umetsu, K | PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN 60(2), 345-375 | | | |
| 2013 | The Contribution of Radio Galaxy Contamination to Measurements of the Sunyaev-Zel'dovich Decrement in Massive Galaxy Clusters at 140 GHz with Bolocam | Sayers, J; Koch, PM; Lin, KY; Umetsu, K | ASTROPHYSICAL JOURNAL 764(2), 152 | | | |
| 2005 | The Mass Profile of A1689 from a Lensing Analysis of Deep Subaru Images | Umetsu, K; Takada, M; Broadhurst, T; Kong, X | Journal of the Korean Astronomical Society 38(2), 191-195 | | | |
| 2010 | The Mass Structure of the Galaxy Cluster Cl0024+1654 from a Full Lensing Analysis of Joint Subaru and ACS/NIC3 Observations | Umetsu, K; Okabe, N; Hsieh, BC; Molnar, SM | ASTROPHYSICAL JOURNAL 714(2), 1470-1496 | | | |
| 2003 | The Topology of a Weak Lensing Field in the Neighborhood of MS 1054-03 | Sato, J; Umetsu, K; Futamase, T; Yamada, T | ASTROPHYSICAL JOURNAL 582(2), L67-L70 | | | |
| 2012 | The Universal Einstein Radius Distribution from 10,000 SDSS Clusters | Zitrin, A; Broadhurst, T; Bartelmann, M; Rephaeli, Y; Oguri, M; Benitez, N; Hao, J; Umetsu, K | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 423(3), 2308-2324 | | | |
| 2011 | Weak and Stong Lensing Analysis of the Trixial Matter Distribution of A1689 | Sereno, M; Umetsu, K | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 416(4), 3187-3200 | | | |
