{"id":18502,"date":"2026-09-01T11:15:24","date_gmt":"2026-09-01T02:15:24","guid":{"rendered":"https:\/\/www.icrr.u-tokyo.ac.jp\/?post_type=co_worker&#038;p=18502"},"modified":"2026-09-01T11:15:24","modified_gmt":"2026-09-01T02:15:24","slug":"list-of-fy2025-inter-university-research-program-international-3-2","status":"publish","type":"co_worker","link":"https:\/\/www.icrr.u-tokyo.ac.jp\/en\/co_worker\/18502\/","title":{"rendered":"List of FY2026 Inter-University Research Program (International)"},"content":{"rendered":"\r\n<h3 class=\"wp-block-heading\">Neutrino and Astroparticle Division<\/h3>\r\n\r\n\r\n\r\n<figure class=\"wp-block-table\">\r\n<table>\r\n<thead>\r\n<tr>\r\n<th>Ref. Num<br \/>ber<\/th>\r\n<th>Affiliation<\/th>\r\n<th>Department<\/th>\r\n<th>Job Title<\/th>\r\n<th>Principal Investigator<\/th>\r\n<th>Research Proposal<\/th>\r\n<th>New\/Ongoing<\/th>\r\n<\/tr>\r\n<\/thead>\r\n<tbody>\r\n<tr>\r\n<td>A1<\/td>\r\n<td>Gwangju Institute of Science and Technology<\/td>\r\n<td>Department of Physics and Photon Science<\/td>\r\n<td>\u8b1b\u5e2b<\/td>\r\n<td>Jang Jee-seung<\/td>\r\n<td>Water Transparency Measurement in Super Kamiokande<\/td>\r\n<td>New<\/td>\r\n<\/tr>\r\n<tr>\r\n<td>A2<\/td>\r\n<td>ILANCE Laboratory<\/td>\r\n<td><\/td>\r\n<td>\u6559\u6388<\/td>\r\n<td>Gonin Michel<\/td>\r\n<td>Study of supernova neutrinos in Super-Kamiokande<\/td>\r\n<td>Ongoing<\/td>\r\n<\/tr>\r\n<tr>\r\n<td>A3<\/td>\r\n<td>University Autonoma Madrid<\/td>\r\n<td>Depto. Theoretical Physics<\/td>\r\n<td>\u6559\u6388<\/td>\r\n<td>Labarga Luis<\/td>\r\n<td>Data Taking, Calibrations, Measurements and Analysis with Super-Kamiokande I &#8211; VIII<\/td>\r\n<td>Ongoing<\/td>\r\n<\/tr>\r\n<tr>\r\n<td>A4<\/td>\r\n<td>\u30ad\u30f3\u30b0\u30b9\u30ab\u30ec\u30c3\u30b8\u30ed\u30f3\u30c9\u30f3<\/td>\r\n<td><\/td>\r\n<td>\u51c6\u6559\u6388<\/td>\r\n<td>\u9999\u53d6 \u54f2\u5e73<\/td>\r\n<td>\u30b9\u30fc\u30d1\u30fc\u30ab\u30df\u30aa\u30ab\u30f3\u30c7\u5916\u6c34\u69fd\u3067\u4f7f\u3046\u30ad\u30e3\u30ea\u30d6\u30ec\u30fc\u30b7\u30e7\u30f3\u30ec\u30fc\u30b6\u30fc\u306e\u8a2d\u7f6e\u3068\u904b\u55b6<\/td>\r\n<td>Ongoing<\/td>\r\n<\/tr>\r\n<tr>\r\n<td>A5<\/td>\r\n<td>\u30ad\u30f3\u30b0\u30b9\u30ab\u30ec\u30c3\u30b8\u30ed\u30f3\u30c9\u30f3<\/td>\r\n<td><\/td>\r\n<td>\u51c6\u6559\u6388<\/td>\r\n<td>\u9999\u53d6 \u54f2\u5e73<\/td>\r\n<td>\u30cf\u30a4\u30d1\u30fc\u30ab\u30df\u30aa\u30ab\u30f3\u30c7\u5916\u6c34\u69fd\u691c\u51fa\u5668\u306e\u5236\u4f5c\u3068\u8a2d\u7f6e<\/td>\r\n<td>New<\/td>\r\n<\/tr>\r\n<tr>\r\n<td>B1<\/td>\r\n<td>University of Birmingham<\/td>\r\n<td>School of Physics and Astronomy<\/td>\r\n<td>\u6559\u6388<\/td>\r\n<td>Nikolopoulos Konstantinos<\/td>\r\n<td>Towards a multiphysics liquid Xe TPC with scintillation and charge multiplication readouts<\/td>\r\n<td>Ongoing<\/td>\r\n<\/tr>\r\n<\/tbody>\r\n<\/table>\r\n<\/figure>\r\n\r\n\r\n\r\n<h3 class=\"wp-block-heading\">High Energy Cosmic Ray Division<\/h3>\r\n\r\n\r\n\r\n<figure class=\"wp-block-table\">\r\n<table>\r\n<thead>\r\n<tr>\r\n<th>Ref. Num<br \/>ber<\/th>\r\n<th><strong>Affiliation<\/strong><\/th>\r\n<th><strong>Department<\/strong><\/th>\r\n<th><strong>Job Title<\/strong><\/th>\r\n<th><strong>Principal Investigator<\/strong><\/th>\r\n<th><strong>Research Proposal<\/strong><\/th>\r\n<th>New\/Ongoing<\/th>\r\n<\/tr>\r\n<\/thead>\r\n<tbody>\r\n<tr>\r\n<td>F1<\/td>\r\n<td>Institute for Nuclear Research of the Russian Academy of Sciences<\/td>\r\n<td><\/td>\r\n<td>Deputy director<\/td>\r\n<td>Rubtsov Grigory<\/td>\r\n<td>Ultra-high-energy cosmic-ray origin studies with the Telescope Array and TAx4 surface detector<\/td>\r\n<td>Ongoing<\/td>\r\n<\/tr>\r\n<tr>\r\n<td>F2<\/td>\r\n<td>Academia Sinica<\/td>\r\n<td>High-Energy Theory Group (HETG)<\/td>\r\n<td>\u52a9\u6559<\/td>\r\n<td>Fedynitch Anatoli<\/td>\r\n<td>TA\u5b9f\u9a13\u3067\u53d6\u5f97\u3057\u305f\u4e8b\u8c61\u3068\u6a5f\u68b0\u5b66\u7fd2\u624b\u6cd5\u3092\u7528\u3044\u305f\u8d85\u9ad8\u30a8\u30cd\u30eb\u30ae\u30fc\u5b87\u5b99\u7dda\u306e\u8d77\u6e90\u63a2\u7d22<\/td>\r\n<td>Ongoing<\/td>\r\n<\/tr>\r\n<tr>\r\n<td>F3<\/td>\r\n<td>Sungkyunkwan university<\/td>\r\n<td>Department of Physics<\/td>\r\n<td>\u51c6\u6559\u6388<\/td>\r\n<td>Lee MyeongJae<\/td>\r\n<td>\u300c\u30c6\u30ec\u30b9\u30b3\u30fc\u30d7\u30a2\u30ec\u30a4\u300d\u691c\u51fa\u5668\u3092\u7528\u3044\u305f\u78c1\u6c17\u5358\u6975\u5b50\u5b87\u5b99\u7dda\u306e\u63a2\u7d22<\/td>\r\n<td>New<\/td>\r\n<\/tr>\r\n<tr>\r\n<td>F4<\/td>\r\n<td>University of Utah<\/td>\r\n<td>Department of Physics and Astronomy<\/td>\r\n<td>\u6559\u6388<\/td>\r\n<td>Matthews John<\/td>\r\n<td>Comparison of the response and reconstruction of the Telescope Array and Auger Surface Detectors<\/td>\r\n<td>New<\/td>\r\n<\/tr>\r\n<tr>\r\n<td>F5<\/td>\r\n<td>\u4e2d\u56fd\u79d1\u5b66\u9662\u56fd\u5bb6\u5929\u6587\u53f0<\/td>\r\n<td><\/td>\r\n<td>\u6559\u6388<\/td>\r\n<td>\u9673 \u9f0e<\/td>\r\n<td>Study of high-energy cosmic rays at a high altitude in Tibet, China<\/td>\r\n<td>Ongoing<\/td>\r\n<\/tr>\r\n<tr>\r\n<td>F6<\/td>\r\n<td>Universidad Mayor de San Andr\u00e9s<\/td>\r\n<td>Instituto de Investigaciones F\u00edsicas<\/td>\r\n<td>\u6559\u6388<\/td>\r\n<td>Miranda Pedro<\/td>\r\n<td>Study for Galactic CR origin using the ALPACA air shower array in Bolivia<\/td>\r\n<td>Ongoing<\/td>\r\n<\/tr>\r\n<tr>\r\n<td>F7<\/td>\r\n<td>Universidad de Guadalajara<\/td>\r\n<td>Departamento de Fisica<\/td>\r\n<td>\u7814\u7a76\u54e1<\/td>\r\n<td>de la Fuente Acosta Eduardo<\/td>\r\n<td>Constraining the nature of the emission in PeVatrons observed by Alpaca.<\/td>\r\n<td>Ongoing<\/td>\r\n<\/tr>\r\n<tr>\r\n<td>F8<\/td>\r\n<td>Universidad Mayor de San Andres<\/td>\r\n<td><\/td>\r\n<td>\u6559\u6388<\/td>\r\n<td>Subieta Vasquez Martin<\/td>\r\n<td>ALPACA\u5b9f\u9a13\u306e\u305f\u3081\u306e\u8868\u9762\u6c34\u30c1\u30a7\u30ec\u30f3\u30b3\u30d5\u691c\u51fa\u5668\u306e\u958b\u767a\u3068\u30b3\u30df\u30c3\u30b7\u30e7\u30cb\u30f3\u30b0<\/td>\r\n<td>New<\/td>\r\n<\/tr>\r\n<\/tbody>\r\n<\/table>\r\n<\/figure>\r\n\r\n\r\n\r\n<h3 class=\"wp-block-heading\">Astrophysics and Gravity Division<\/h3>\r\n\r\n\r\n\r\n<figure class=\"wp-block-table\">\r\n<table>\r\n<thead>\r\n<tr>\r\n<th>Ref. Num<br \/>ber<\/th>\r\n<th><strong>Affiliation<\/strong><\/th>\r\n<th><strong>Department<\/strong><\/th>\r\n<th><strong>Job Title<\/strong><\/th>\r\n<th><strong>Principal Investigator<\/strong><\/th>\r\n<th><strong>Research Proposal<\/strong><\/th>\r\n<th>New\/Ongoing<\/th>\r\n<\/tr>\r\n<\/thead>\r\n<tbody>\r\n<tr>\r\n<td>G1<\/td>\r\n<td>National Tsing Hua University<\/td>\r\n<td><\/td>\r\n<td>\u6559\u6388<\/td>\r\n<td>Lee Ray-Kuang<\/td>\r\n<td>Quantum Noise Reduction for KAGRA<\/td>\r\n<td>Ongoing<\/td>\r\n<\/tr>\r\n<tr>\r\n<td>G2<\/td>\r\n<td>Phenikaa University<\/td>\r\n<td>The Phenikaa Institute for Advanced Study<\/td>\r\n<td>\u51c6\u6559\u6388<\/td>\r\n<td>Nguyen Quynh-Lan<\/td>\r\n<td>Self interacting dark matter and gravitational waves<\/td>\r\n<td>Ongoing<\/td>\r\n<\/tr>\r\n<tr>\r\n<td>G3<\/td>\r\n<td>University of Perugia<\/td>\r\n<td>Department of Physics and Geology<\/td>\r\n<td>\u51c6\u6559\u6388<\/td>\r\n<td>Bawaj Mateusz<\/td>\r\n<td>Position control system for silicon monolithic suspension in cryogenic gravitational waves detectors.<\/td>\r\n<td>Ongoing<\/td>\r\n<\/tr>\r\n<tr>\r\n<td>G4<\/td>\r\n<td>ShanghaiTech University<\/td>\r\n<td>School of Physical Science and Technology<\/td>\r\n<td>\u52a9\u6559<\/td>\r\n<td>Chou Chia-Jui<\/td>\r\n<td>Noise Subtraction of KAGRA O4 Data<\/td>\r\n<td>Ongoing<\/td>\r\n<\/tr>\r\n<tr>\r\n<td>G5<\/td>\r\n<td>\u56fd\u7acb\u6e05\u83ef\u5927\u5b66<\/td>\r\n<td>\u5929\u6587\u5b66\u7814\u7a76\u6240<\/td>\r\n<td>\u7814\u7a76\u54e1<\/td>\r\n<td>\u6797 \u7950\u7fa4<\/td>\r\n<td>Low-Latency Localization and Parameter Estimation of Gravitational Waves Using Probabilistic Deep Learning<\/td>\r\n<td>Ongoing<\/td>\r\n<\/tr>\r\n<tr>\r\n<td>G6<\/td>\r\n<td>Tamkang University<\/td>\r\n<td>Department of Physics<\/td>\r\n<td>\u6559\u6388<\/td>\r\n<td>Liu Guo Chin<\/td>\r\n<td>\u78ba\u7387\u7684\u91cd\u529b\u6ce2\u80cc\u666f\u306e\u624b\u6cd5\u691c\u8a3c\u304a\u3088\u3073\u7269\u7406\u7684\u7814\u7a76<\/td>\r\n<td>Ongoing<\/td>\r\n<\/tr>\r\n<tr>\r\n<td>G7<\/td>\r\n<td>National Tsing Hua University<\/td>\r\n<td>Institute of Astronomy<\/td>\r\n<td>\u6559\u6388<\/td>\r\n<td>Kong Albert<\/td>\r\n<td>Improving parameter estimation of gravitational wave events using KAGRA data<\/td>\r\n<td>New<\/td>\r\n<\/tr>\r\n<tr>\r\n<td>G8<\/td>\r\n<td>National Tsing Hua University<\/td>\r\n<td>Institute of Astronomy<\/td>\r\n<td>Postdoctoral Researcher<\/td>\r\n<td>SAHA SUROJIT<\/td>\r\n<td>\u7269\u7406\u60c5\u5831\u306b\u57fa\u3065\u304f\u30cb\u30e5\u30fc\u30e9\u30eb\u30cd\u30c3\u30c8\u30ef\u30fc\u30af\u306e\u5b9f\u88c5\u306b\u3088\u308b\u30d0\u30a4\u30aa\u30ea\u30f3\u306e\u5171\u9cf4\u30e2\u30fc\u30c9\u4f4e\u6e1b<\/td>\r\n<td>New<\/td>\r\n<\/tr>\r\n<tr>\r\n<td>G9<\/td>\r\n<td>Beijing Normal University<\/td>\r\n<td>School of Physics and Astronomy<\/td>\r\n<td>\u6559\u6388<\/td>\r\n<td>Zhu Xingjiang<\/td>\r\n<td>Searching for a Gravitational-Wave Background with KAGRA and Next-Generation Detectors<\/td>\r\n<td>New<\/td>\r\n<\/tr>\r\n<tr>\r\n<td>G10<\/td>\r\n<td>Ewha Womans University<\/td>\r\n<td>Physics<\/td>\r\n<td>\u51c6\u6559\u6388<\/td>\r\n<td>Kim Chunglee<\/td>\r\n<td>KAGRA\u3092\u6d3b\u7528\u3057\u305f\u91cd\u529b\u6ce2\u5929\u6587\u5b66\u304a\u3088\u3073\u691c\u51fa\u5668\u7279\u6027\u8a55\u4fa1<\/td>\r\n<td>New<\/td>\r\n<\/tr>\r\n<tr>\r\n<td>G11<\/td>\r\n<td>National Cheng-Kung University<\/td>\r\n<td>Physics Department<\/td>\r\n<td>\u7279\u4efb\u51c6\u6559\u6388<\/td>\r\n<td>Lin Chun-Che (Lupin)<\/td>\r\n<td>\u91cd\u529b\u6ce2\u30a4\u30d9\u30f3\u30c8\u306e\u5929\u7a7a\u4f4d\u7f6e\u7279\u5b9a\u306b\u95a2\u3059\u308b\u6a5f\u68b0\u5b66\u7fd2\u306b\u3088\u308b\u8abf\u67fb<\/td>\r\n<td>New<\/td>\r\n<\/tr>\r\n<tr>\r\n<td>G12<\/td>\r\n<td>Chungnam National University<\/td>\r\n<td>Department of Astronomy &amp; Space Science<\/td>\r\n<td>\u6559\u6388<\/td>\r\n<td>David Hui<\/td>\r\n<td>De-noising KAGRA data with seqARIMA and search for possible gravitational wave signals<\/td>\r\n<td>New<\/td>\r\n<\/tr>\r\n<tr>\r\n<td>G13<\/td>\r\n<td>Yonsei University<\/td>\r\n<td>Department of physcis<\/td>\r\n<td>\u52a9\u6559<\/td>\r\n<td>Park June Gyu<\/td>\r\n<td>Heterodyne Interferometer design for Test Mass Birefringence Characterization<\/td>\r\n<td>New<\/td>\r\n<\/tr>\r\n<\/tbody>\r\n<\/table>\r\n<\/figure>\r\n\r\n\r\n\r\n<h3 class=\"wp-block-heading\">Research Center for Cosmic Neutrinos\uff08RCCN)<\/h3>\r\n\r\n\r\n\r\n<figure class=\"wp-block-table\">\r\n<table>\r\n<thead>\r\n<tr>\r\n<th>Ref. Number<\/th>\r\n<th>Affiliation<\/th>\r\n<th>Department<\/th>\r\n<th>Job Title<\/th>\r\n<th>Principal Investigator<\/th>\r\n<th>Research Proposal<\/th>\r\n<th>New\/Ongoing<\/th>\r\n<\/tr>\r\n<\/thead>\r\n<tbody>\r\n<tr>\r\n<td>J1<\/td>\r\n<td>University of Seville<\/td>\r\n<td>Department of Atomic, Molecular and Nuclear Physics<\/td>\r\n<td>\u51c6\u6559\u6388<\/td>\r\n<td>Guillermo Megias<\/td>\r\n<td>Constraining systematics at T2K and SuperKamiokande oscillation analyses using neutrino-nucleus interaction models<\/td>\r\n<td>Ongoing<\/td>\r\n<\/tr>\r\n<tr>\r\n<td>J2<\/td>\r\n<td>Istituto Nazionale di Fisica Nucleare INFN<\/td>\r\n<td>Sezione di Bari<\/td>\r\n<td>Senior Postdoctoral researcher<\/td>\r\n<td>Ospina Nataly<\/td>\r\n<td>Development and optimisation of event selection for Long-Baseline neutrino interactions in the Hyper-Kamiokande Far Detector<\/td>\r\n<td>New<\/td>\r\n<\/tr>\r\n<\/tbody>\r\n<\/table>\r\n<\/figure>\r\n\r\n\r\n\r\n<p>&nbsp;<\/p>\r\n","protected":false},"featured_media":0,"template":"","taxo_co_worker":[36,38,42],"tag_news":[],"tag_year":[102],"class_list":["post-18502","co_worker","type-co_worker","status-publish","hentry","taxo_co_worker-research-results","taxo_co_worker-international-inter-university-research","taxo_co_worker-research-titles-and-results","tag_year-102","en-US"],"aioseo_notices":[],"_links":{"self":[{"href":"https:\/\/www.icrr.u-tokyo.ac.jp\/wp-json\/wp\/v2\/co_worker\/18502","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.icrr.u-tokyo.ac.jp\/wp-json\/wp\/v2\/co_worker"}],"about":[{"href":"https:\/\/www.icrr.u-tokyo.ac.jp\/wp-json\/wp\/v2\/types\/co_worker"}],"wp:attachment":[{"href":"https:\/\/www.icrr.u-tokyo.ac.jp\/wp-json\/wp\/v2\/media?parent=18502"}],"wp:term":[{"taxonomy":"taxo_co_worker","embeddable":true,"href":"https:\/\/www.icrr.u-tokyo.ac.jp\/wp-json\/wp\/v2\/taxo_co_worker?post=18502"},{"taxonomy":"tag_news","embeddable":true,"href":"https:\/\/www.icrr.u-tokyo.ac.jp\/wp-json\/wp\/v2\/tag_news?post=18502"},{"taxonomy":"tag_year","embeddable":true,"href":"https:\/\/www.icrr.u-tokyo.ac.jp\/wp-json\/wp\/v2\/tag_year?post=18502"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}