{"id":147,"date":"2024-05-15T18:48:51","date_gmt":"2024-05-15T09:48:51","guid":{"rendered":"https:\/\/www.physics.okayama-u.ac.jp\/ishino-lab\/details\/wordpress\/product\/web\/?page_id=147"},"modified":"2025-11-20T11:26:35","modified_gmt":"2025-11-20T02:26:35","slug":"talks","status":"publish","type":"page","link":"https:\/\/www.physics.okayama-u.ac.jp\/ishino-lab\/details\/wordpress\/product\/web\/achievement\/talks\/","title":{"rendered":"\u5b66\u4f1a\u767a\u8868"},"content":{"rendered":"\n

2025<\/mark><\/h2>\n\n\n\n
Second International Conference on the Physics of the Two Infinities<\/a><\/td>11\u670817\u65e5 – 11\u670821\u65e5
Koshiba Hall Hongo Campus, University of Tokyo<\/td>		Hybrid Delta-map: Combining Harmonic and Real-space Methods for CMB Foreground Removal<\/td>\u751f\u718a\u6e05<\/td><\/tr>
\u7b2c14\u56de\u89b3\u6e2c\u7684\u5b87\u5b99\u8ad6\u30ef\u30fc\u30af\u30b7\u30c3\u30d7<\/a><\/td>10\u67086\u65e5 – 10\u67088\u65e5, \u5ca1\u5c71\u30b3\u30f3\u30d9\u30f3\u30b7\u30e7\u30f3\u30bb\u30f3\u30bf\u30fc<\/td>CMB\u5927\u89d2\u5ea6\u30b9\u30b1\u30fc\u30eb\u504f\u5149\u89b3\u6e2c\u306e\u610f\u7fa9\u3068\u5b9f\u9a13\u8a08\u753b<\/td>\u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
MPA Cosmology Seminar II<\/a><\/td>10\u670814\u65e5, Max Planck Institute for Astrophysics<\/td>Delta-map Bayes: Accounting for Spatially Varying Foreground Spectra in CMB B-mode Polarization<\/td>\u751f\u718a\u6e05<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a2025\u5e74\u7b2c80\u56de\u5e74\u6b21\u5927\u4f1a<\/a><\/td>9\u670819\u65e5, \u5e83\u5cf6\u5927\u5b66<\/td>\u96fb\u5b50\u30cb\u30e5\u30fc\u30c8\u30ea\u30ce\u691c\u51fa\u3092\u76ee\u6a19\u3068\u3057\u305f\u30a4\u30f3\u30b8\u30a6\u30e0\u6a19\u7684\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668MKID\u306e\u7279\u6027\u8a55\u4fa1<\/td>\u67ff\u6728\u5065\u675c<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a2025\u5e74\u7b2c80\u56de\u5e74\u6b21\u5927\u4f1a<\/a><\/td>9\u670819\u65e5, \u5e83\u5cf6\u5927\u5b66<\/td>FPGA\u3092\u7528\u3044\u305f\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668MKID\u7528\u8aad\u307f\u51fa\u3057DAQ\u30b7\u30b9\u30c6\u30e0\u306e\u958b\u767a\u304a\u3088\u3073\u6e2c\u5b9a<\/td>\u6a0b\u53e3\u5149\u5b8f<\/td><\/tr>
CMB\u504f\u5149\u89b3\u6e2c\u3068\u524d\u666f\u653e\u5c04\u306e\u7406\u89e3\u3068\u91cd\u8981\u6027<\/a><\/td>9\u670818\u65e5 – 9\u670819\u65e5, \u540d\u53e4\u5c4b\u5927\u5b66<\/td>CMB\u504f\u5149\u89b3\u6e2c\u3068\u524d\u666f\u653e\u5c04\u306e\u7406\u89e3\u3068\u91cd\u8981\u6027<\/td>\u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a2025\u5e74\u7b2c80\u56de\u5e74\u6b21\u5927\u4f1a<\/a><\/td>9\u670816\u65e5, \u5e83\u5cf6\u5927\u5b66<\/td>\u30df\u30ea\u6ce2\u5149\u5b66\u7d20\u5b50\u306b\u5411\u3051\u305f\u8d85\u77ed\u30d1\u30eb\u30b9\u30ec\u30fc\u30b6\u30fc\u52a0\u5de5\u3067\u4f5c\u88fd\u3059\u308b\u516d\u89d2\u683c\u5b50\u30e2\u30b9\u30a2\u30a4\u53cd\u5c04\u9632\u6b62\u69cb\u9020<\/td>\u9ad8\u4e45\u8ad2\u592a<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a2025\u5e74\u7b2c80\u56de\u5e74\u6b21\u5927\u4f1a<\/a><\/td>9\u670816\u65e5, \u5e83\u5cf6\u5927\u5b66<\/td>\u65b0\u898f\u624b\u6cd5 Hybrid Delta-map:\u7403\u9762\u8abf\u548c\u30c6\u30f3\u30d7\u30ec\u30fc\u30c8\u3068\u5b9f\u7a7a\u9593\u89e3\u6790\u3092\u878d\u5408\u3057\u305f\u5927\u89d2\u5ea6\u30b9\u30b1\u30fc\u30ebCMB\u524d\u666f\u653e\u5c04\u9664\u53bb<\/td>\u751f\u718a\u6e05<\/td><\/tr>
KEK\u6e2c\u5b9a\u5668\u958b\u767a\u30bb\u30f3\u30bf\u30fc\u30d7\u30e9\u30c3\u30c8\u30d5\u30a9\u30fc\u30e0 D\u30ad\u30c3\u30af\u30aa\u30d5\u30df\u30fc\u30c6\u30a3\u30f3\u30b0<\/a><\/td>9\u67081\u65e5 – 9\u67082\u65e5, KEK \u3064\u304f\u3070<\/td>\u8d85\u4f1d\u5c0e\u3068\u5fae\u7d30\u52a0\u5de5\u6280\u8853\u3092\u7d44\u307f\u5408\u308f\u305b\u305f\u691c\u51fa\u5668\u306e\u958b\u767a<\/td>\u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
Low Temperature Detector Conference 2025<\/a><\/td>6\u67081-7\u65e5 Santa Fe, USA<\/td>Development of Electron Neutrino Detectors Using MKID and Indium Targets with Micro-Machined Mask<\/td>Ryota Takaku<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a2025\u5e74\u6625\u5b63<\/a>\u5927\u4f1a<\/a><\/td>3\u670821\u65e5\u3000\u30aa\u30f3\u30e9\u30a4\u30f3<\/td>\u96fb\u5b50\u30cb\u30e5\u30fc\u30c8\u30ea\u30ce\u691c\u51fa\u3092\u76ee\u6307\u3059\u30a4\u30f3\u30b8\u30a6\u30e0\u6a19\u7684\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668\u306e\u958b\u767a\u3068\u6027\u80fd\u8a55\u4fa1<\/td>\u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a2025\u5e74\u6625\u5b63\u5927\u4f1a<\/a><\/td>3\u670821\u65e5\u3000\u30aa\u30f3\u30e9\u30a4\u30f3<\/td>CMB\u504f\u5149\u89b3\u6e2c\u306b\u304a\u3051\u308bDelta-map\u524d\u666f\u653e\u5c04\u9664\u53bb\u6cd5\u306e\u9032\u5c55\u3068\u65b0\u305f\u306a\u5c55\u958b<\/td>\u751f\u718a\u6e05<\/td><\/tr>
CMB B-mode – NEXT<\/a><\/td>1\u670827-29\u65e5, KEK<\/td>Systematic effects mitigation by spin moment decomposition<\/td>\u9ad9\u702c\u7950\u4ecb<\/td><\/tr>
CMB B-mode – NEXT<\/a><\/td>1\u670827-29\u65e5, KEK<\/td>HWP and systematics effects with asymmetric beams<\/td>\u9577\u91ce\u4f51\u54c9<\/td><\/tr>
CMB B-mode – NEXT<\/a><\/td>1\u670827-29\u65e5, KEK<\/td>Foreground Cleaning – Delta Maps<\/td>\u751f\u718a\u6e05<\/td><\/tr><\/tbody><\/table><\/figure>\n\n\n\n

2024<\/mark><\/h2>\n\n\n\n
The 37th International Symposium on Superconductivity ISS2024<\/a><\/td>12\u67085\u65e5
\u91d1\u6ca2\u6587\u5316\u30db\u30fc\u30eb<\/td>		Superconducting detectors, the universe, and elementary particles<\/a><\/td>Hirokazu Ishino<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a2024\u5e74\u7b2c79\u56de\u5e74\u6b21\u5927\u4f1a<\/a><\/td>9\u670818\u65e5
\u5317\u6d77\u9053\u5927\u5b66<\/td>		FPGA\u3092\u7528\u3044\u305f\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668\u7528\u8aad\u307f\u51fa\u3057DAQ\u30b7\u30b9\u30c6\u30e0\u306e\u958b\u767a<\/td>\u6a0b\u53e3\u5149\u5b8f<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a2024\u5e74\u7b2c79\u56de\u5e74\u6b21\u5927\u4f1a<\/a><\/td>9\u670818\u65e5
\u5317\u6d77\u9053\u5927\u5b66<\/td>		\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668MKID\u3092\u7528\u3044\u305f\u30a4\u30f3\u30b8\u30a6\u30e0\u6a19\u7684\u30cb\u30e5\u30fc\u30c8\u30ea\u30ce\u691c\u51fa\u5668\u306e\u8a66\u4f5c\u6a5f\u6027\u80fd\u8a55\u4fa1<\/td>\u5927\u524d\u9f8d\u4e8c<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a2024\u5e74\u7b2c79\u56de\u5e74\u6b21\u5927\u4f1a<\/a><\/td>9\u670819\u65e5
\u5317\u6d77\u9053\u5927\u5b66<\/td>		CMB\u504f\u5149\u89b3\u6e2c\u306b\u304a\u3051\u308b\u691c\u51fa\u5229\u5f97\u306e\u6642\u9593\u5909\u5316\u306b\u8d77\u56e0\u3059\u308b\u7cfb\u7d71\u8aa4\u5dee\u306e\u7814\u7a76<\/td>\u5965\u6751\u4fca\u8f14<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a2024\u5e74\u7b2c79\u56de\u5e74\u6b21\u5927\u4f1a<\/a><\/td>9\u670819\u65e5
\u5317\u6d77\u9053\u5927\u5b66<\/td>		CMB\u504f\u5149\u89b3\u6e2c\u306e\u305f\u3081\u306e\u5e83\u89d2\u5ea6\u30b9\u30b1\u30fc\u30eb\u524d\u666f\u653e\u5c04\u9664\u53bb\u306b\u5411\u3051\u305f\u65b0\u3057\u3044\u878d\u5408\u624b\u6cd5\u306e\u958b\u767a<\/td>\u751f\u718a\u6e05<\/td><\/tr>
\n
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a2024\u5e74\u6625\u5b63\u5927\u4f1a<\/a>\n<\/td>		3\u670819\u65e5\u3000\u30aa\u30f3\u30e9\u30a4\u30f3

<\/td>		\nCMB\u5168\u5929\u504f\u5149\u89b3\u6e2c\u306b\u304a\u3051\u308b\u691c\u51fa\u5668\u5229\u5f97\u306e\u7cfb\u7d71\u8aa4\u5dee\u306e\u89e3\u6790\u7684\u8a08\u7b97\n<\/td>\u68ee\u6c38\u771f\u672b<\/td><\/tr>
\n
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a2024\u5e74\u6625\u5b63\u5927\u4f1a<\/a>\n<\/td>		3\u670819\u65e5\u3000\u30aa\u30f3\u30e9\u30a4\u30f3

<\/td>		\nCMB\u504f\u5149\u89b3\u6e2c\u5b9f\u9a13\u306e\u9ad8\u611f\u5ea6\u5316\u306b\u5411\u3051\u305f\u65b0\u305f\u306a\u5168\u5929\u5730\u56f3\u4f5c\u6210\u6cd5\u306e\u7814\u7a76\uff0d\u30b9\u30d4\u30f3\u3092\u7528\u3044\u305f\u7cfb\u7d71\u7684\u52b9\u679c\u306e\u5206\u96e2\uff0d\n<\/td>\u9ad8\u702c\u7950\u4ecb<\/td><\/tr>
\n
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a2024\u5e74\u6625\u5b63\u5927\u4f1a<\/a>\n<\/td>		3\u670819\u65e5\u3000\u30aa\u30f3\u30e9\u30a4\u30f3

<\/td>		\nCMB\u504f\u5149\u89b3\u6e2c\u5b9f\u9a13\u306b\u304a\u3051\u308b\u524d\u666f\u653e\u5c04\u9664\u53bb\u6cd5Delta-map\u306e\u30de\u30eb\u30c1\u30af\u30e9\u30b9\u30bf\u30ea\u30f3\u30b0\u5316\u306e\u958b\u767a\n<\/td>\u751f\u718a\u6e05<\/td><\/tr>
\n
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a2024\u5e74\u6625\u5b63\u5927\u4f1a<\/a>\n<\/td>		3\u670819\u65e5\u3000\u30aa\u30f3\u30e9\u30a4\u30f3

<\/td>		\n\u6642\u9593\u4f9d\u5b58\u6027\u306e\u3042\u308b\u30d3\u30fc\u30e0\u306e\u5f62\u72b6\u5909\u5316\u304cCMB\u306eB\u30e2\u30fc\u30c9\u504f\u5149\u89b3\u6e2c\u306b\u4e0e\u3048\u308b\u7cfb\u7d71\u8aa4\u5dee\u306b\u3064\u3044\u3066\u306e\u7814\u7a76\n<\/td>\u9577\u91ce\u4f51\u54c9<\/td><\/tr>
\n
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a2024\u5e74\u6625\u5b63\u5927\u4f1a<\/a>\n<\/td>		3\u670819\u65e5\u3000\u30aa\u30f3\u30e9\u30a4\u30f3

<\/td>		\n\u5916\u6765\u653e\u5c04\u7dda\u306b\u3088\u308b\u5f71\u97ff\u3092\u6392\u9664\u3057\u305f\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668\u306e\u958b\u767a\n<\/td>\u5927\u524d\u9f8d\u4e8c<\/td><\/tr><\/tbody><\/table><\/figure>\n\n\n\n

2023<\/font><\/a><\/h2>\n\n\n\n
\n
\nIPNS workshop \u7d20\u7c92\u5b50\u7269\u7406\u306e\u4eca\u3068\u672a\u6765<\/a>\n<\/td>		12\u670821-23\u65e5\u3001\u9ad8\u30a8\u30cd\u7814

<\/td>		\nCMB\u5b9f\u9a13\u306e\u73fe\u72b6\u3068\u4eca\u5f8c\u306e\u5c55\u671b\n<\/td>\u685c\u4e95\u96c4\u57fa<\/td><\/tr>
\n
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a\u3000\u7b2c78\u56de\u5e74\u6b21\u5927\u4f1a<\/a>\n<\/td>		9\u670817\u65e5\u3001\u6771\u5317\u5927\u5b66

<\/td>		\nCMB\u306e\u5168\u5929\u89b3\u6e2c\u306b\u304a\u3051\u308b\u6307\u5411\u65b9\u5411\u4e0d\u5b9a\u6027\u306e\u7cfb\u7d71\u7684\u8aa4\u5dee\u306e\u8a55\u4fa1\n<\/td>\u68ee\u6c38\u771f\u672a<\/td><\/tr>
\n
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a\u3000\u7b2c78\u56de\u5e74\u6b21\u5927\u4f1a<\/a>\n<\/td>		9\u670817\u65e5\u3001\u6771\u5317\u5927\u5b66

<\/td>		\nCMB\u89b3\u6e2c\u885b\u661f\u306b\u642d\u8f09\u3055\u308c\u308b\u504f\u5149\u5909\u8abf\u5668\u306b\u7528\u3044\u308b\u5e83\u5e2f\u57df\u534a\u6ce2\u9577\u677f\u306e\u6700\u9069\u5316\u306e\u7814\u7a76\n<\/td>\u751f\u718a\u6e05<\/td><\/tr>
\n
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a\u3000\u7b2c78\u56de\u5e74\u6b21\u5927\u4f1a<\/a>\n<\/td>		9\u670817\u65e5\u3001\u6771\u5317\u5927\u5b66

<\/td>		\nCMB\u89b3\u6e2c\u885b\u661f\u306b\u304a\u3051\u308b\u504f\u5149\u5909\u8abf\u5668\u642d\u8f09\u7528\u306e\u8fd1\u8d64\u5916\u30c0\u30a4\u30aa\u30fc\u30c9\u5f0f\u5149\u5b66\u30a8\u30f3\u30b3\u30fc\u30c0\u306e\u653e\u5c04\u7dda\u30fb\u4f4e\u6e29\u74b0\u5883\u7279\u6027\n<\/td>\u690d\u677e\u4ee4\u592a<\/td><\/tr>
\n
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a\u3000\u7b2c78\u56de\u5e74\u6b21\u5927\u4f1a<\/a>\n<\/td>		9\u670817\u65e5\u3001\u6771\u5317\u5927\u5b66

<\/td>		\nLiteBIRD\u885b\u661f\u306b\u304a\u3051\u308b\u30b9\u30ad\u30e3\u30f3\u6226\u7565\u306e\u591a\u6b21\u5143\u6700\u9069\u5316\n<\/td>\u9ad9\u702c\u7950\u4ecb<\/td><\/tr>
\n
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a\u3000\u7b2c78\u56de\u5e74\u6b21\u5927\u4f1a<\/a>\n<\/td>		9\u670817\u65e5\u3001\u6771\u5317\u5927\u5b66

<\/td>		\n\u30d3\u30fc\u30e0\u5f62\u72b6\u3068HWP\u306e\u4e0d\u5b9a\u6027\u304cCMB\u306eB\u30e2\u30fc\u30c9\u504f\u5149\u89b3\u6e2c\u306b\u4e0e\u3048\u308b\u7cfb\u7d71\u8aa4\u5dee\u306b\u3064\u3044\u3066\u306e\u7814\u7a76\n<\/td>\u9577\u91ce\u4f51\u54c9<\/td><\/tr>
\n
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a\u3000\u7b2c78\u56de\u5e74\u6b21\u5927\u4f1a<\/a>\n<\/td>		9\u670818\u65e5\u3001\u6771\u5317\u5927\u5b66

<\/td>		\n\u96fb\u5b50\u30cb\u30e5\u30fc\u30c8\u30ea\u30ce\u691c\u51fa\u3092\u76ee\u6307\u3057\u305f\u30a4\u30f3\u30b8\u30a6\u30e0\u6a19\u7684\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668MKID\u306e\u8a66\u4f5c\u6a5f\u5fdc\u7b54\u8a55\u4fa1\n<\/td>\u5927\u524d\u9f8d\u4e8c,<\/td><\/tr>
\nColloquium, Oslo University\n<\/td> 25th of Aug., Oslo, Norway,

<\/td>		\nFredagskollokvium: Dr. Strangedata or: How I learned to start worrying and hate cosmic rays\n<\/td>Samantha Stever<\/td><\/tr>
\n
\nLow Temperature Detector (LTD20)\n<\/td>		 25th of July, Daejon Korea,

<\/td>		\nDevelopment of electron neutrino detector system using superconducting detector and microfabrication support materials(Poster)\n<\/td>Ryuji Omae<\/td><\/tr>
\n
\nLow Temperature Detector (LTD20)\n<\/td>		 24th of July, Daejon Korea,

<\/td>		\nUpdated forecasts of cosmic ray systematic effects and a new filtering method for the LiteBIRD space mission (Poster)\n<\/td>Samantha Stever<\/td><\/tr>
\nFrom the Galaxy to the Big Bang, Banyuls-sur-mer, France\n<\/td> 16th of June, Orsay, France,

<\/td>		\nDr. Strangedata or: How I learned to start worrying and hate cosmic rays\n<\/td>Samantha Stever<\/td><\/tr>
\nseminar, Institut d\u2019Astrophysique Spatiale [Institute for space astrophysics]\n<\/td> 24th of May, Orsay, France,

<\/td>		\nCosmic rays, primordial B-modes, and DRACULA\n<\/td>Samantha Stever<\/td><\/tr>
\n
\n2nd Japan Canadian Frontier of Science (JCFoS) Symposium,<\/a>\n<\/td>		 March 2023, Banff, Canada,

<\/td>		\nExploring the origin of the universe ~ Cosmic Microwave Background Experiment ~\n<\/td>Yuki Sakurai<\/td><\/tr>
\n
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a\u30002023\u5e74\u6625\u5b63\u5927\u4f1a<\/a>\n<\/td>		3\u670825\u65e5\u3001\u30aa\u30f3\u30e9\u30a4\u30f3

<\/td>		\nCMB\u89b3\u6e2c\u885b\u661f\u306b\u304a\u3051\u308b\u504f\u5149\u5909\u8abf\u5668\u642d\u8f09\u7528\u5149\u5b66\u30a8\u30f3\u30b3\u30fc\u30c0\u306e\u305f\u3081\u306e\u8fd1\u8d64\u5916\u30c0\u30a4\u30aa\u30fc\u30c9\u306e\u653e\u5c04\u7dda\u30fb\u4f4e\u6e29\u74b0\u5883\u7279\u6027\n<\/td>\u690d\u677e\u4ee4\u592a<\/td><\/tr>
\n
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a\u30002023\u5e74\u6625\u5b63\u5927\u4f1a<\/a>\n<\/td>		3\u670825\u65e5\u3001\u30aa\u30f3\u30e9\u30a4\u30f3

<\/td>		\nCMB\u504f\u5149\u89b3\u6e2c\u306b\u304a\u3051\u308b\u30b9\u30d4\u30f3\u56de\u8ee2\u5bfe\u79f0\u6027\u3092\u7528\u3044\u305f\u7cfb\u7d71\u8aa4\u5dee\u89e3\u6790\u624b\u6cd5\u306e\u7814\u7a76\n<\/td>\u9ad9\u702c\u7950\u4ecb<\/td><\/tr>
\n
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a\u30002023\u5e74\u6625\u5b63\u5927\u4f1a<\/a>\n<\/td>		3\u670825\u65e5\u3001\u30aa\u30f3\u30e9\u30a4\u30f3

<\/td>		\nCMB\u306eB\u30e2\u30fc\u30c9\u504f\u5149\u89b3\u6e2c\u306b\u304a\u3051\u308b\u30d3\u30fc\u30e0\u306e\u5927\u89d2\u5ea6\u69cb\u9020\u7531\u6765\u306e\u7cfb\u7d71\u8aa4\u5dee\u306e\u7814\u7a76\n<\/td>\u9577\u91ce\u4f51\u54c9<\/td><\/tr>
\n
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a\u30002023\u5e74\u6625\u5b63\u5927\u4f1a<\/a>\n<\/td>		3\u670825\u65e5\u3001\u30aa\u30f3\u30e9\u30a4\u30f3

<\/td>		\n\u96fb\u5b50\u30cb\u30e5\u30fc\u30c8\u30ea\u30ce\u691c\u51fa\u3092\u76ee\u6307\u3057\u305f\u30a4\u30f3\u30b8\u30a6\u30e0\u6a19\u7684\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668MKID\u306e\u4f5c\u88fd\u3068\u6027\u80fd\u8a55\u4fa1\n<\/td>\u5927\u524d\u9f8d\u4e8c<\/td><\/tr><\/tbody><\/table><\/figure>\n\n\n\n

2022<\/font><\/a><\/h2>\n\n\n\n
\n
\n\u8d85\u4f1d\u5c0e\u30a8\u30ec\u30af\u30c8\u30ed\u30cb\u30af\u30b9\u7814\u7a76\u4f1a<\/a>\n<\/td>		11\u67084\u65e5\u3001\u6771\u5317\u5927\u5b66\uff0b\u30aa\u30f3\u30e9\u30a4\u30f3

<\/td>		\n\u96fb\u5b50\u30cb\u30e5\u30fc\u30c8\u30ea\u30ce\u691c\u51fa\u3092\u76ee\u7684\u3068\u3057\u305f\u30a4\u30f3\u30b8\u30a6\u30e0\u6a19\u7684\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668\u306e\u958b\u767a\n<\/td>\u98a8\u65e9\u548c\u4e5f\u3001\u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
\n
\nExploration of Particle Physics and Cosmology with Neutrino, Kyoto University<\/a>\n<\/td>		11\u67081\u65e5\u3001\u4eac\u90fd\u5927\u5b66

<\/td>		\nDevelopment of a novel electron neutrino detection system with a combination
\nof superconducting detectors and microstructure forming system\n<\/td>		Hirokazu Ishino<\/td><\/tr>
\n
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a\u3000\u7b2c77\u56de\u79cb\u5b63\u5927\u4f1a<\/a>\n<\/td>		9\u67086\u65e5\u3001\u5ca1\u5c71\u7406\u79d1\u5927\u5b66

<\/td>		\n\u7cfb\u7d71\u7684\u52b9\u679c\u306e\u56de\u8ee2\u5bfe\u79f0\u6027\u89e3\u6790\u3092\u7528\u3044\u305fLiteBIRD\u885b\u661f\u306e\u6700\u9069\u6383\u5f15\u624b\u6cd5\u306e\u63a2\u7d22\n<\/td>\u9ad8\u702c\u7950\u4ecb<\/td><\/tr>
\n
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a\u3000\u7b2c77\u56de\u79cb\u5b63\u5927\u4f1a<\/a>\n<\/td>		9\u67086\u65e5\u3001\u5ca1\u5c71\u7406\u79d1\u5927\u5b66

<\/td>		\nCMB\u89b3\u6e2c\u885b\u661f\u642d\u8f09\u306e\u5149\u5b66\u30a8\u30f3\u30b3\u30fc\u30c0\u3068\u3057\u3066\u306e\u8fd1\u8d64\u5916\u30c0\u30a4\u30aa\u30fc\u30c9\u306e\u653e\u5c04\u7dda\u8010\u6027\n<\/td>\u690d\u677e\u4ee4\u592a<\/td><\/tr>
\n
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a\u3000\u7b2c77\u56de\u79cb\u5b63\u5927\u4f1a<\/a>\n<\/td>		9\u67086\u65e5\u3001\u5ca1\u5c71\u7406\u79d1\u5927\u5b66

<\/td>		\n\u5e83\u5929\u57df\u3067\u306eCMB\u504f\u5149\u89b3\u6e2c\u5b9f\u9a13\u306b\u304a\u3051\u308b1\/f\u3086\u3089\u304e\u306e\u5f71\u97ff\u306b\u95a2\u3059\u308b\u6e96\u89e3\u6790\u7684\u7814\u7a76\n<\/td>\u77f3\u5742\u9ad8\u8f1d<\/td><\/tr>
\n
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a\u3000\u7b2c77\u56de\u79cb\u5b63\u5927\u4f1a<\/a>\n<\/td>		9\u67088\u65e5\u3001\u5ca1\u5c71\u7406\u79d1\u5927\u5b66

<\/td>		In\u6a19\u7684\u96fb\u5b50\u30cb\u30e5\u30fc\u30c8\u30ea\u30ce\u691c\u51fa\u3092\u76ee\u6307\u3057\u305f\u5fae\u7d30\u52a0\u5de5\u30de\u30b9\u30af\u4ed8\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668\u306e\u958b\u767a\n<\/td>\u98a8\u65e9\u548c\u4e5f<\/td><\/tr>
\n
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a\u3000\u7b2c77\u56de\u79cb\u5b63\u5927\u4f1a<\/a>\n<\/td>		9\u67088\u65e5\u3001\u5ca1\u5c71\u7406\u79d1\u5927\u5b66

<\/td>		In\u6a19\u7684\u96fb\u5b50\u30cb\u30e5\u30fc\u30c8\u30ea\u30ce\u691c\u51fa\u3092\u76ee\u6307\u3057\u305f\u5fae\u7d30\u52a0\u5de5\u30de\u30b9\u30af\u4ed8\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668\u306e\u958b\u767a\n<\/td>\u98a8\u65e9\u548c\u4e5f<\/td><\/tr>
\n
\nSPIE Astronomical Telescope + Instrumentation<\/a>\n<\/td>		7\u670817-22\u65e5\u3001Montreal, Canada

<\/td>		\nInstrumental Performance and Scientific Requirements of Polarization Modulation Unit for LiteBIRD low frequency telescope\n<\/td>Yuki Sakurai<\/td><\/tr>
\n
\nUpcoming CMB observations and Cosmology<\/a>\n<\/td>		3\u670823\u65e5\u3001\u4eac\u90fd\u5927\u5b66\u57fa\u7814 (\u62db\u5f85\u8b1b\u6f14)

<\/td>		\n\u6b21\u4e16\u4ee3CMB\u504f\u5149\u89b3\u6e2c\u5b9f\u9a13\u306b\u304a\u3051\u308b\u504f\u5149\u5909\u8abf\u6280\u8853\n<\/td>\u685c\u4e95\u96c4\u57fa<\/td><\/tr>
\n
\nPTEP\u3000\u30d5\u30ec\u30f3\u30c9\u30b7\u30c3\u30d7\u30df\u30fc\u30c6\u30a3\u30f3\u30b0 <\/a>\n<\/td>		3\u670818\u65e5\u3001\u30aa\u30f3\u30e9\u30a4\u30f3(\u62db\u5f85\u8b1b\u6f14)

<\/td>		\n\u5b87\u5b99\u306e\u71b1\u3044\u30d3\u30c3\u30af\u30d0\u30f3\u306e\u524d\u3092\u63a2\u308b\u30df\u30ea\u6ce2\u504f\u5149\u5168\u5929\u89b3\u6e2c\u885b\u661f LiteBIRD\n<\/td>\u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
\n
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a\u3000\u7b2c77\u56de\u5e74\u6b21\u5927\u4f1a<\/a>\n<\/td>		3\u670816\u65e5\u3001\u30aa\u30f3\u30e9\u30a4\u30f3

<\/td>		\nCMB\u504f\u5149\u89b3\u6e2c\u5b9f\u9a13\u306b\u304a\u3051\u308b\u5229\u5f97\u53ca\u3073\u6307\u5411\u65b9\u5411\u306e\u4e0d\u5b9a\u6027\u3092\u8d77\u6e90\u3068\u3059\u308b\u7cfb\u7d71\u8aa4\u5dee\u306e\u89e3\u6790\u7684\u7814\u7a76\n<\/td>\u77f3\u5742\u9ad8\u8f1d<\/td><\/tr>
\n
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a\u3000\u7b2c77\u56de\u5e74\u6b21\u5927\u4f1a<\/a>\n<\/td>		3\u670816\u65e5\u3001\u30aa\u30f3\u30e9\u30a4\u30f3

<\/td>		\n\u8d85\u4f1d\u5c0e\u6280\u8853\u3068\u5fae\u7d30\u69cb\u9020\u5f62\u6210\u6280\u8853\u3092\u7d44\u307f\u5408\u308f\u305b\u305f\u96fb\u5b50\u30cb\u30e5\u30fc\u30c8\u30ea\u30ce\u691c\u51fa\u5668\u306e\u958b\u767a\n<\/td>\u98a8\u65e9\u548c\u4e5f<\/td><\/tr>
\n
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a\u3000\u7b2c77\u56de\u5e74\u6b21\u5927\u4f1a<\/a>\n<\/td>		3\u670816\u65e5\u3001\u30aa\u30f3\u30e9\u30a4\u30f3

<\/td>		\nCMB\u504f\u5149\u89b3\u6e2c\u885b\u661fLiteBIRD\u306b\u304a\u3051\u308b\u9023\u7d9a\u56de\u8ee2\u534a\u6ce2\u9577\u677f\u306b\u540c\u671f\u3059\u308b\u7cfb\u7d71\u8aa4\u5dee\u306e\u7814\u7a76\n<\/td>\u685c\u4e95\u96c4\u57fa<\/td><\/tr>
\n
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a\u3000\u7b2c77\u56de\u5e74\u6b21\u5927\u4f1a<\/a>\n<\/td>		3\u670816\u65e5\u3001\u30aa\u30f3\u30e9\u30a4\u30f3

<\/td>		\nCryogenic characterisation of Transition Edge Sensors for the LiteBIRD space mission and their susceptibility to cosmic rays\n<\/td>Stever Samantha Lynn<\/td><\/tr>
\n
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a\u3000\u7b2c77\u56de\u5e74\u6b21\u5927\u4f1a<\/a>\n<\/td>		3\u670816\u65e5\u3001\u30aa\u30f3\u30e9\u30a4\u30f3

<\/td>		\nCMB\u504f\u5149\u7cbe\u5bc6\u89b3\u6e2c\u885b\u661fLiteBIRD\u306b\u304a\u3051\u308b\u5168\u5929\u89b3\u6e2c\u624b\u6cd5\u306e\u6700\u9069\u5316 -\u7cfb\u7d71\u8aa4\u5dee\u306e\u6291\u5236\u3068\u8f03\u6b63\u3092\u53ef\u80fd\u306b\u3059\u308b\u30b9\u30ad\u30e3\u30f3\u6226\u7565\u306e\u63a2\u7d22-\n<\/td>\u9ad9\u702c\u7950\u4ecb<\/td><\/tr>
\n
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a\u3000\u7b2c77\u56de\u5e74\u6b21\u5927\u4f1a<\/a>\n<\/td>		3\u670816\u65e5\u3001\u30aa\u30f3\u30e9\u30a4\u30f3

<\/td>		\nCMB\u5168\u5929\u504f\u5149\u89b3\u6e2c\u306b\u304a\u3051\u308b4\u03c0\u30d3\u30fc\u30e0\u306e\u975e\u5bfe\u79f0\u6027\u3068\u8f03\u6b63\u7cbe\u5ea6\u306b\u7531\u6765\u3059\u308b\u7cfb\u7d71\u8aa4\u5dee\u306e\u7814\u7a76\n<\/td>\u9577\u91ce\u4f51\u54c9<\/td><\/tr>
\n
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a\u3000\u7b2c77\u56de\u5e74\u6b21\u5927\u4f1a<\/a>\n<\/td>		3\u670816\u65e5\u3001\u30aa\u30f3\u30e9\u30a4\u30f3

<\/td>		\n\u8907\u6570\u691c\u51fa\u5668\u3067\u306e\u89b3\u6e2c\u3092\u8003\u616e\u3057\u305fCMB\u5168\u5929\u504f\u5149\u89b3\u6e2c\u306b\u304a\u3051\u308b\u6307\u5411\u4f4d\u7f6e\u306e\u4e0d\u5b9a\u6027\u306b\u3088\u308b\u7cfb\u7d71\u7684\u52b9\u679c\u306e\u7814\u7a76\n<\/td>\u571f\u5c45\u76f4\u4e5f<\/td><\/tr>
\n
\n\u7b2c22\u56de\u5b87\u5b99\u79d1\u5b66\u30b7\u30f3\u30dd\u30b8\u30a6\u30e0<\/a>\n<\/td>		1\u67086-7\u65e5\u3001\u30aa\u30f3\u30e9\u30a4\u30f3

<\/td>		\nJulia\u8a00\u8a9e\u3092\u7528\u3044\u305f\u885b\u661f\u89b3\u6e2c\u9ad8\u901f\u30b7\u30df\u30e5\u30ec\u30fc\u30bf\u306e\u958b\u767a -LiteBIRD\u3078\u306e\u5fdc\u7528-\n<\/td>\u9ad8\u702c\u7950\u4ecb<\/td><\/tr>
\n
\n\u7b2c22\u56de\u5b87\u5b99\u79d1\u5b66\u30b7\u30f3\u30dd\u30b8\u30a6\u30e0<\/a>\n<\/td>		1\u67086-7\u65e5\u3001\u30aa\u30f3\u30e9\u30a4\u30f3

<\/td>		\nCMB\u5168\u5929\u504f\u5149\u89b3\u6e2c\u306b\u304a\u3051\u308b\u30dd\u30a4\u30f3\u30c6\u30a3\u30f3\u30b0\u30a8\u30e9\u30fc\u306b\u7531\u6765\u3059\u308b\u7cfb\u7d71\u8aa4\u5dee\u306e\u6642\u7cfb\u5217\u30c7\u30fc\u30bf\u30b7\u30df\u30e5\u30ec\u30fc\u30b7\u30e7\u30f3\n<\/td>\u571f\u5c45\u76f4\u4e5f<\/td><\/tr>
\n
\n\u7b2c22\u56de\u5b87\u5b99\u79d1\u5b66\u30b7\u30f3\u30dd\u30b8\u30a6\u30e0<\/a>\n<\/td>		1\u67086-7\u65e5\u3001\u30aa\u30f3\u30e9\u30a4\u30f3

<\/td>		\n\u89e3\u6790\u7684\u624b\u6cd5\u3092\u7528\u3044\u305f\u5e83\u5929\u57df\u3067\u306eCMB\u504f\u5149\u89b3\u6e2c\u5b9f\u9a13\u306b\u304a\u3051\u308b\u7cfb\u7d71\u8aa4\u5dee\u306e\u7814\u7a76\n<\/td>\u77f3\u5742\u9ad8\u8f1d<\/td><\/tr>
\n
\n\u7b2c22\u56de\u5b87\u5b99\u79d1\u5b66\u30b7\u30f3\u30dd\u30b8\u30a6\u30e0<\/a>\n<\/td>		1\u67086-7\u65e5\u3001\u30aa\u30f3\u30e9\u30a4\u30f3

<\/td>		\nCMB\u5168\u5929\u504f\u5149\u89b3\u6e2c\u306b\u304a\u3051\u308b\u30a2\u30f3\u30c6\u30ca\u30d1\u30bf\u30fc\u30f3\u306e\u975e\u5bfe\u79f0\u6027\u7531\u6765\u306e\u7cfb\u7d71\u8aa4\u5dee\u306e\u898b\u7a4d\u3082\u308a\n<\/td>\u9577\u91ce\u4f51\u54c9<\/td><\/tr>
\n
\n\u7b2c22\u56de\u5b87\u5b99\u79d1\u5b66\u30b7\u30f3\u30dd\u30b8\u30a6\u30e0<\/a>\n<\/td>		1\u67086-7\u65e5\u3001\u30aa\u30f3\u30e9\u30a4\u30f3

<\/td>		\nLiteBIRD\u4f4e\u5468\u6ce2\u671b\u9060\u93e1\u7528\u504f\u5149\u5909\u8abf\u5668\u306e\u958b\u767a\u6982\u8981\n<\/td>\u685c\u4e95\u96c4\u57fa<\/td><\/tr><\/tbody><\/table><\/figure>\n\n\n\n

2021<\/font><\/a><\/h2>\n\n\n\n
\n
\n\u65b0\u5b66\u8853\u9818\u57df\u300c\u30cb\u30e5\u30fc\u30c8\u30ea\u30ce\u3067\u62d3\u304f\u7d20\u7c92\u5b50\u3068\u5b87\u5b99\u300d\u516c\u52df\u7814\u7a76\u30bb\u30df\u30ca\u30fc<\/a>\n<\/td>		11\u670816\u65e5\u3001\u30aa\u30f3\u30e9\u30a4\u30f3

<\/td>		\n\u8d85\u4f1d\u5c0e\u6280\u8853\u3068\u5fae\u7d30\u69cb\u9020\u5f62\u6210\u6280\u8853\u306e\u5408\u4f53\u306b\u3088\u308b\u65b0\u3057\u3044\u30cb\u30e5\u30fc\u30c8\u30ea\u30ce\u7269\u7406\u5b66\u306e\u5c55\u958b\n<\/td>\u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
\nMichigan State University, Astronomy Seminar series\n<\/td>14th of October, Online (Michigan, United States)

<\/td>		\nSimulations of systematic effects arising from cosmic rays in the LiteBIRD space telescope, and effects on the measurements of CMB B-modes\n<\/td>Samantha Lynn Stever<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u79d1\u30002021\u5e74\u79cb\u5b63\u5927\u4f1a\n<\/td>9\u670814\u65e5\u3001\u30aa\u30f3\u30e9\u30a4\u30f3

<\/td>		\n\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668\u3068\u5fae\u7d30\u69cb\u9020\u5f62\u6210\u6280\u8853\u3092\u7528\u3044\u305f\u30a4\u30f3\u30b8\u30a6\u30e0\u6a19\u7684\u96fb\u5b50\u30cb\u30e5\u30fc\u30c8\u30ea\u30ce\u691c\u51fa\u5668\u306e\u958b\u767a\n<\/td>\u98a8\u65e9\u548c\u4e5f<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u79d1\u30002021\u5e74\u79cb\u5b63\u5927\u4f1a\n<\/td>9\u670815\u65e5\u3001\u30aa\u30f3\u30e9\u30a4\u30f3

<\/td>		\n\u5927\u89d2\u5ea6\u30b9\u30b1\u30fc\u30eb\u3067\u306e\u539f\u59cb\u91cd\u529b\u6ce2\u63a2\u7d22\u306b\u898b\u8fbc\u307e\u308c\u308b\u975e\u5bfe\u79f0\u306a\u30cb\u30a2\u30b5\u30a4\u30c9\u30ed\u30fc\u30d6\u306e\u7cfb\u7d71\u8aa4\u5dee\u306e\u7814\u7a76\n<\/td>\u9577\u91ce\u4f51\u54c9<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u79d1\u30002021\u5e74\u79cb\u5b63\u5927\u4f1a\n<\/td>9\u670815\u65e5\u3001\u30aa\u30f3\u30e9\u30a4\u30f3

<\/td>		\nCMB\u5168\u5929\u504f\u5149\u89b3\u6e2c\u306b\u304a\u3051\u308b\u6307\u5411\u4f4d\u7f6e\u306e\u4e0d\u5b9a\u6027\u306b\u3088\u308b\u7cfb\u7d71\u8aa4\u5dee\u306e\u8a55\u4fa1\n<\/td>\u571f\u5c45\u76f4\u4e5f<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u79d1\u30002021\u5e74\u79cb\u5b63\u5927\u4f1a\n<\/td>9\u670815\u65e5\u3001\u30aa\u30f3\u30e9\u30a4\u30f3

<\/td>		\nCMB\u504f\u5149\u7cbe\u5bc6\u89b3\u6e2c\u885b\u661f\u306b\u304a\u3051\u308b\u5168\u5929\u89b3\u6e2c\u624b\u6cd5\u306e\u6700\u9069\u5316\n<\/td>\u9ad8\u702c\u7950\u4ecb<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u79d1\u30002021\u5e74\u79cb\u5b63\u5927\u4f1a\n<\/td>9\u670815\u65e5\u3001\u30aa\u30f3\u30e9\u30a4\u30f3

<\/td>		\n\u5e83\u5929\u57df\u3067\u306eCMB\u504f\u5149\u89b3\u6e2c\u5b9f\u9a13\u306b\u304a\u3051\u308b\u7cfb\u7d71\u8aa4\u5dee\u306e\u89e3\u6790\u7684\u7814\u7a76\n<\/td>\u77f3\u5742\u9ad8\u8f1d<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u79d1\u30002021\u5e74\u79cb\u5b63\u5927\u4f1a\n<\/td>9\u670815\u65e5\u3001\u30aa\u30f3\u30e9\u30a4\u30f3

<\/td>		\nSimulations of systematic effects arising from cosmic rays in the LiteBIRD space telescope, and effects on the measurements of CMB B-modes\n<\/td>Samantha Lynn Stever<\/td><\/tr>
\nJulia in Physics<\/a>\n<\/td>9\u67083\u65e5\u3001\u30aa\u30f3\u30e9\u30a4\u30f3

<\/td>		\n\u6b21\u4e16\u4ee3\u578bCMB\u89b3\u6e2c\u5b9f\u9a13\u306e\u305f\u3081\u306e\u5168\u5929\u30b9\u30ad\u30e3\u30f3\u30b7\u30df\u30e5\u30ec\u30fc\u30bf
\nFalcons.jl<\/a>\n<\/td>		\u9ad8\u702c\u7950\u4ecb<\/td><\/tr>
\n
\n19th International Workshop on Low Temperature Detectors
\n<\/a>\n<\/td>		29th of July, Online

<\/td>		\nDevelopment of an electron neutrino detector system using superconducting detectors and the surface microstructure forming technique\n<\/td>Hirokazu Ishino<\/td><\/tr>
\n
\n19th International Workshop on Low Temperature Detectors
\n<\/a>\n<\/td>		22th of July, Online

<\/td>		\nModelling signal oscillations arising from electrothermal coupling and stray capacitance in semiconducting bolometer impulse response\n<\/td>Samantha Lynn Stever<\/td><\/tr>
\n
\nEURAXESS, CMB-INFLATE
\n<\/a>\n<\/td>		8th of June, Online

<\/td>		\nObservation strategies and cosmological data\n<\/td>Hirokazu Ishino<\/td><\/tr>
\nPythagorean Astronomy\n<\/td>2nd of July, Online (Podcast Guest)

<\/td>		\nCosmic Developments\n<\/td>Samantha Lynn Stever<\/td><\/tr>
\nInstitut d\u2019Astrophysique Spatiale\n<\/td>26th of March, Online (Orsay, France)

<\/td>		\nSimulations of systematic effects arising from cosmic rays in the LiteBIRD space telescope, and effects on the measurements of CMB B-modes\n<\/td>Samantha Lynn Stever<\/td><\/tr>
\nCardiff University, Great Western Seminar Series\n<\/td>25th of March, Online (Cardiff University, UK)

<\/td>		\nSimulations of systematic effects arising from cosmic rays in the LiteBIRD space telescope, and effects on the measurements of CMB B-modes\n<\/td>Samantha Lynn Stever<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u79d1\u3000\u7b2c76\u56de\u5e74\u6b21\u5927\u4f1a\n<\/td>3\u670812\u65e5\u3001\u30aa\u30f3\u30e9\u30a4\u30f3

<\/td>		\nLiteBIRD\u306eCMB\u504f\u5149\u89b3\u6e2c\u306b\u304a\u3044\u3066\u5149\u5b66\u7cfb\u5185\u306e\u53cd\u5c04\u304c\u53ca\u307c\u3059\u7cfb\u7d71\u7684\u52b9\u679c\u306e\u7814\u7a76\n<\/td>\u9ad8\u702c\u7950\u4ecb<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u79d1\u3000\u7b2c76\u56de\u5e74\u6b21\u5927\u4f1a\n<\/td>3\u670812\u65e5\u3001\u30aa\u30f3\u30e9\u30a4\u30f3

<\/td>		\nLiteBIRD \u306b\u898b\u8fbc\u307e\u308c\u308b\u30b5\u30a4\u30c9\u30ed\u30fc\u30d6\u9818\u57df\u306e\u8f03\u6b63\u7cbe\u5ea6\u7531\u6765\u306e\u7cfb\u7d71\u8aa4\u5dee\u306b\u3064\u3044\u3066\u306e\u7814\u7a76\n<\/td>\u9577\u91ce\u4f51\u54c9<\/td><\/tr>
\n
\n\u5b87\u5b99\u79d1\u5b66\u30b7\u30f3\u30dd\u30b8\u30a6\u30e0<\/a>\n<\/td>		1\u67086-7\u65e5\u3001\u30aa\u30f3\u30e9\u30a4\u30f3

<\/td>		\n\u5927\u89d2\u5ea6\u30b9\u30b1\u30fc\u30eb\u306eCMB\u504f\u5149\u6e2c\u5b9a\u306b\u304a\u3044\u3066\u5149\u5b66\u7cfb\u5185\u306e\u53cd\u5c04\u304c\u53ca\u307c\u3059\u7cfb\u7d71\u7684\u52b9\u679c\u306e\u7814\u7a76 (\u30dd\u30b9\u30bf\u30fc)\n<\/td>\u9ad8\u702c\u7950\u4ecb<\/td><\/tr>
\n\u5b87\u5b99\u79d1\u5b66\u30b7\u30f3\u30dd\u30b8\u30a6\u30e0\n<\/td>1\u67086-7\u65e5\u3001\u30aa\u30f3\u30e9\u30a4\u30f3

<\/td>		\n\u5927\u89d2\u5ea6\u30b9\u30b1\u30fc\u30eb\u3067\u306eCMB\u6e2c\u5b9a\u306b\u304a\u3051\u308b\u30cb\u30a2\u30b5\u30a4\u30c9\u30ed\u30fc\u30d6\u306e\u7cfb\u7d71\u7684\u5f71\u97ff\u306e\u7814\u7a76 (\u30dd\u30b9\u30bf\u30fc)\n<\/td>\u9577\u91ce\u4f51\u54c9<\/td><\/tr>
\n\u5b87\u5b99\u79d1\u5b66\u30b7\u30f3\u30dd\u30b8\u30a6\u30e0\n<\/td>1\u67086-7\u65e5\u3001\u30aa\u30f3\u30e9\u30a4\u30f3

<\/td>		\n\u5b87\u5b99\u671b\u9060\u93e1LiteBIRD\u306b\u304a\u3051\u308b\u5b87\u5b99\u7dda\u306b\u8d77\u56e0\u3059\u308b\u7cfb\u7d71\u7684\u52b9\u679c\u306e\u30b7\u30df\u30e5\u30ec\u30fc\u30b7\u30e7\u30f3\u3068CMB B\u30e2\u30fc\u30c9\u306e\u6e2c\u5b9a\u3078\u306e\u5f71\u97ff(\u30dd\u30b9\u30bf\u30fc)\n<\/td>Samantha Lynn Stever<\/td><\/tr><\/tbody><\/table><\/figure>\n\n\n\n

2020<\/font><\/a><\/h2>\n\n\n\n
\n
\n\u65b0\u5b66\u8853\u9818\u57df\u300c\u30cb\u30e5\u30fc\u30c8\u30ea\u30ce\u3067\u62d3\u304f\u7d20\u7c92\u5b50\u3068\u5b87\u5b99\u300d\u7814\u7a76\u4f1a<\/a>\n<\/td>		12\u670821\uff0d22\u65e5\u3001\u30aa\u30f3\u30e9\u30a4\u30f3

<\/td>		\nNew Development of Neutrino Research Using Superconducting Technology (Poster)\n<\/td>Hirokazu Ishino<\/td><\/tr>
\n
\nCMB systematics and calibration focus workshop\n<\/a><\/td>		30th of Nov-3rd of Dec., Online

<\/td>		\nLiteBIRD systematics\n<\/td>Hirokazu Ishino<\/td><\/tr>
\nCMB systematics and calibration focus workshop<\/td>30th of Nov-3rd of Dec., Online

<\/td>		\nProgress towards a tool for evaluating the effect of common-mode cosmic ray systematic effects\n<\/td>Samantha Lynn Stever<\/td><\/tr>
\nCMB systematics and calibration focus workshop<\/td>30th of Nov-3rd of Dec., Online

<\/td>		\nStudy of systematic error due to reflection of half-wave plate at LiteBIRD\n<\/td>Yusuke Takase<\/td><\/tr>
\nCMB systematics and calibration focus workshop<\/td>30th of Nov-3rd of Dec., Online

<\/td>		\nStudy of the near side lobe systematic effects for large angular scale measurements\n<\/td>Yuya Nagano<\/td><\/tr>
\n
\n\u96fb\u5b50\u60c5\u5831\u901a\u4fe1\u5b66\u4f1a\u8d85\u4f1d\u5c0e\u30a8\u30ec\u30af\u30c8\u30ed\u30cb\u30af\u30b9\u7814\u7a76\u4f1a\uff08SCE\uff09
\n<\/a>\n<\/td>		11\u670825-26\u65e5
\u30aa\u30f3\u30e9\u30a4\u30f3
\u958b\u50ac

<\/td>		\n\u8d85\u4f1d\u5c0e\u6280\u8853\u3068\u30a4\u30f3\u30b8\u30a6\u30e0\u6a19\u7684\u3092\u7d44\u307f\u5408\u308f\u305b\u96fb\u5b50\u30cb\u30e5\u30fc\u30c8\u30ea\u30ce\u691c\u51fa\u3092\u76ee\u6307\u3059\u691c\u51fa\u5668\u958b\u767a
\n<\/td>		\u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
\nJapanese core-to-core meeting\n<\/td>September, Online (Japan)

<\/td>		\nMeasuring the polarised dust emission in the Galactic centre with the PILOT balloon-borne telescope\n<\/td>Samantha Lynn Stever<\/td><\/tr>
\n

\u65e5\u672c\u7269\u7406\u5b66\u4f1a2020\u5e74\u79cb\u5b63\u5927\u4f1a<\/a><\/p><\/td>

9\u670814\u65e5
\u30aa\u30f3\u30e9\u30a4\u30f3
\u958b\u50ac

<\/td>		\n Towards a complete study of potential cosmic ray systematic effects on the LiteBIRD space mission\n<\/td>Samantha Lynn Stever<\/td><\/tr>
\n \u65e5\u672c\u7269\u7406\u5b66\u4f1a2020\u5e74\u79cb\u5b63\u5927\u4f1a<\/td>9\u670814\u65e5
\u30aa\u30f3\u30e9\u30a4\u30f3
\u958b\u50ac

<\/td>		\nLiteBIRD\u4f4e\u5468\u6ce2\u671b\u9060\u93e1\u7528\u306e\u5e83\u5e2f\u57df\u591a\u5c64\u534a\u6ce2\u9577\u677f\u306e\u5c0f\u578b\u7248\u3067\u306e\u6975\u4f4e\u6e29\u30df\u30ea\u6ce2\u504f\u5149\u6027\u80fd\u8a55\u4fa1(2)\n<\/td>\u5c0f\u677e\u56fd\u5e79<\/td><\/tr>
\n \u65e5\u672c\u7269\u7406\u5b66\u4f1a2020\u5e74\u79cb\u5b63\u5927\u4f1a<\/td>9\u670814\u65e5
\u30aa\u30f3\u30e9\u30a4\u30f3
\u958b\u50ac

<\/td>		\n \u30a4\u30f3\u30b8\u30a6\u30e0\u3068\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668\u3092\u7d44\u307f\u5408\u308f\u305b\u305f\u96fb\u5b50\u30cb\u30e5\u30fc\u30c8\u30ea\u30ce\u691c\u51fa\u5668\u306e\u958b\u767a\n<\/td>\u4e2d\u5c3e\u53cb\u54c9<\/td><\/tr>
\n \u65e5\u672c\u7269\u7406\u5b66\u4f1a2020\u5e74\u79cb\u5b63\u5927\u4f1a<\/td>9\u670814\u65e5
\u30aa\u30f3\u30e9\u30a4\u30f3
\u958b\u50ac

<\/td>		\n LiteBIRD\u306b\u304a\u3051\u308b\u534a\u6ce2\u9577\u677f\u306e\u53cd\u5c04\u306b\u3088\u308b\u7cfb\u7d71\u8aa4\u5dee\u306e\u7814\u7a76\n<\/td>\u9ad9\u702c\u7950\u4ecb<\/td><\/tr>
\n \u65e5\u672c\u7269\u7406\u5b66\u4f1a2020\u5e74\u79cb\u5b63\u5927\u4f1a<\/td>9\u670814\u65e5
\u30aa\u30f3\u30e9\u30a4\u30f3
\u958b\u50ac

<\/td>		\nLiteBIRD\u306b\u642d\u8f09\u3059\u308b\u5149\u5b66\u90e8\u6750\u306b\u8d77\u56e0\u3059\u308b\u7cfb\u7d71\u8aa4\u5dee\u306e\u7814\u7a76\n<\/td>\u9577\u91ce\u4f51\u54c9<\/td><\/tr>
\n \u5fdc\u7528\u7269\u7406\u30fb\u7269\u7406\u7cfb\u5b66\u4f1a\u4e2d\u56fd\u56db\u56fd\u652f\u90e8\u5408\u540c\u5b66\u8853\u8b1b\u6f14\u4f1a<\/td>8\u67082\u65e5
\u9ce5\u53d6\u5927\u5b66\u62c5\u5f53
\uff08\u30aa\u30f3\u30e9\u30a4\u30f3\u958b\u50ac\uff09<\/td>		\n CMB\u89b3\u6e2c\u306e\u305f\u3081\u306bLiteBIRD\u885b\u661f\u304c\u642d\u8f09\u3059\u308b\u5149\u5b66\u90e8\u6750\u306e\u6027\u80fd\u8a55\u4fa1\u88c5\u7f6e\u306e\u958b\u767a\u3068\u305d\u306e\u5fdc\u7528\n<\/td>\u9ad9\u702c\u7950\u4ecb<\/td><\/tr>
\n \u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c75\u56de\u5e74\u6b21\u5927\u4f1a<\/a><\/td>		3\u670817\u65e5
\u540d\u53e4\u5c4b\u5927\u5b66
\uff08WEB\u63b2\u8f09\uff09<\/td>		\n LiteBIRD\u4f4e\u5468\u6ce2\u671b\u9060\u93e1\u7528\u306e\u5e83\u5e2f\u57df\u591a\u5c64\u534a\u6ce2\u9577\u677f\u306e\u5c0f\u578b\u7248\u3067\u306e\u4f4e\u6e29\u30df\u30ea\u6ce2\u504f\u5149\u6027\u80fd\u8a55\u4fa1\n<\/td>\u5c0f\u677e\u56fd\u5e79<\/td><\/tr>
\n\u8d85\u4f1d\u5c0e\u30a8\u30ec\u30af\u30c8\u30ed\u30cb\u30af\u30b9\u7814\u7a76\u4f1a
\n<\/td>		1\u670817\u65e5
\u6a2a\u6d5c\u5e02
\u958b\u6e2f\u8a18\u5ff5\u4f1a\u9928<\/td>		\nNew development of neutrino research using superconducting technology\n<\/td>Yuya Nakao
(poster)<\/td><\/tr><\/tbody><\/table><\/figure>\n\n\n\n

2019<\/font><\/a><\/h2>\n\n\n\n
\nB-mode from Space
\n<\/td>		December 17
Max-Planck-Institut f\u00fcr Astrophysik<\/td>		\nDemonstration of mm-wave performance of small prototype LiteBIRD LFT AHWP at around 20K<\/a><\/td>Kunimoto Komatsu<\/td><\/tr>
\n\u91cf\u5b50\u30a8\u30ec\u30af\u30c8\u30ed\u30cb\u30af\u30b9\u7814\u7a76\u4f1a<\/a><\/td>11\u67088\u65e5
\u6771\u4eac\u5927\u5b66
\u5c71\u4e2d\u5bee
\u5185\u85e4\u30bb\u30df\u30ca\u30fc\u30cf\u30a6\u30b9<\/td>		\nCMB\u504f\u5149\u89b3\u6e2c\u885b\u661fLiteBIRD\u3068\u8d85\u4f1d\u5c0e\u6280\u8853\n<\/td>\u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
\nFundamental Physics with Future CMB probes
\n<\/td>		30th of Oct
SISSA<\/td>		\nLiteBIRD and development of superconducting detectors\n<\/td>Hirokazu Ishino<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a

\n2019\u5e74\u79cb\u5b63\u5927\u4f1a<\/a><\/td>		9\u670817-20\u65e5
\u5c71\u5f62\u5927\u5b66<\/td>		\n\u30cb\u30e5\u30fc\u30c8\u30ea\u30ce\u306e\u7814\u7a76\u3092\u76ee\u6307\u3057\u305f\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668\u306e\u958b\u767a\n<\/td>\u4e2d\u5c3e\u53cb\u54c9<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
2019\u5e74\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670817-20\u65e5
\u5c71\u5f62\u5927\u5b66<\/td>		\n\u30a6\u30a3\u30f3\u30b9\u30c8\u30f3\u30b3\u30fc\u30f3\u69cb\u9020\u3092\u7528\u3044\u305f\u30d5\u30a9\u30ce\u30f3\u306e\u691c\u51fa\u306e\u7814\u7a76\n<\/td>\u67f3\u6fa4\u96c5\u4eba<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
2019\u5e74\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670817-20\u65e5
\u5c71\u5f62\u5927\u5b66<\/td>		\n\u30cb\u30e5\u30fc\u30c8\u30ea\u30ce\u7269\u7406\u7814\u7a76\u3092\u76ee\u6307\u3057\u305f\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668\u3068\u30cb\u30e5\u30fc\u30c8\u30ea\u30ce\u6a19\u7684\u306e\u958b\u767a\u306e\u6982\u8981\n<\/td>\u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
2019\u5e74\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670817-20\u65e5
\u5c71\u5f62\u5927\u5b66<\/td>		\nLiteBIRD\u885b\u661f\u306b\u304a\u3051\u308b\u5229\u5f97\u306e\u6642\u9593\u5909\u5316\u306b\u3088\u308b\u7cfb\u7d71\u8aa4\u5dee\u306e\u8a55\u4fa1\n<\/td>\u4e2d\u5d8b\u5927\u6a39<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
2019\u5e74\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670817-20\u65e5
\u5c71\u5f62\u5927\u5b66<\/td>		\nLiteBIRD\u885b\u661f\u3067\u5229\u7528\u3059\u308b\u591a\u5c64\u504f\u5149\u5909\u8abf\u677f\u306e\u63a5\u7740\u3068\u305d\u306e\u632f\u52d5\u8010\u6027\u306e\u7814\u7a76\n<\/td>\u6238\u7530\u8cb4\u4e4b<\/td><\/tr>
\nExploration of Particle Physics and Cosmology with Neutrinos Workshop2019<\/a><\/td>June\u300012-14
\u30d2\u30eb\u30db\u30c6\u30eb
\u30b5\u30f3\u30d4\u30a2\u4f0a\u8cc0
<\/td>		\nDevelopment of New Superconducting Detectors for Neutrino Researches\n<\/td>M.Yanagisawa Y.Nakao (poster)<\/td><\/tr>
\nTPC\u5ea7\u8ac7\u4f1a
\n<\/td>		3\u670822\u65e5
\u795e\u6238\u5927\u5b66<\/td>		\n\u6db2\u4f53\u30d8\u30ea\u30a6\u30e0\u3092\u7528\u3044\u305f\u6697\u9ed2\u7269\u8cea\u306e\u63a2\u7d22\n<\/td>\u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a

\n\u7b2c74\u56de\u5e74\u6b21\u5927\u4f1a<\/td>		3\u670814-17\u65e5
\u4e5d\u5dde\u5927\u5b66<\/td>		\n\u30a2\u30eb\u30df\u30ca\u306b\u5bfe\u3059\u308b\u30e2\u30b9\u30a2\u30a4\u52a0\u5de5\u3092\u7528\u3044\u305f\u30df\u30ea\u6ce2\u5e2f\u57df\u306b\u304a\u3051\u308b\u53cd\u5c04\u9632\u6b62\u69cb\u9020\u306e\u958b\u767a\n<\/td>\u67f3\u6fa4\u96c5\u4eba<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a

\n\u7b2c74\u56de\u5e74\u6b21\u5927\u4f1a<\/td>		3\u670814-17\u65e5
\u4e5d\u5dde\u5927\u5b66<\/td>		\nLiteBIRD\u504f\u5149\u5909\u8abf\u5668\u306e\u5c0f\u578b\u5e83\u5e2f\u57df\u591a\u5c64\u534a\u6ce2\u9577\u306e\u4f4e\u6e29\u30df\u30ea\u6ce2\u504f\u5149\u6027\u80fd\u8a55\u4fa1\n<\/td>\u5c0f\u677e\u56fd\u5e79<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\n\u7b2c74\u56de\u5e74\u6b21\u5927\u4f1a
\n\n<\/a><\/td>		3\u670814-17\u65e5
\u4e5d\u5dde\u5927\u5b66<\/td>		\n\u30df\u30ea\u6ce2\u306e\u5782\u76f4\u5165\u5c04\u306b\u5bfe\u3059\u308b\u53cd\u5c04\u7387\u6e2c\u5b9a\n<\/td>\u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
\n\u65e5\u672c\u5b66\u8853\u4f1a\u8b70
\u516c\u958b\u30b7\u30f3\u30dd\u30b8\u30a6\u30e0
<\/a><\/td>		2\u670819\u65e5
\u65e5\u672c\u5b66\u8853\u4f1a\u8b70
\u8b1b\u5802
<\/td>		\nCMB\u306e\u30ec\u30d3\u30e5\u30fc\n<\/td>\u77f3\u91ce\u5b8f\u548c<\/td><\/tr><\/tbody><\/table><\/figure>\n\n\n\n

2018<\/font><\/a><\/h2>\n\n\n\n
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\n \u79cb\u5b63\u5927\u4f1a<\/a><\/td>		9\u670814-17\u65e5
\u4fe1\u5dde\u5927\u5b66<\/td>		\nCMB\u89b3\u6e2c\u5e2f\u57df\u3067\u306e\u30df\u30ea\u6ce2\u306e\u53cd\u5c04\u7387\u6e2c\u5b9a\u7cfb\u306e\u69cb\u7bc9\n<\/td>\u7247\u5ca1\u96c4\u4e00\u90ce<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\n\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670814-17\u65e5
\u4fe1\u5dde\u5927\u5b66<\/td>		\nLiteBIRD\u504f\u5149\u5909\u8abf\u5668\u306e\u6975\u4f4e\u6e29\u3067\u4f5c\u52d5\u3059\u308b\u56de\u8ee2\u6a5f\u69cb\u306e\u5b9f\u73fe\u6027\u5b9f\u8a3c\u306b\u5411\u3051\u305f\u5c0f\u578b\u8a66\u4f5c\u6a5f\u306e\u6027\u80fd\u8a55\u4fa1\n<\/td>\u5c0f\u677e\u56fd\u5e79<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\n\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670814-17\u65e5
\u4fe1\u5dde\u5927\u5b66<\/td>		\n\u5b87\u5b99\u30de\u30a4\u30af\u30ed\u6ce2\u80cc\u666f\u653e\u5c04\u306e\u89b3\u6e2c\u3067\u7528\u3044\u308b\u53cd\u5c04\u9632\u6b62\u69cb\u9020\u306e\u958b\u767a\n<\/td> \u67f3\u6fa4\u96c5\u4eba<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\n\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670814-17\u65e5
\u4fe1\u5dde\u5927\u5b66<\/td>		\n\u6db2\u4f53\u30d8\u30ea\u30a6\u30e0\u3092\u7528\u3044\u305f\u8efd\u3044\u6697\u9ed2\u7269\u8cea\u63a2\u7d22\u7528\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668(LEKID)\u306e\u958b\u767a(7)\n<\/td>\u559c\u7530\u6d0b\u4ecb<\/td><\/tr>
\n\u5fdc\u7528\u7269\u7406\u30fb\u7269\u7406\u7cfb\u5b66\u4f1a
\n\u4e2d\u56fd\u56db\u56fd\u652f\u90e8 \u5408\u540c\u5b66\u8853\u8b1b\u6f14\u4f1a<\/td>		8\u67084\u65e5
\u5e83\u5cf6\u5927\u5b66<\/td>		\nLiteBIRD:\u79d1\u5b66\u885b\u661f\u3092\u7528\u3044\u305f\u5b87\u5b99\u30de\u30a4\u30af\u30ed\u6ce2\u80cc\u666f\u653e\u5c04\u504f\u5149\u7cbe\u5bc6\u6e2c\u5b9a\u5b9f\u9a13\n<\/td>\u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
\nSPIE
\n
\nSPIE Astronomical Telescopes + Instrumentation<\/a><\/td>		June 10-15
Austin, Texas<\/td>		\nPrototype design and evaluation of the nine-layer achromatic half-wave plate for the LiteBIRD low frequency telescope\n<\/td>K. Komatsu<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\n\u7b2c73\u56de\u5e74\u6b21\u5927\u4f1a<\/a><\/td>		3\u670822-25\u65e5
\u6771\u4eac\u7406\u79d1\u5927\u5b66<\/td>		\nLiteBIRD\u3067\u4f7f\u7528\u3059\u308b\u5149\u5b66\u90e8\u6750\u306e\u967d\u5b50\u7dda\u306b\u3088\u308b\u5f71\u97ff(6)\n<\/td>\u7247\u5ca1\u96c4\u4e00\u90ce<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\n\u7b2c73\u56de\u5e74\u6b21\u5927\u4f1a<\/td>		3\u670822-25\u65e5
\u6771\u4eac\u7406\u79d1\u5927\u5b66<\/td>		\n\u6db2\u4f53\u30d8\u30ea\u30a6\u30e0\u3092\u7528\u3044\u305f\u8efd\u3044\u6697\u9ed2\u7269\u8cea\u63a2\u7d22\u7528\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668(LEKID)\u306e\u958b\u767a(6)\n<\/td>\u559c\u7530\u6d0b\u4ecb<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\n\u7b2c73\u56de\u5e74\u6b21\u5927\u4f1a<\/td>		3\u670822-25\u65e5
\u6771\u4eac\u7406\u79d1\u5927\u5b66<\/td>		\n\u6db2\u4f53\u30d8\u30ea\u30a6\u30e0\u3092\u7528\u3044\u305f\u8efd\u3044\u6697\u9ed2\u7269\u8cea\u63a2\u7d22\u7528\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668(LEKID)\u306e\u6027\u80fd\u8a55\u4fa1(3)\n<\/td>\u79c0\u5e73\u76f4\u4eba<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\n\u7b2c73\u56de\u5e74\u6b21\u5927\u4f1a<\/td>		3\u670822-25\u65e5
\u6771\u4eac\u7406\u79d1\u5927\u5b66<\/td>		\nLiteBIRD \u306e\u504f\u5149\u5909\u8abf\u5668\u306b\u7528\u3044\u308b\u5e83\u5e2f\u57df\u591a\u5c64\u534a\u6ce2\u9577\u677f\u306e\u958b\u767a(2)\n<\/td>\u5c0f\u677e\u56fd\u5e79<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\n\u7b2c73\u56de\u5e74\u6b21\u5927\u4f1a<\/td>		3\u670822-25\u65e5
\u6771\u4eac\u7406\u79d1\u5927\u5b66<\/td>		\nLiteBIRD\u306e\u7cfb\u7d71\u8aa4\u5dee\u306e\u7814\u7a76\n<\/td>\u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\n\u7b2c73\u56de\u5e74\u6b21\u5927\u4f1a<\/td>		3\u670822-25\u65e5
\u6771\u4eac\u7406\u79d1\u5927\u5b66<\/td>		\n\u6db2\u4f53\u30d8\u30ea\u30a6\u30e0\u3092\u7528\u3044\u305f\u6697\u9ed2\u7269\u8cea\u63a2\u7d22\n<\/td>\u77f3\u91ce\u5b8f\u548c<\/td><\/tr><\/tbody><\/table><\/figure>\n\n\n\n

2017<\/font><\/a><\/h2>\n\n\n\n
\nISS2017<\/a><\/td>Dec. 13-15
Tokyo, Japan<\/td>		\nStudy on Lumped Element Kinetic Inductance Detectors for Light Dark Matter Searches Using Liquid Helium\n<\/td>Yosuke Kida
(poster)<\/td><\/tr>
\nB-MODE FROM SPACE WORKSHOP<\/a><\/td>Dec. 4-6
UC Berkeley<\/td>		\nLiteBIRD systematics study\n<\/td>Hirokazu Ishino<\/td><\/tr>
\nB-MODE FROM SPACE WORKSHOP<\/td>Dec. 4-6
UC Berkeley<\/td>		\nDevelopment of Pancharatnam achromatic half-wave plate
\nfor polarization modulator of LiteBIRD\n<\/td>		Kunimoto Komatsu
(poster)<\/td><\/tr>
\n\u8d85\u4f1d\u5c0e\u30a8\u30ec\u30af\u30c8\u30ed\u30cb\u30af\u30b9\u7814\u7a76\u4f1a<\/a><\/td>10\u67084-5\u65e5
\u6771\u5317\u5927\u5b66<\/td>		\n\u6db2\u4f53\u30d8\u30ea\u30a6\u30e0\u3092\u7528\u3044\u305f\u8efd\u3044\u6697\u9ed2\u7269\u8cea\u63a2\u7d22\u7528\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668(LEKID)\u306e\u958b\u767a(3)\n<\/td>\u559c\u7530\u6d0b\u4ecb<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\n\u79cb\u5b63\u5927\u4f1a<\/a><\/td>		9\u670812-15\u65e5
\u5b87\u90fd\u5bae\u5927\u5b66<\/td>		\nLiteBIRD\u306e\u504f\u5149\u5909\u8abf\u5668\u306b\u7528\u3044\u308b\u5e83\u5e2f\u57df\u591a\u5c64\u534a\u6ce2\u9577\u677f\u306e\u958b\u767a\n<\/td>\u5c0f\u677e\u56fd\u5e79<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\n\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670812-15\u65e5
\u5b87\u90fd\u5bae\u5927\u5b66<\/td>		\nLiteBIRD\u3067\u4f7f\u7528\u3059\u308b\u5149\u5b66\u90e8\u6750\u306e\u967d\u5b50\u7dda\u306b\u3088\u308b\u5f71\u97ff(5)\n<\/td>\u7247\u5ca1\u96c4\u4e00\u90ce<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\n\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670812-15\u65e5
\u5b87\u90fd\u5bae\u5927\u5b66<\/td>		\nLiteBIRD\u306b\u304a\u3051\u308b\u7cfb\u7d71\u8aa4\u5dee\u3068\u30b9\u30ad\u30e3\u30f3\u65b9\u6cd5\u306e\u95a2\u9023\u6027\u306e\u7814\u7a76\n<\/td>\u9b5a\u4f4f\u8056<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\n\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670812-15\u65e5
\u5b87\u90fd\u5bae\u5927\u5b66<\/td>		\n\u6db2\u4f53\u30d8\u30ea\u30a6\u30e0\u3092\u7528\u3044\u305f\u8efd\u3044\u6697\u9ed2\u7269\u8cea\u63a2\u7d22\u7528\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668(LEKID)\u306e\u958b\u767a(5)\n<\/td>\u559c\u7530\u6d0b\u4ecb<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\n\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670812-15\u65e5
\u5b87\u90fd\u5bae\u5927\u5b66<\/td>		\n\u6db2\u4f53\u30d8\u30ea\u30a6\u30e0\u3092\u7528\u3044\u305f\u8efd\u3044\u6697\u9ed2\u7269\u8cea\u63a2\u7d22\u7528\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668(LEKID)\u306e\u6027\u80fd\u8a55\u4fa1(2)\n<\/td>\u79c0\u5e73\u76f4\u4eba<\/td><\/tr>
\nLTD17<\/a><\/td>July 17-21
Kurume, Japan <\/td>		\nDevelopment of Lumped Element Kinetic Inductance Detectors for Light Dark Matter Searches using Liquid Helium (poster)\n<\/td> Yosuke Kida <\/td><\/tr>
\n\u7b2c8\u56deSOIPIX\u7814\u7a76\u4f1a<\/td>6\u670824-25\u65e5
\u5bae\u5d0e\u5927\u5b66, \u6728\u82b1\u30ad\u30e3\u30f3\u30d1\u30b9 <\/td>		\n\u6975\u4f4e\u6e29SOI\u53ef\u8996\u5149\u30bb\u30f3\u30b5\u30fc\u3068CMB\u89b3\u6e2c\u7528\u5149\u5b66\u7cfb\u8a55\u4fa1\u3078\u306e\u5fdc\u7528\n<\/td> \u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
\nCRC\u30bf\u30a6\u30f3\u30df\u30fc\u30c6\u30a3\u30f3\u30b0<\/a><\/td>6\u670824-25\u65e5
\u6771\u4eac\u5927\u5b66, \u67cf\u30ad\u30e3\u30f3\u30d1\u30b9 <\/td>		\n\u5ca1\u5c71\u30d8\u30ea\u30a6\u30e0\n<\/td> \u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
\n\u5929\u6587\u5b66\u306b\u304a\u3051\u308b\u30c7\u30fc\u30bf\u79d1\u5b66\u7684\u65b9\u6cd5<\/a><\/td>5\u670829-31\u65e5
\u7d71\u8a08\u6570\u7406\u7814\u7a76\u6240, \u7acb\u5ddd <\/td>		\n\uff23\uff2d\uff22\u30fb\u89e3\u6790\u30d1\u30a4\u30d7\u30e9\u30a4\u30f3\u30fb\u7cfb\u7d71\u8aa4\u5dee\n<\/td> \u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
\n\u30a2\u30af\u30c6\u30a3\u30d6\u5a92\u8ceaTPC\u958b\u767a\u5ea7\u8ac7\u4f1a<\/a><\/td>4\u670822\u65e5
KEK, \u3064\u304f\u3070<\/td>		\n\u8efd\u3044DM\u63a2\u7d22\u306e\u305f\u3081\u306e\u6db2\u30d8\u30ea\u30a6\u30e0TPC\n<\/td> \u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
\n\u653e\u533b\u7814\u6210\u679c\u5831\u544a\u4f1a<\/td>4\u670818\u65e5
HIMAC, \u5343\u8449<\/td>		\n\u967d\u5b50\u30d3\u30fc\u30e0\u7167\u5c04\u8a66\u9a13\u7d50\u679c\u5831\u544a\n<\/td> \u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
\nOPIC 2017<\/a><\/td>April 18-21
Pacifico, Yokohama<\/td>		\nLiteBIRD\n<\/td> Satoru Uozumi<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c72\u56de\u5e74\u6b21\u5927\u4f1a<\/a><\/td>		3\u670817-20\u65e5
\u5927\u962a\u5927\u5b66
\u8c4a\u4e2d<\/td>		\n\u6db2\u4f53\u30d8\u30ea\u30a6\u30e0\u3092\u7528\u3044\u305f\u8efd\u3044\u6697\u9ed2\u7269\u8cea\u63a2\u7d22\u7528\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668(LEKID)\u306e\u958b\u767a(4)\n<\/td>\u559c\u7530\u6d0b\u4ecb<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c72\u56de\u5e74\u6b21\u5927\u4f1a<\/td>		3\u670817-20\u65e5
\u5927\u962a\u5927\u5b66
\u8c4a\u4e2d<\/td>		\n\u6db2\u4f53\u30d8\u30ea\u30a6\u30e0\u3092\u7528\u3044\u305f\u8efd\u3044\u6697\u9ed2\u7269\u8cea\u63a2\u7d22\u7528\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668LEKID\u306e\u6027\u80fd\u8a55\u4fa1\n<\/td>\u79c0\u5e73\u76f4\u4eba<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c72\u56de\u5e74\u6b21\u5927\u4f1a<\/td>		3\u670817-20\u65e5
\u5927\u962a\u5927\u5b66
\u8c4a\u4e2d<\/td>		\nLiteBIRD\u3067\u4f7f\u7528\u3059\u308b\u5149\u5b66\u90e8\u6750\u306e\u967d\u5b50\u7dda\u306b\u3088\u308b\u5f71\u97ff(4)\n<\/td>\u5c0f\u677e\u56fd\u5e79<\/td><\/tr>
\nWhy does the Universe accelerate?<\/td>March 8-10
KEK, Tsukuba<\/td>		\nLiteBIRD\n<\/td> Hirokazu Ishino<\/td><\/tr>
\n Cosmic Polarimetry from Micro to Macro Scales <\/a><\/td>Feb. 17-18
Hiroshima University<\/td>		\nLiteBIRD: Lite satellite for the study of B-mode polarization and Inflation from cosmic microwave background radiation detection\n<\/td> Hirokazu Ishino<\/td><\/tr>
\nB-Modes rfom Space Workshop 2017<\/a><\/td>Jan. 23-25
Montreal, Canada<\/td>		\nScan Strategy\n<\/td> Satoru Uozumi <\/td><\/tr>
\nB-Modes rfom Space Workshop 2017<\/td>Jan. 23-25
Montreal, Canada<\/td>		\nSystematics Summary\n<\/td> Hirokazu Ishino <\/td><\/tr>
\nB-Modes rfom Space Workshop 2017
(poster)<\/td>		Jan. 23-25
Montreal, Canada<\/td>		\nIrradiation tests of the LiteBIRD optical components using a 160 MeV proton beam at HIMAC (2)\n<\/td>Kunimoto Komatsu<\/td><\/tr><\/tbody><\/table><\/figure>\n\n\n\n

2016<\/font><\/a><\/h2>\n\n\n\n
\nISS2016<\/a>
(poster)<\/td>		Dec. 13-15
Tokyo, Japan<\/td>		\nDevelopment of LEKID detectors for Light Dark Matter Searches using Liquid Helium\n<\/td>Yosuke Kida<\/td><\/tr>
\nISS2016<\/td>Dec. 13-15
Tokyo, Japan<\/td>		\nDevelopment of Superconducting Detectors for Dark Matter Searches using Liquid Helium\n<\/td>Hirokazu Ishino<\/td><\/tr>
\n\u7b2c\uff17\u56deSOI\u65b0\u5b66\u8853\u9818\u57df\u7814\u7a76\u4f1a<\/td>11\u670821-22\u65e5
Spring-8\u5175\u5eab<\/td>		\n\u6975\u4f4e\u6e29\u53ef\u8996\u5149\u30bb\u30f3\u30b5\u30fc\u306e\u958b\u767a\n<\/td>\u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
\nIWSSD2016<\/td>Nov. 11-14
AIST, Tsukuba<\/td>		\nDevelopment of Kinetic Inductance Detectors to search for dark matter\n<\/td>Hirokazu Ishino<\/td><\/tr>
\n\u8d85\u4f1d\u5c0e\u30a8\u30ec\u30af\u30c8\u30ed\u30cb\u30af\u30b9\u7814\u7a76\u4f1a\uff08SCE\uff09\n<\/td>10\u670826-27\u65e5
\u6771\u5317\u5927\u5b66\u96fb\u6c17\u901a\u4fe1\u7814\u7a76\u6240 <\/td>		\n\u6db2\u4f53\u30d8\u30ea\u30a6\u30e0\u3092\u7528\u3044\u305f\u8efd\u3044\u6697\u9ed2\u7269\u8cea\u63a2\u7d22\u7528\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668(LEKID)\u306e\u958b\u767a(2)\n<\/td>\u559c\u7530\u6d0b\u4ecb<\/td><\/tr>
\n\u8d85\u4f1d\u5c0e\u30a8\u30ec\u30af\u30c8\u30ed\u30cb\u30af\u30b9\u7814\u7a76\u4f1a\uff08SCE\uff09\n<\/td>10\u670826-27\u65e5
\u6771\u5317\u5927\u5b66\u96fb\u6c17\u901a\u4fe1\u7814\u7a76\u6240 <\/td>		\n\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668KID\u7528\u9ad8\u901f\u591a\u91cd\u540c\u6642\u8aad\u307f\u51fa\u3057\u30b7\u30b9\u30c6\u30e0\n<\/td>\u5c71\u7530\u8981\u4ecb<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\n\u79cb\u5b63\u5927\u4f1a<\/a><\/td>		9\u670821-24\u65e5
\u5bae\u5d0e\u5927\u5b66<\/td>		\n\u6db2\u4f53\u30d8\u30ea\u30a6\u30e0\u3092\u7528\u3044\u305f\u8efd\u3044\u6697\u9ed2\u7269\u8cea\u63a2\u7d22\u7528\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668(LEKID)\u306e\u958b\u767a(3)\n<\/td>\u559c\u7530\u6d0b\u4ecb<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a\u3000
\n\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670821-24\u65e5
\u5bae\u5d0e\u5927\u5b66<\/td>		\n\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668KID\u7528\u30d1\u30eb\u30b9\u591a\u91cd\u540c\u6642\u8aad\u307f\u51fa\u3057DAQ\u30b7\u30b9\u30c6\u30e0\u306e\u958b\u767a\n<\/td>\u5c71\u7530\u8981\u4ecb<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a\u3000
\n\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670821-24\u65e5
\u5bae\u5d0e\u5927\u5b66<\/td>		\nSOI\u6280\u8853\u3092\u7528\u3044\u305f\u6975\u4f4e\u6e29\u53ef\u8996\u5149\u30bb\u30f3\u30b5\u30fc\u306e\u958b\u767a1\n<\/td>\u6a39\u6797\u6566\u5b50<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a\u3000
\n\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670821-24\u65e5
\u5bae\u5d0e\u5927\u5b66<\/td>		\nLiteBIRD\u8a08\u753b\u306b\u304a\u3051\u308b\u7cfb\u7d71\u8aa4\u5dee\u306e\u7814\u7a76\n<\/td>\u9b5a\u4f4f\u8056<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a\u3000
\n\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670821-24\u65e5
\u5bae\u5d0e\u5927\u5b66<\/td>		\nLiteBIRD\u3067\u4f7f\u7528\u3059\u308b\u5149\u5b66\u90e8\u6750\u306e\u967d\u5b50\u7dda\u306b\u3088\u308b\u5f71\u97ff\uff083\uff09\n<\/td>\u5c0f\u677e\u56fd\u5e79<\/td><\/tr>
\n\u4e2d\u56db\u56fd\u5408\u540c\u5b66\u8853\u8b1b\u6f14\u4f1a<\/td>7\u670831\u65e5
\u5ca1\u5c71\u5927\u5b66<\/td>		\n\u79d1\u5b66\u885b\u661fLiteBIRD\u3067\u63a2\u308b\u539f\u59cb\u91cd\u529b\u6ce2\n<\/td>\u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
\nSOI\u65b0\u5b66\u8853\u9818\u57df
\u7b2c6\u56de\u7814\u7a76\u4f1a<\/td>		6\u670828-29\u65e5
\u5317\u6d77\u9053\u5927\u5b66 <\/td>		\nSOI\u6280\u8853\u3092\u7528\u3044\u305f\u6975\u4f4e\u6e29\u53ef\u8996\u5149\u30bb\u30f3\u30b5\u30fc\u306e\u958b\u767a\n<\/td>\u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
\nSPIE<\/a><\/td>June 26 – July 1
Edinburgh, Scotland<\/td>		\nLiteBIRD: lite satellite for the study of B-mode polarization and inflation from cosmic microwave background radiation detection\n<\/td>Hirokazu Ishino<\/td><\/tr>
\n\u9ad8\u5b87\u9023\u3000
\u7b2c15\u56de\u7814\u7a76\u4f1a<\/td>		3\u670823-25\u65e5
\u6771\u4eac\u7406\u79d1\u5927\u5b66<\/td>		\n\u5b87\u5b99\u30de\u30a4\u30af\u30ed\u6ce2\u504f\u5149\uff1aLiteBIRD\n<\/td>\u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c71\u56de\u5e74\u6b21\u5927\u4f1a<\/a><\/td>		3\u670819-22\u65e5
\u6771\u5317\u5b66\u9662\u5927\u5b66\u3000\u6cc9\u30ad\u30e3\u30f3\u30d1\u30b9
\u4ed9\u53f0<\/td>		\nLiteBIRD\u306b\u304a\u3051\u308b\u30b7\u30df\u30e5\u30ec\u30fc\u30b7\u30e7\u30f3\u3092\u7528\u3044\u305f\u7cfb\u7d71\u8aa4\u5dee\u306e\u8a55\u4fa1\n<\/td>\u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c71\u56de\u5e74\u6b21\u5927\u4f1a<\/td>		3\u670819-22\u65e5
\u6771\u5317\u5b66\u9662\u5927\u5b66\u3000\u6cc9\u30ad\u30e3\u30f3\u30d1\u30b9
\u4ed9\u53f0<\/td>		\nLiteBIRD\u3067\u4f7f\u7528\u3059\u308b\u5149\u5b66\u90e8\u6750\u306e\u967d\u5b50\u7dda\u306b\u3088\u308b\u5f71\u97ff\uff082\uff09\n<\/td>\u5c0f\u677e\u56fd\u5e79<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c71\u56de\u5e74\u6b21\u5927\u4f1a<\/td>		3\u670819-22\u65e5
\u6771\u5317\u5b66\u9662\u5927\u5b66\u3000\u6cc9\u30ad\u30e3\u30f3\u30d1\u30b9
\u4ed9\u53f0<\/td>		\n\u6db2\u4f53\u30d8\u30ea\u30a6\u30e0\u3092\u7528\u3044\u305f\u8efd\u3044\u6697\u9ed2\u7269\u8cea\u63a2\u7d22\u7528\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668(LEKID)\u306e\u958b\u767a(2)\n<\/td>\u559c\u7530\u6d0b\u4ecb<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c71\u56de\u5e74\u6b21\u5927\u4f1a<\/td>		3\u670819-22\u65e5
\u6771\u5317\u5b66\u9662\u5927\u5b66
\u6cc9\u30ad\u30e3\u30f3\u30d1\u30b9
\u4ed9\u53f0<\/td>		\n\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668KID\u7528\u591a\u91cd\u540c\u6642\u8aad\u307f\u51fa\u3057\u30b7\u30b9\u30c6\u30e0\u306b\u3088\u308b\u30d1\u30eb\u30b9\u5149\u4fe1\u53f7\u306e\u6e2c\u5b9a\n<\/td>\u5c71\u7530\u8981\u4ecb<\/td><\/tr>
\nJAXA
\u7b2c16\u56de\u3000\u5b87\u5b99\u79d1\u5b66\u30b7\u30f3\u30dd\u30b8\u30a6\u30e0<\/a><\/td>		1\u67086-7\u65e5
JAXA
\u76f8\u6a21\u539f\u30ad\u30e3\u30f3\u30d1\u30b9<\/td>		\nLiteBIRD \u7cfb\u7d71\u8aa4\u5dee (poster)\n<\/td>\u77f3\u91ce\u5b8f\u548c<\/td><\/tr><\/tbody><\/table><\/figure>\n\n\n\n

2015<\/font><\/a><\/h2>\n\n\n\n
\nB-mode from Space<\/td>Dec. 10-16
Kavli, IPMU
Kashiwa<\/td>		\nSimulation\n<\/td>Hirokazu Ishino<\/td><\/tr>
\nB-mode from Space
(poster)<\/td>		Dec. 10-16
Kavli, IPMU
Kashiwa <\/td>		\nIrradiation tests of the LiteBIRD optical components using a 160 MeV proton beam at HIMAC\n<\/td>Kunimoto Komatsu<\/td><\/tr>
\nB-mode from Space
(poster)<\/td>		Dec. 10-16
Kavli, IPMU
Kashiwa <\/td>		\nDevelopment of Lumped Element Kinetic Inductance Detectors for light detection\n<\/td>Yosuke Kida<\/td><\/tr>
\nB-mode from Space
(poster)<\/td>		Dec. 10-16
Kavli, IPMU
Kashiwa <\/td>		\nDevelopment of a readout system of Kinetic Inductance Detectors with FPGA self-triggering for pulsed events\n<\/td>Yosuke Yamada<\/td><\/tr>
\nSOI\u65b0\u5b66\u8853\u9818\u57df
\u7b2c\uff15\u56de\u7814\u7a76\u4f1a<\/td>		12\u67081-2\u65e5
\u9759\u5ca1\u5927\u5b66 <\/td>		\nSOIKID\u3068\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668\n<\/td>\u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
\nCosPA2015<\/a><\/td>Oct. 12-16
KAIST, Munji Camplus
Daejeon, Korea<\/td>		\nLiteBIRD, Lite satellite for the study of B-mode polarization and Inflation from cosmic microwave background Radiation Detection\n<\/td>Hirokazu Ishino<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\n\u79cb\u5b63\u5927\u4f1a<\/a><\/td>		9\u670825\u221228\u65e5
\u5927\u962a\u5e02\u7acb\u5927\u5b66
\uff08\u6749\u672c\u30ad\u30e3\u30f3\u30d1\u30b9\uff09<\/td>		\n\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668KID\u306e\u5468\u6ce2\u6570\u99c6\u52d5\u591a\u91cd\u8aad\u307f\u51fa\u3057\u30b7\u30b9\u30c6\u30e0\u306e\u958b\u767a\n<\/td>\u5c71\u7530\u8981\u4ecb<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\n\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670825\u221228\u65e5
\u5927\u962a\u5e02\u7acb\u5927\u5b66
\uff08\u6749\u672c\u30ad\u30e3\u30f3\u30d1\u30b9\uff09<\/td>		\n\u8efd\u3044\u6697\u9ed2\u7269\u8cea\u63a2\u7d22\u7528\u6db2\u4f53\u30d8\u30ea\u30a6\u30e0TPC\u306b\u7528\u3044\u308b\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668\u306e\u958b\u767a\n<\/td>\u559c\u7530\u6d0b\u4ecb<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\n\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670825\u221228\u65e5
\u5927\u962a\u5e02\u7acb\u5927\u5b66
\uff08\u6749\u672c\u30ad\u30e3\u30f3\u30d1\u30b9\uff09<\/td>		\nLiteBIRD\u306b\u304a\u3051\u308b\u89e3\u6790\u30d7\u30ed\u30b0\u30e9\u30e0\u306e\u958b\u767a\u30681\/f\u30ce\u30a4\u30ba\u30fb\u5b87\u5b99\u7dda\u30b0\u30ea\u30c3\u30c1\u306b\u3088\u308b\u5f71\u97ff\n<\/td>\u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
\nISEC2015
(poster)<\/td>		July 6-9
Nagoya, Japan<\/td>		\nStudy on the Lumped Element Kinetic Inductance Detector for Photon Detection\n<\/td>Hirokazu Ishino<\/td><\/tr>
\nSOIPIX2015<\/a><\/td>Jun2 3-6
Sendai, Japan<\/td>		\nSOIKID, SOI pixel detector combined with the superconducting detector KID\n<\/td>Hirokazu Ishino<\/td><\/tr>
\nI2MTC<\/a>
(poster)<\/td>		May 11-15
Pisa, Italy<\/td>		\nDevelopment of Lumped Element Kinetic Inductance Detectors for Phonon and Photon Detections\n<\/td>Atsuko Kibayashi<\/td><\/tr>
\nHIMAC \u5171\u540c\u5229\u7528\u7814\u7a76\u6210\u679c\u767a\u8868\u4f1a\n<\/td>4 \u6708 20-21 \u65e5
\u5343\u8449<\/td>		\n\u5b87\u5b99\u80cc\u666f\u653e\u5c04\u504f\u5149\u6e2c\u5b9a\u79d1\u5b66\u885b\u661f\u5b9f\u9a13\u3067\u4f7f\u7528\u3059\u308b\u90e8\u6750\u306e\u653e\u5c04\u7dda\u8010\u6027\u306e\u7814\u7a76\n<\/td>\u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c70\u56de\u5e74\u6b21\u5927\u4f1a<\/td>		3\u670821-24\u65e5
\u65e9\u7a32\u7530\u5927\u5b66<\/td>		\n\u6fc3\u7e2e\u30ac\u30c9\u30ea\u30cb\u30a6\u30e0(A=155,157)\u3067\u306e\u71b1\u4e2d\u6027\u5b50\u6355\u7372\u53cd\u5fdc\u304b\u3089\u653e\u51fa\u3055\u308c\u308b\u03b3\u7dda\u6e2c\u5b9a\u5b9f\u9a13\n<\/td>\u8429\u539f\u958b\u4eba<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c70\u56de\u5e74\u6b21\u5927\u4f1a<\/td>		3\u670821-24\u65e5
\u65e9\u7a32\u7530\u5927\u5b66<\/td>		\n200\u20151000MeV\u9818\u57df\u3067\u306e\u96fb\u5b50\u30fb\u30cb\u30e5\u30fc\u30c8\u30ea\u30ce\u3068\u9178\u7d20\u70ad\u7d20\u6e96\u5f3e\u6027\u53cd\u5fdc\u65ad\u9762\u7a4d\u7cbe\u5bc6\u8a08\u7b97\n<\/td>\u4f5c\u7530\u8aa0<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c70\u56de\u5e74\u6b21\u5927\u4f1a<\/td>		3\u670821-24\u65e5
\u65e9\u7a32\u7530\u5927\u5b66<\/td>		\n\u9178\u7d20\u30fb\u70ad\u7d20\u539f\u5b50\u6838\u306e\u5de8\u5927\u5171\u9cf4\u72b6\u614b\u304b\u3089\u653e\u51fa\u3055\u308c\u308b\u03b3\u7dda\u306e\u6e2c\u5b9a\uff1aE398\u30c7\u30fc\u30bf\u89e3\u6790\n<\/td>\u738b\u5ca9<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c70\u56de\u5e74\u6b21\u5927\u4f1a<\/td>		3\u670821-24\u65e5
\u65e9\u7a32\u7530\u5927\u5b66<\/td>		LiteBIRD\u306e\u6982\u8981\u3068\u6210\u7acb\u6027\u306e\u691c\u8a0e\n<\/td>\u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c70\u56de\u5e74\u6b21\u5927\u4f1a<\/td>		3\u670821-24\u65e5
\u65e9\u7a32\u7530\u5927\u5b66<\/td>		LiteBIRD\u3067\u4f7f\u7528\u3059\u308b\u5149\u5b66\u90e8\u6750\u306e\u967d\u5b50\u7dda\u306b\u3088\u308b\u5f71\u97ff\n<\/td>\u821f\u6728\u5de7<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c70\u56de\u5e74\u6b21\u5927\u4f1a<\/td>		3\u670821-24\u65e5
\u65e9\u7a32\u7530\u5927\u5b66<\/td>		\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668\u3068SOI\u691c\u51fa\u5668\u3092\u7d44\u307f\u5408\u308f\u305b\u305fX\u7dda\u691c\u51fa\u5668\u306e\u958b\u767a\uff082\uff09\n<\/td>\u6a39\u6797\u6566\u5b50<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c70\u56de\u5e74\u6b21\u5927\u4f1a<\/td>		3\u670821-24\u65e5
\u65e9\u7a32\u7530\u5927\u5b66<\/td>		\u8efd\u3044\u6697\u9ed2\u7269\u8cea\u63a2\u7d22\u306b\u7528\u3044\u308b\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668\u3068\u6db2\u4f53\u30d8\u30ea\u30a6\u30e0TPC\u306e\u958b\u767a\n<\/td>\u559c\u7530\u6d0b\u4ecb<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c70\u56de\u5e74\u6b21\u5927\u4f1a<\/td>		3\u670821-24\u65e5
\u65e9\u7a32\u7530\u5927\u5b66<\/td>		FPGA\u3092\u7528\u3044\u305f\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668KID(Kinetic Inductance Detector)\u591a\u91cd\u8aad\u307f\u51fa\u3057\u30b7\u30b9\u30c6\u30e0\u306e\u958b\u767a\n<\/td>\u5c71\u7530\u8981\u4ecb<\/td><\/tr>
\n\u65b0\u5b66\u8853\u300c\u5730\u4e0b\u7d20\u6838\u7814\u7a76\u300d
\n\u7b2c\u4e00\u56de\u8d85\u65b0\u661f\u30cb\u30e5\u30fc\u30c8\u30ea\u30ce\u7814\u7a76\u4f1a<\/td>		3\u670816-17\u65e5
\u6771\u4eac\u7406\u79d1\u5927\u5b66<\/td>		\n\u9178\u7d20\u70ad\u7d20\u539f\u5b50\u6838\u306e\u5de8\u5927\u5171\u9cf4\u304b\u3089\u306e\u03b3\u7dda\u6e2c\u5b9a\u3068\u4e2d\u6027\u30ab\u30ec\u30f3\u30c8\u30cb\u30e5\u30fc\u30c8\u30ea\u30ce\u53cd\u5fdc\u691c\u51fa\n<\/td>\u738b\u5ca9<\/td><\/tr>
\n\u65b0\u5b66\u8853\u300c\u5730\u4e0b\u7d20\u6838\u7814\u7a76\u300d
\n\u7b2c\u4e00\u56de\u8d85\u65b0\u661f\u30cb\u30e5\u30fc\u30c8\u30ea\u30ce\u7814\u7a76\u4f1a<\/td>		3\u670816-17\u65e5
\u6771\u4eac\u7406\u79d1\u5927\u5b66<\/td>		\n\u30ac\u30c9\u30ea\u30cb\u30a6\u30e0\u71b1\u4e2d\u6027\u5b50\u53cd\u5fdc\u306b\u3088\u308b\u03b3\u7dda\u751f\u6210\n<\/td>\u4f5c\u7530\u8aa0<\/td><\/tr><\/tbody><\/table><\/figure>\n\n\n\n

2014<\/font><\/a><\/h2>\n\n\n\n
\n\u65b0\u5b66\u8853\u9818\u57df\u300c\u91cf\u5b50\u30a4\u30e1\u30fc\u30b8\u30f3\u30b0\u300d\u7814\u7a76\u4f1a<\/td>11\u670826-27\u65e5
\u91d1\u6ca2\u5de5\u696d\u5927\u5b66<\/td>		SOI\u30d4\u30af\u30bb\u30eb\u3068\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668\u3092\u5408\u4f53\u3057\u305fSOIKID\u306e\u958b\u767a\n<\/td>\u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
\nNNR14 Workshop<\/td>11\u67085-6\u65e5
\u5927\u962a\u5927\u5b66<\/td>		Charged current and Neutral current neutrino-nucleus interaction\n<\/td>\u4f5c\u7530\u8aa0<\/td><\/tr>
\nNNR14 Workshop<\/td>11\u67085-6\u65e5
\u5927\u962a\u5927\u5b66<\/td>		Measurement of \u03b3-rays from giant resonances of 12C and 16O\n<\/td>\u738b\u5ca9<\/td><\/tr>
\n\u8d85\u4f1d\u5c0e\u30a8\u30ec\u30af\u30c8\u30ed\u30cb\u30af\u30b9\u7814\u7a76\u4f1a<\/td>10\u670816-17\u65e5
\u6771\u5317\u5927\u5b66<\/td>		\u30d5\u30a9\u30ce\u30f3\u30fb\u30d5\u30a9\u30c8\u30f3\u691c\u51fa\u7528KID\n<\/td>\u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
\n\u65e5\u7c73\u5408\u540c\u7269\u7406\u5b66\u4f1a Hawaii2014<\/td>10\u67087-11\u65e5
US Hawaii<\/td>		\u03b3-rays from giant resonances of 12C and 16O\n<\/td>\u738b\u5ca9<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
2014\u5e74\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670818-21\u65e5
\u4f50\u8cc0\u5927\u5b66<\/td>		FPGA\u3092\u7528\u3044\u305f\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668KID(Kinetic Inductance Detector)\u7528\u30c7\u30fc\u30bf\u53ce\u96c6\u30b7\u30b9\u30c6\u30e0\u306e\u6982\u8981\n<\/td>\u5c71\u7530\u8981\u4ecb<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
2014\u5e74\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670818-21\u65e5
\u4f50\u8cc0\u5927\u5b66<\/td>		\u6db2\u4f53\u30d8\u30ea\u30a6\u30e0\u3092\u7528\u3044\u305f\u8efd\u3044\u6697\u9ed2\u7269\u8cea\u63a2\u7d22\u7528\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668\u306e\u958b\u767a\n<\/td>\u559c\u7530\u6d0b\u4ecb<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
2014\u5e74\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670818-21\u65e5
\u4f50\u8cc0\u5927\u5b66<\/td>		\u8efd\u3044\u6697\u9ed2\u7269\u8cea\u63a2\u7d22\u3092\u76ee\u6307\u3057\u305f\u8d85\u4f1d\u5c0e\u5149\u691c\u51fa\u5668\u3068\u6db2\u4f53\u30d8\u30ea\u30a6\u30e0\u3092\u7528\u3044\u305fTPC\u306e\u958b\u767a\u306e\u6982\u8981\n<\/td>\u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
2014\u5e74\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670818-21\u65e5
\u4f50\u8cc0\u5927\u5b66<\/td>		\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668\u3068SOI\u691c\u51fa\u5668\u3092\u7d44\u307f\u5408\u308f\u305b\u305fX\u7dda\u691c\u51fa\u5668\u306e\u958b\u767a\n<\/td>\u5ca1\u672c\u6643\u7bc4<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
2014\u5e74\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670818-21\u65e5
\u4f50\u8cc0\u5927\u5b66<\/td>		Super-Kamiokande Gadolinium R&D project:Gd\u6dfb\u52a0\u6c34\u30c1\u30a7\u30ec\u30f3\u30b3\u30d5\u691c\u51fa\u5668EGADS\u306e\u73fe\u72b6\n<\/td>\u68ee\u4fca\u5f70<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
2014\u5e74\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670818-21\u65e5
\u4f50\u8cc0\u5927\u5b66<\/td>		LiteBIRD\u306b\u304a\u3051\u308b\u5b87\u5b99\u7dda\u30681\/f\u30ce\u30a4\u30ba\u306b\u3088\u308b\u7cfb\u7d71\u8aa4\u5dee\u306e\u7814\u7a76\n<\/td>\u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
\n\u65e5\u672c\u5929\u6587\u5b66\u4f1a\u30002014\u5e74\u79cb\u5b63\u5927\u4f1a<\/td>9\u670811-13\u65e5
\u5c71\u5f62\u5927\u5b66<\/td>		\u79d1\u5b66\u885b\u661f\u3092\u7528\u3044\u305f\u5b87\u5b99\u80cc\u666f\u653e\u5c04\u504f\u5149\u7cbe\u5bc6\u6e2c\u5b9a\u8a08\u753bLiteBIRD\u306e\u6982\u8981\n<\/td>\u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
\nNeutrino Oscillation Workshop<\/td>9\u67087-14\u65e5
Italy<\/td>		Prospect for detection of supernova neutrino\n<\/td>\u68ee\u4fca\u5f70<\/td><\/tr>
\n\u65b0\u5b66\u8853\u9818\u57df\u300c\u5730\u4e0b\u7d20\u6838\u7814\u7a76\u300d\u30ad\u30c3\u30af\u30aa\u30d5\u30df\u30fc\u30c6\u30a3\u30f3\u30b0<\/td>8\u670824\u65e5
\u5927\u962a\u5927\u5b66<\/td>		\u8a08\u753b\u7814\u7a76\u300c\u8d85\u65b0\u661f\u80cc\u666f\u30cb\u30e5\u30fc\u30c8\u30ea\u30ce\u89b3\u6e2c\u306b\u3088\u308b\u661f\u5f62\u6210\u306e\u6b74\u53f2\u306e\u7814\u7a76\u300d\n<\/td>\u4f5c\u7530\u8aa0<\/td><\/tr>
\nElba2014 Workshop<\/td>6\u670823-28\u65e5
Elba Island<\/td>		Charged current and Neutral current neutrino-nucleus interaction from 100MeV to 1 GeV\n<\/td>\u4f5c\u7530\u8aa0<\/td><\/tr>
\nNEUTRINO2014
(poster)<\/td>		June 2-7
Boston<\/td>		Recent\tProgress of EGADS\n<\/td>Atsuko Kibayashi<\/td><\/tr>
\nNEUTRINO2014<\/td>June 2-7
Boston<\/td>		Measurement of the Multiplicity and Energy Spectrum of \u03b3-rays from the Thermal Neutron Capture Reaction Gd(n,\u03b3)\n<\/td>\u738b\u5ca9<\/td><\/tr>
\nTIPP2014<\/a><\/td>June 2-6
Amsterdam<\/td>		Development of Microwave Kinetic Inductance Detectors for phonon and photon detections\n<\/td>Hirokazu Ishino<\/td><\/tr>
\n\u80cc\u666f\u653e\u5c04\u3067\u62d3\u304f\u5b87\u5b99\u5275\u6210\u306e\u7269\u7406 \u30b7\u30f3\u30dd\u30b8\u30a6\u30e0<\/a>
(poster)<\/td>		6\u67082-3\u65e5
\u7406\u7814\uff08\u548c\u5149\uff09<\/td>		 Lumped Element KID\u306e\u958b\u767a\u3068\u305d\u306e\u5fdc\u7528<\/td>\u5c71\u7530\u8981\u4ecb<\/td><\/tr>
\nSOI\u65b0\u5b66\u8853\u9818\u57df<\/a>
\u7b2c\u4e8c\u56de\u7814\u7a76\u4f1a<\/td>		5\u67089-10\u65e5
\u5927\u962a\u5927\u5b66<\/td>		\u7a76\u6975\u306e\u30a8\u30cd\u30eb\u30ae\u30fc\u5206\u89e3\u80fd\u3092\u6301\u3064\u5927\u9762\u7a4d\uff38\u7dda\u691c\u51fa\u5668\u306e\u958b\u767a\n<\/td>\u77f3\u91ce\u3000\u5b8f\u548c<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\n \u7b2c69\u56de\u5e74\u6b21\u5927\u4f1a<\/a><\/td>		3\u670827-30\u65e5
\u6771\u6d77\u5927\u5b66<\/td>		\u5b87\u5b99\u30de\u30a4\u30af\u30ed\u6ce2\u80cc\u666f\u653e\u5c04\u504f\u5149\u89b3\u6e2c\u7528\u691c\u51fa\u5668 MKIDs(Microwave Kinetic Inductance Detectors) \u306b\u304a\u3051\u308b\u591a\u30c1\u30e3\u30f3\u30cd\u30eb\u8aad\u307f\u51fa\u3057\u7cfb\u306e\u958b\u767a\uff085\uff09\n<\/td>\u5c90\u90e8\u4f73\u6717<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c69\u56de\u5e74\u6b21\u5927\u4f1a<\/td>		3\u670827-30\u65e5
\u6771\u6d77\u5927\u5b66<\/td>		\u8efd\u3044\u6697\u9ed2\u7269\u8cea\u63a2\u7d22\u306b\u5229\u7528\u53ef\u80fd\u306a\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668Microwave Kinetic Inductance detector(MKID)\u306e\u958b\u767a\n<\/td>\u5c71\u7530\u8981\u4ecb<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c69\u56de\u5e74\u6b21\u5927\u4f1a<\/td>		3\u670827-30\u65e5
\u6771\u6d77\u5927\u5b66<\/td>		\u691c\u51fa\u52b9\u7387\u3092\u6539\u5584\u3057\u305f\u8d85\u4f1d\u5c0e\u30d5\u30a9\u30ce\u30f3\u691c\u51fa\u5668\u306e\u958b\u767a\n<\/td>\u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c69\u56de\u5e74\u6b21\u5927\u4f1a<\/td>		3\u670827-30\u65e5
\u6771\u6d77\u5927\u5b66<\/td>		\u30ac\u30c9\u30ea\u30cb\u30a6\u30e0\u306e\u71b1\u4e2d\u6027\u5b50\u6355\u7372\u304b\u3089\u653e\u51fa\u3055\u308c\u308b\u03b3\u7dda\u306e\u6e2c\u5b9a\uff1a\u8a08\u7b97\u3068\u6bd4\u8f03\n<\/td>\u5c71\u7530\u82b3\u5e78<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c69\u56de\u5e74\u6b21\u5927\u4f1a<\/td>		3\u670827-30\u65e5
\u6771\u6d77\u5927\u5b66<\/td>		\u30ac\u30c9\u30ea\u30cb\u30a6\u30e0\u306e\u71b1\u4e2d\u6027\u5b50\u6355\u7372\u53cd\u5fdc\u304b\u3089\u653e\u51fa\u3055\u308c\u308b\u03b3\u7dda\u6e2c\u5b9a\uff1a\u5b9f\u9a13\u30c7\u30fc\u30bf\u89e3\u6790\n<\/td>\u738b\u5ca9<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c69\u56de\u5e74\u6b21\u5927\u4f1a<\/td>		3\u670827-30\u65e5
\u6771\u6d77\u5927\u5b66<\/td>		Super-Kamiokande Gadolinium R&D Project\uff1aGd\u6dfb\u52a0\u6c34\u30c1\u30a7\u30ec\u30f3\u30b3\u30d5\u691c\u51fa\u5668EGADS\u306b\u304a\u3051\u308bGd\u306e\u4e2d\u6027\u5b50\u6355\u7372\u306b\u3088\u308b\u30ac\u30f3\u30de\u7dda\u4e8b\u8c61\u306e\u89e3\u6790\n<\/td>\u68ee\u4fca\u5f70<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c69\u56de\u5e74\u6b21\u5927\u4f1a<\/td>		3\u670827-30\u65e5
\u6771\u6d77\u5927\u5b66<\/td>		Super-Kamiokande Gadolinium R&D Project: Gd\u6dfb\u52a0\u6c34\u30c1\u30a7\u30ec\u30f3\u30b3\u30d5\u691c\u51fa\u5668 \u5b9f\u8a3c\u5b9f\u9a13EGADS\u306e\u73fe\u72b6
\n<\/td>		\u77e2\u91ce\u5b5d\u81e3<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c69\u56de\u5e74\u6b21\u5927\u4f1a<\/td>		3\u670827-30\u65e5
\u6771\u6d77\u5927\u5b66<\/td>		LiteBIRD\u7126\u70b9\u9762\u691c\u51fa\u5668\u306e\u653e\u5c04\u7dda\u306b\u3088\u308b\u5f71\u97ff1\n<\/td>\u6a39\u6797\u6566\u5b50<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c69\u56de\u5e74\u6b21\u5927\u4f1a<\/td>		3\u670827-30\u65e5
\u6771\u6d77\u5927\u5b66<\/td>		\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668LEKID(Lumped Element Kinetic Inductance Detector)\u306e\u591a\u7d20\u5b50\u5316\u914d\u5217\u306b\u5411\u3051\u305f\u7814\u7a76\n<\/td>\u5ca1\u672c\u6643\u7bc4<\/td><\/tr>
\n\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c69\u56de\u5e74\u6b21\u5927\u4f1a<\/td>		3\u670827-30\u65e5
\u6771\u6d77\u5927\u5b66<\/td>		Super-Kamiokande Gadolinium R&D project:Gd\u6dfb\u52a0\u6c34\u30c1\u30a7\u30ec\u30f3\u30b3\u30d5\u691c\u51fa\u5668EGADS\u306b\u304a\u3051\u308bGd\u306e\u4e2d\u6027\u5b50\u6355\u7372\u306b\u3088\u308b\u30ac\u30f3\u30de\u7dda\u4e8b\u8c61\u306e\u89e3\u6790\n<\/td>\u68ee\u4fca\u5f70<\/td><\/tr>
\n\u7b2c20\u56deICEPP\u30b7\u30f3\u30dd\u30b8\u30a6\u30e0<\/td>2\u670823-26\u65e5
\u9577\u91ce\u770c<\/td>		Gd\u71b1\u4e2d\u6027\u5b50\u6355\u7372\u53cd\u5fdc\u3067\u653e\u51fa\u3055\u308c\u308b\u03b3\u7dda\u306e\u6e2c\u5b9a
\n<\/td>		\u738b\u5ca9<\/td><\/tr>
\n\u65b0\u5b66\u8853\u9818\u57df\u5929\u4f53\u6ce2\u5929\u4f53\u306e\u591a\u69d8\u306a\u89b3\u6e2c\u306b\u3088\u308b\u5b87\u5b99\u7269\u7406\u5b66\u306e\u65b0\u5c55\u958b\u7b2c\u4e8c\u56de\u30b7\u30f3\u30dd\u30b8\u30a6\u30e0\u82e5\u624b\u30bb\u30c3\u30b7\u30e7\u30f3<\/td>1\u670813\u65e5-15\u65e5
\u6771\u4eac\u5de5\u696d\u5927\u5b66<\/td>		Supernova Neutrino Search and Information Sharing\n<\/td>\u68ee\u4fca\u5f70<\/td><\/tr>
\n\u65b0\u5b66\u8853\u9818\u57df\u300c\u91cd\u529b\u5929\u4f53\u300d\u30b7\u30f3\u30dd\u30b8\u30a6\u30e0<\/td>1\u670813\u65e5
\u6771\u5de5\u5927<\/td>		Report on thermal neutron capture reaction Gd(n,gamma)\n<\/td>\u4f5c\u7530\u8aa0<\/td><\/tr>
\n\u7b2c14\u56de\u5b87\u5b99\u79d1\u5b66\u30b7\u30f3\u30dd\u30b8\u30a6\u30e0
(poster)<\/td>		1\u67089-10\u65e5
JAXA \u5b87\u5b99\u79d1\u5b66\u7814\u7a76\u6240<\/td>		LiteBIRD \u306e\u30b5\u30a4\u30a8\u30f3\u30b9\u3068\u885b\u661f\u6982\u8981\n<\/td>\u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
\n\u7b2c14\u56de\u5b87\u5b99\u79d1\u5b66\u30b7\u30f3\u30dd\u30b8\u30a6\u30e0
(poster)<\/td>		1\u67089-10\u65e5
JAXA \u5b87\u5b99\u79d1\u5b66\u7814\u7a76\u6240<\/td>		\u5b87\u5b99\u30de\u30a4\u30af\u30ed\u6ce2\u80cc\u666f\u653e\u5c04\u504f\u5149\u89b3\u6e2c\u7528\u691c\u51fa\u5668MKID\u306b\u304a\u3051\u308b\u5468\u6ce2\u6570\u9818\u57df\u3067\u306e\u4fe1\u53f7\u591a\u91cd\u5316\u3092\u7528\u3044\u305f\u8aad\u307f\u51fa\u3057\u7cfb\u306e\u958b\u767a\n<\/td>\u5c90\u90e8\u4f73\u6717<\/td><\/tr>
\n\u7b2c14\u56de\u5b87\u5b99\u79d1\u5b66\u30b7\u30f3\u30dd\u30b8\u30a6\u30e0
(poster)<\/td>		1\u67089-10\u65e5
JAXA \u5b87\u5b99\u79d1\u5b66\u7814\u7a76\u6240<\/td>		CMB\u504f\u5149\u89b3\u6e2c\u885b\u661f LiteBIRD \u306e\u7cfb\u7d71\u8aa4\u5dee\u7814\u7a76
\n<\/td>		\u6c38\u7530\u7adc(KEK), \u6a39\u6797\u6566\u5b50<\/td><\/tr><\/tbody><\/table><\/figure>\n\n\n\n

2013<\/font><\/a><\/h2>\n\n\n\n
KEK Detector Technology Project
\n
International Review Committee 2013<\/td>		Dec. 10-11
KEK<\/td>		Developments of STJ for millimeter waves and MKID for phonons and photons
\n<\/td>		Hirokazu Ishino<\/td><\/tr>
KEK Detector Technology Project
\n
International Review Committee 2013<\/a><\/td>		Dec. 10-11
KEK<\/td>		Development of MKID readout system
\n<\/td>		Yoshiaki Kibe<\/td><\/tr>
\u5b87\u5b99\u80cc\u666f\u653e\u5c04\u3092\u542b\u3080\u30df\u30ea\u6ce2\u30fb\u30b5\u30d6\u30df\u30ea\u6ce2\u89b3\u6e2c\u306e\u30b7\u30b9\u30c6\u30e0
\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d7<\/a><\/td>		11\u670829-30\u65e5
\u5009\u6577\u30b7\u30fc\u30b5\u30a4\u30c9\u30db\u30c6\u30eb<\/td>		GroundBIRD\/LiteBIRD\u306b\u304a\u3051\u308b\u8aad\u307f\u51fa\u3057
\n<\/td>		\u5c90\u90e8\u4f73\u6717<\/td><\/tr>
\u5b87\u5b99\u80cc\u666f\u653e\u5c04\u3092\u542b\u3080\u30df\u30ea\u6ce2\u30fb\u30b5\u30d6\u30df\u30ea
\n\u6ce2\u89b3\u6e2c\u306e\u30b7\u30b9\u30c6\u30e0
\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d7<\/td>		11\u670829-30\u65e5
\u5009\u6577\u30b7\u30fc\u30b5\u30a4\u30c9\u30db\u30c6\u30eb<\/td>		LiteBIRD\u3067\u4e88\u6e2c\u3055\u308c\u308b\u653e\u5c04\u7dda\n<\/td>\u6a39\u6797\u6566\u5b50<\/td><\/tr>
\u96fb\u5b50\u60c5\u5831\u901a\u4fe1\u5b66\u4f1a
\u8d85\u4f1d\u5c0e\u30a8\u30ec\u30af\u30c8\u30ed\u30cb\u30af\u30b9\u7814\u7a76\u4f1a<\/a><\/td>		10\u67082-3\u65e5
\u6771\u5317\u5927\u5b66 \u96fb\u6c17\u901a\u4fe1\u7814\u7a76\u6240<\/td>		MKID\u3068\u5b87\u5b99\u30fb\u7d20\u7c92\u5b50\u5b9f\u9a13\u3078\u306e\u5fdc\u7528\n<\/td>\u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670820-23\u65e5
\u9ad8\u77e5\u5927\u5b66<\/td>		JPARC-MLF\u306e\u4e2d\u6027\u5b50\u6838\u53cd\u5fdc\u6e2c\u5b9a\u88c5\u7f6e(ANNRI)\u3092\u4f7f\u3063\u305f\u30ac\u30c9\u30ea\u30cb\u30a6\u30e0\u306e\u71b1\u4e2d\u6027\u5b50\u6355\u7372\u5b9f\u9a13\uff1a\u5b9f\u9a13\u6982\u8981\u3068\u30b7\u30df\u30e5\u30ec\u30fc\u30b7\u30e7\u30f3\n<\/td>\u5c71\u7530\u82b3\u5e78<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670820-23\u65e5
\u9ad8\u77e5\u5927\u5b66<\/td>		JPARC-MLF\u306e\u4e2d\u6027\u5b50\u6838\u53cd\u5fdc\u6e2c\u5b9a\u88c5\u7f6e(ANNRI)\u3092\u4f7f\u3063\u305f\u30ac\u30c9\u30ea\u30cb\u30a6\u30e0\u306e\u71b1\u4e2d\u6027\u5b50\u6355\u7372\u5b9f\u9a13\uff1a\u30c7\u30fc\u30bf\u89e3\u6790\u72b6\u6cc1\n<\/td>\u738b\u5ca9<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670820-23\u65e5
\u9ad8\u77e5\u5927\u5b66<\/td>		\u30b9\u30fc\u30d1\u30fc\u30ab\u30df\u30aa\u30ab\u30f3\u30c7\u306b\u304a\u3051\u308b\u8d85\u65b0\u661f\u7206\u767a\u30cb\u30e5\u30fc\u30c8\u30ea\u30ce\u30e2\u30cb\u30bf\u30fc\u306e\u958b\u767a\n<\/td>\u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670820-23\u65e5
\u9ad8\u77e5\u5927\u5b66<\/td>		Microwave Kinetic Inductance Detector(MKID)\u306e\u53ef\u8996\u5149\u53cd\u5fdc\u306e\u7814\u7a76\n<\/td>\u5c71\u7530\u8981\u4ecb<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670820-23\u65e5
\u9ad8\u77e5\u5927\u5b66<\/td>		\u5b87\u5b99\u30de\u30a4\u30af\u30ed\u6ce2\u80cc\u666f\u653e\u5c04\u504f\u5149\u89b3\u6e2c\u7528\u691c\u51fa\u5668 MKIDs(Microwave Kinetic Inductance Detectors) \u306b\u304a\u3051\u308b\u591a\u30c1\u30e3\u30f3\u30cd\u30eb\u8aad\u307f\u51fa\u3057\u7cfb\u306e\u958b\u767a\uff084\uff09\n<\/td>\u5c90\u90e8\u4f73\u6717<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670820-23\u65e5
\u9ad8\u77e5\u5927\u5b66<\/td>		\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668Lumped Element Kinetic Inductance Detector(LEKID)\u306e\u7814\u7a76\n<\/td>\u5ca1\u672c\u6643\u7bc4<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670820-23\u65e5
\u9ad8\u77e5\u5927\u5b66<\/td>		Super-Kamiokande Gadolinium R&D Project: Gd\u30c6\u30b9\u30c8\u5b9f\u8a3c\u5b9f\u9a13\u3068\u305d\u306e\u6c34\u30c1\u30a7\u30ec\u30f3\u30b3\u30d5\u691c\u51fa\u5668\u5efa\u8a2d\u306e\u73fe\u72b6\n<\/td>\u6a39\u6797\u6566\u5b50<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670820-23\u65e5
\u9ad8\u77e5\u5927\u5b66<\/td>		Super-Kamiokande Gadolinium R&D Project\uff1aSK-IV\u306b\u304a\u3051\u308b\u30ac\u30c9\u30ea\u30cb\u30a6\u30e0\u306e\u4e2d\u6027\u5b50\u6355\u7372\u306b\u3088\u308b\u30ac\u30f3\u30de\u7dda\u4e8b\u8c61\u3068\u30d0\u30c3\u30af\u30b0\u30e9\u30a6\u30f3\u30c9\u306e\u8a55\u4fa1\n<\/td>\u68ee\u4fca\u5f70<\/td><\/tr>
WIN2013<\/td>Sept. 16-21
Natal, Brazil<\/td>		GADZOOKS!<\/td>Takatomi Yano<\/td><\/tr>
\u7b2c4\u56de\u65e5\u672c\u4e2d\u6027\u5b50\u6355\u7372\u533b\u7642\u5b66\u4f1a<\/td>9\u67087\u65e5
\u5ca1\u5c71\u5927\u5b66<\/td>		\u71b1\u4e2d\u6027\u5b50\u30ac\u30c9\u30ea\u30cb\u30a6\u30e0\u6355\u7372\u53cd\u5fdc\u306b\u304a\u3051\u308b\u30ac\u30f3\u30de\u7dda\u751f\u6210Gd(n,g)\u306e\u7814\u7a76\u3068\u7d20\u7c92\u5b50\u30cb\u30e5\u30fc\u30c8\u30ea\u30ce\u7269\u7406\u5206\u91ce\u3067\u306e\u30ac\u30c9\u30ea\u30cb\u30a6\u30e0\u306e\u5fdc\u7528<\/td>\u4f5c\u7530\u8aa0<\/td><\/tr>
APPC12<\/td>July 14-19
Makuhari Messe<\/td>		Latest Results from Super-Kamiokande<\/td>Hirokazu Ishino<\/td><\/tr>
APPC12
(poster)<\/td>		July 14-19
Makuhari Messe<\/td>		Development of the Superconducting Detectors for Applications to Particle Physics and Astrophysics<\/td>Atsuko Kibayashi<\/td><\/tr>
LTD15
(poster)<\/td>		June 24-28
Cal Tech<\/td>		Development of Microwave Kinetic Inductance Detectors for a Detection of Phonons<\/td>Hirokazu Ishino<\/td><\/tr>
LTD15
(poster)<\/td>		June 24-28
Cal Tech<\/td>		Low Noise Readout System for MKIDs with Frequency-domain Multiplexing Technique towards Application of CMB Observation <\/td>Yoshiaki Kibe<\/td><\/tr>
RENO-50<\/td>June 13-14
Seuol National Univ.<\/td>		 Future SK programs on reactor, relic supernova, and galactic supernova neutrinos<\/td>Atsuko Kibayashi<\/td><\/tr>
CMB2013
(poster)<\/td>		June 10-14
Okinawa<\/td>		Low noise readout system for MKIDs with frequency-domain multiplexing technique towards application of CMB observation <\/td>Yoshiaki Kibe<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a<\/td>3\u670826-29\u65e5
\u5e83\u5cf6\u5927\u5b66<\/td>		\u8d85\u4f1d\u5c0e\u30d5\u30a9\u30ce\u30f3\u691c\u51fa\u5668\u306e\u958b\u767a\uff14<\/td>\u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a<\/td>3\u670826-29\u65e5
\u5e83\u5cf6\u5927\u5b66<\/td>		\u5b87\u5b99\u30de\u30a4\u30af\u30ed\u6ce2\u80cc\u666f\u653e\u5c04\u504f\u5149\u89b3\u6e2c\u7528\u691c\u51fa\u5668MKID\u306b\u304a\u3051\u308b\u591a\u30c1\u30e3\u30f3\u30cd\u30eb\u8aad\u307f\u51fa\u3057\u7cfb\u306e\u958b\u767a\uff08\uff13\uff09<\/td>\u5c90\u90e8\u4f73\u6717<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a<\/td>3\u670826-29\u65e5
\u5e83\u5cf6\u5927\u5b66<\/td>		Microwave Kinetic Inductance Detector(MKID)\u306e\u53ef\u8996\u5149\u53cd\u5fdc\u306e\u7814\u7a76<\/td>\u5c71\u7530\u8981\u4ecb<\/td><\/tr>
VCI2013<\/td>February 11-15
Vienna, Austria<\/td>		Status of Super-Kamiokande gadolinium project<\/td>Takaaki Mori<\/td><\/tr><\/tbody><\/table><\/figure>\n\n\n\n

2012<\/font><\/a><\/h2>\n\n\n\n
\u6771\u4eac\u5927\u5b66\u5b87\u5b99\u7dda\u7814\u7a76\u6240
\u5e73\u6210\uff12\uff14\u5e74\u5ea6\u5171\u540c\u5229\u7528\u7814\u7a76\u767a\u8868\u4f1a<\/td>		12\u67087-8\u65e5
\u6771\u4eac\u5927\u5b66\u67cf\u30ad\u30e3\u30f3\u30d1\u30b9\u3000<\/td>		\u30b9\u30fc\u30d1\u30fc\u30ab\u30df\u30aa\u30ab\u30f3\u30c7\uff08\u592a\u967d\u30cb\u30e5\u30fc\u30c8\u30ea\u30ce\u3001\u8d85\u65b0\u661f\u30cb\u30e5\u30fc\u30c8\u30ea\u30ce\u7b49)<\/td>\u6a39\u6797\u6566\u5b50<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670811-14\u65e5
\u4eac\u90fd\u7523\u696d\u5927<\/td>		\u9178\u7d20\u30fb\u70ad\u7d20\u539f\u5b50\u6838\u306e\u5de8\u5927\u5171\u9cf4\u72b6\u614b\u304b\u3089\u306e\u653e\u5c04\u03b3\u7dda\u6e2c\u5b9a\u5b9f\u9a13\u306e\u8a2d\u8a08<\/td>\u738b\u5ca9<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670811-14\u65e5
\u4eac\u90fd\u7523\u696d\u5927<\/td>		Super-Kamiokande Gadolinium R&D Project:200\u30c8\u30f3\u6c34 \u30c1\u30a7\u30ec \u30f3\u30b3 \u30d5\u691c\u51fa\u5668\u306e\u30c7\u30fc\u30bf\u53ce\u96c6\u30b7\u30b9\u30c6\u30e0\u3068\u691c\u51fa\u5668\u306e\u6027\u80fd\u8a55\u4fa1<\/td>\u68ee\u4fca\u5f70<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670811-14\u65e5
\u4eac\u90fd\u7523\u696d\u5927<\/td>		Super-Kamiokande Gadolinium R&D Project:\u30ac\u30c9\u30ea\u30cb\u30a6\u30e0\u3092\u542b\u3080\u6c34 \u306e\u5faa\u74b0\u624b\u6cd5\u304a\u3088\u3073\u900f\u904e\u7387\u306e\u7814\u7a76<\/td>\u77e2\u91ce\u5b5d\u81e3<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670811-14\u65e5
\u4eac\u90fd\u7523\u696d\u5927<\/td>		Super-Kamiokande Gadolinium R&D Project: Am\/Be\u7dda\u6e90\u30682.4\u2113\u30ac
\n\u30c9\u30ea\u30cb\u30a6\u30e0\u6c34\u6eb6\u6db2\u3092\u7528\u3044\u305f\u4e2d\u6027\u5b50\u6355\u7372\u30ac\u30f3\u30de\u7dda\u4e8b\u8c61\u306e\u89e3\u6790<\/td>		\u5c71\u53e3\u7adc\u592a<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670811-14\u65e5
\u4eac\u90fd\u7523\u696d\u5927<\/td>		\u8d85\u4f1d\u5c0e\u30d5\u30a9\u30ce\u30f3\u691c\u51fa\u5668\uff13<\/td>\u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670811-14\u65e5
\u4eac\u90fd\u7523\u696d\u5927<\/td>		\u30cb\u30aa\u30d6\u3068\u30a2\u30eb\u30df\u30cb\u30a6\u30e0\u3092\u7d44\u307f\u5408\u308f\u305b\u305f\u30b9\u30c8\u30ea\u30c3\u30d7\u578bMicrowaveKinetic Inductance Detector (MKID)\u306e\u958b\u767a<\/td>\u6e6f\u6d45\u6cf0\u6c17<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670811-14\u65e5
\u4eac\u90fd\u7523\u696d\u5927<\/td>		\u5b87\u5b99\u30de\u30a4\u30af\u30ed\u6ce2\u80cc\u666f\u653e\u5c04\u504f\u5149\u89b3\u6e2c\u7528\u691c\u51fa\u5668 MKIDs(Microwave Kinetic Inductance Detectors)\u306b\u304a\u3051\u308b\u591a\u30c1\u30e3\u30f3\u30cd\u30eb\u8aad\u307f\u51fa\u3057\u7cfb\u306e\u958b\u767a\uff08\uff12\uff09<\/td>\u5c90\u90e8\u4f73\u6717<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670811-14\u65e5
\u4eac\u90fd\u7523\u696d\u5927<\/td>		\u8d85\u4f1d\u5c0e\u30c8\u30f3\u30cd\u30eb\u63a5\u5408\u7d20\u5b50(STJ)\u3092\u3082\u3061\u3044\u305f\u5b87\u5b99\u30de\u30a4\u30af\u30ed\u6ce2\u80cc\u666f\u653e\u5c04\u504f\u5149\u89b3\u6e2c\u30ab\u30e1\u30e9\u306e\u958b\u767a<\/td>\u7f8e\u99ac\u899a<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670811-14\u65e5
\u4eac\u90fd\u7523\u696d\u5927<\/td>		\u30cb\u30aa\u30d6Microwave Kinetic Inductance Detector (MKID) \u306e\u57fa\u790e\u7279\u6027<\/td>\u5c71\u7530\u8981\u4ecb<\/td><\/tr>
36th International Conference on High Energy Physics <\/td>4-11 July 2012.
Melbourne Convention and Exhibition Centre<\/td>		Status of the Gadolinium project for Super-Kamiokande<\/td>Takatomi Yano\u3000<\/td><\/tr>
The 4th International Symposium on Neutrinos and Dark Matter in Nuclear Physics<\/td>June 13th,
2012
(NDM12)
Nara, Japan<\/td>		Neutrino-nucleus interactions relevant to atmospheric neutrinos &neutrino oscillation experiments<\/td>M.Sakuda<\/td><\/tr>
Neutrino2012
(poster)<\/td>		June 3-9
Kyoto<\/td>		R&D status of O,C(p,p\u2019) and (He,t) experiment at RCNP<\/td>Iwa Ou (R.Yamaguchi, T.Mori, T.Yano, M.Sakuda, A.Tamii, T.Suzuki, M.Yosoi, A.Ankowski, and O.Benhar<\/td><\/tr>
Neutrino2012
(poster)<\/td>		June 3-9
Kyoto<\/td>		Supernova neutrino monitor at Super-Kamiokande<\/td>Hirokazu Ishino (The Super-Kamiokande Collaboration)<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c67\u56de\u5e74\u6b21\u5927\u4f1a<\/td>		3\u670824-27\u65e5
\u95a2\u897f\u5b66\u9662\u5927\u5b66<\/td>		\u30a2\u30eb\u30df\u8d85\u4f1d\u5c0e\u30c8\u30f3\u30cd\u30eb\u63a5\u5408\u7d20\u5b50(STJ)\u3092\u3082\u3061\u3044\u305f\u5b87\u5b99\u30de\u30a4\u30af\u30ed\u6ce2\u80cc\u666f\u653e\u5c04\u504f\u5149\u89b3\u6e2c\u30ab\u30e1\u30e9\u306e\u958b\u767a<\/td>\u7f8e\u99ac\u899a<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c67\u56de\u5e74\u6b21\u5927\u4f1a<\/td>		3\u670824-27\u65e5
\u95a2\u897f\u5b66\u9662\u5927\u5b66<\/td>		\u5b87\u5b99\u30de\u30a4\u30af\u30ed\u6ce2\u80cc\u666f\u653e\u5c04\u504f\u5411\u89b3\u6e2c\u7528\u691c\u51fa\u5668 MKIDs(Microwave Kinetic Inductance Detectors) \u306b\u304a\u3051\u308b\u591a\u30c1\u30e3\u30f3\u30cd\u30eb\u8aad\u307f\u51fa\u3057\u7cfb\u306e\u958b\u767a<\/td>\u5c90\u90e8\u4f73\u660e<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c67\u56de\u5e74\u6b21\u5927\u4f1a<\/td>		3\u670824-27\u65e5
\u95a2\u897f\u5b66\u9662\u5927\u5b66<\/td>		\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668Microwave Kinetic Inductance Detector\u306e\u57fa\u790e\u7279\u6027\u306e\u7814\u7a76<\/td>\u5c71\u7530\u8981\u4ecb<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c67\u56de\u5e74\u6b21\u5927\u4f1a<\/td>		3\u670824-27\u65e5
\u95a2\u897f\u5b66\u9662\u5927\u5b66<\/td>		\u8d85\u4f1d\u5c0e\u30c8\u30f3\u30cd\u30eb\u63a5\u5408\u7d20\u5b50(STJ)\u88fd\u4f5c\u6761\u4ef6\u306e\u6700\u9069\u5316<\/td>\u6e6f\u6d45\u6cf0\u6c17<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c67\u56de\u5e74\u6b21\u5927\u4f1a<\/td>		3\u670824-27\u65e5
\u95a2\u897f\u5b66\u9662\u5927\u5b66<\/td>		Super-Kamiokande Gadolinium R&D Project:200\u30c8\u30f3\u6c34\u30c1\u30a7\u30ec\u30f3\u30b3\u30d5\u691c\u51fa\u5668\u306e\u5efa\u8a2d\u72b6\u6cc1\u3068\u30c7\u30fc\u30bf\u53ce\u96c6\u30b7\u30b9\u30c6\u30e0<\/td>\u68ee\u4fca\u5f70
\u77e2\u91ce\u5b5d\u81e3
\u7af9\u5185\u6df3\u609f
\u5c71\u53e3\u7adc\u592a
\u4f5c\u7530\u8aa0
\u6a39\u6797\u6566\u5b50
\u77f3\u91ce\u5b8f\u548c
\u4e0a\u91ce\u6602A
\u5cb8\u672c\u5eb7\u5b8fA
\u5c0f\u6c50\u7531\u4ecbA
\u95a2\u8c37\u6d0b\u4e4bA
\u7af9\u7530\u6566A
\u4e2d\u7551\u96c5\u884cA
\u6a2a\u6fa4\u5b5d\u7ae0A
L.MartiA
\u7af9\u5185\u5eb7\u96c4B
L.LabargaC
K.BaysD
G.CarminatiD
A.RenshawD
M.SmyD
M.VaginsE
H.ZhangF
J.StoneG
for the Super-K Collaboration)<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c67\u56de\u5e74\u6b21\u5927\u4f1a<\/td>		3\u670824-27\u65e5
\u95a2\u897f\u5b66\u9662\u5927\u5b66<\/td>		Super-Kamiokande Gadolinium R&D Project:200\u30c8\u30f3\u5b9f\u8a3c\u6a5f\u306b\u4f7f\u3046240\u672c\u306e\u5149\u96fb\u5b50\u5897\u500d\u7ba1\u306e\u4e8b\u524d\u6027\u80fd\u8a55\u4fa1<\/td>\u5c71\u53e3\u7adc\u592a
\u68ee\u4fca\u5f70
\u7af9\u5185\u6df3\u609f
\u4f5c\u7530\u8aa0
\u6a39\u6797\u6566\u5b50
\u77f3\u91ce\u5b8f\u548c
\u77e2\u91ce\u5b5d\u81e3
\u4e0a\u91ce\u6634A
\u5cb8\u672c\u5eb7\u5f18A
\u5c0f\u6c50\u7531\u4ecbA
\u95a2\u8c37\u6d0b\u4e4bA
\u7af9\u7530\u6566A
\u4e2d\u7551\u96c5\u884cA
\u6a2a\u6fa4\u5b5d\u5f70A
L.MartiA
\u4e2d\u91ce\u4f51\u6a39A
\u7af9\u5185\u5eb7\u96c4B
L.LabargaC
P.FernandezC
K.BaysD
G.CarminatiD
A.RenshawD
M.SmyD
M.VaginsE
H.ZhangF
J.StoneGfor the Super-K Collaboration<\/td><\/tr>
\u5927\u962a\u5927\u5b66\u6838\u7269\u7406\u7814\u7a76\u30bb\u30f3\u30bf\u30fc
\u5b9f\u9a13\u63d0\u6848\u59d4\u54e1\u4f1a\u3067\u306e\u767a\u8868<\/td>		3\u670815\u65e5
\u5927\u962a\u5927\u5b66\u6838\u7269\u7406\u7814\u7a76\u30bb\u30f3\u30bf\u30fc<\/td>		Proposed experiment to measure g-rays from O(p,p’)O* in relation to O(n,n’g)X<\/td>M.Sakuda<\/td><\/tr>
RCNP \u30b3\u30ed\u30ad\u30a6\u30e0<\/td>1\u670826\u65e5
\u5927\u962a\u5927\u5b66
\u6838\u7269\u7406\u7814\u7a76\u30bb\u30f3\u30bf\u30fc<\/td>		Proposed experiment to measure g-rays from O(p,p’)O* in relation to O(n,n’g) X<\/td>M.Sakuda<\/td><\/tr>
\u6771\u5317\u5927\u5b66
\u30cb\u30e5\u30fc\u30c8\u30ea\u30ce\u30bb\u30f3\u30bf\u30fc\u30bb\u30df\u30ca\u30fc<\/td>		1\u670824\u65e5
\u6771\u5317\u5927\u5b66<\/td>		\u30cb\u30e5\u30fc\u30c8\u30ea\u30ce\u9178\u7d20\u53cd\u5fdc\u3067\u306e\u30ac\u30f3\u30de\u7dda\u751f\u6210<\/td>M.Sakuda<\/td><\/tr><\/tbody><\/table><\/figure>\n\n\n\n

2011<\/font><\/a><\/h2>\n\n\n\n
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670816\uff5e19\u65e5
\u5f18\u524d\u5927\u5b66<\/td>		RCNP\u3067\u306e16O\uff08p,p’\uff09\u5b9f\u9a13\u3067\u4f7f\u7528\u3059\u308b\u30ac\u30f3\u30de\u7dda\u691c\u51fa\u5668\u306e\u6027\u80fd\u8a55\u4fa1<\/td>\u6cc9\u5353\u5b8f
\u68ee\u4fca\u5f70
\u5c71\u53e3\u7adc\u592a
\u4f5c\u7530\u8aa0
\u6c11\u4e95\u6df3A
\u9234\u6728\u667a\u548cA
\u8207\u66fe\u4e95\u512aA<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670816\uff5e19\u65e5
\u5f18\u524d\u5927\u5b66
<\/td>		Super-Kamiokande Gadolinium R&D Project: Gd\u30c6\u30b9\u30c8\u5b9f\u8a3c\u65bd\u8a2d\u5efa\u8a2d\u306e\u73fe\u72b6<\/td>\u6a39\u6797\u6566\u5b50
\u77f3\u91ce\u5b8f\u548c
\u4f5c\u7530\u8aa0
\u7af9\u5185\u6df3\u609f
\u68ee\u4fca\u5f70
\u5c71\u53e3\u7adc\u592a
\u4e0a\u91ce\u6602A
\u5cb8\u672c\u5eb7\u5b8fA
\u5c0f\u6c50\u7531\u4ecbA
\u95a2\u8c37\u6d0b\u4e4bA
\u7af9\u7530\u6566A
\u4e2d\u7551\u96c5\u884cA
\u6a2a\u6fa4\u5b5d\u7ae0A
L.MartiA
\u7af9\u5185\u5eb7\u96c4B
L.LabargaC
K.BaysD
G.CarminatiD
A.RenshawD
M.SmyD
M.VaginsE
H.ZhangF
for the Super-K Collaboration<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670816\uff5e19\u65e5
\u5f18\u524d\u5927\u5b66<\/td>		Super-Kamiokande Gadolinium R&D Project:200\u30c8\u30f3\u5b9f\u8a3c\u65bd\u8a2d\u306b\u88c5\u7740\u4e88\u5b9a\u306e\u5149\u96fb\u5b50\u5897\u500d\u7ba1240\u672c\u306e\u4e8b\u524d\u8f03\u6b63<\/td>\u68ee\u4fca\u5f70
\u7af9\u5185\u6df3\u609f
\u5c71\u53e3\u7adc\u592a
\u4f5c\u7530\u8aa0
\u6a39\u6797\u6566\u5b50
\u77f3\u91ce\u5b8f\u548c
\u4e0a\u91ce\u6602A
\u5cb8\u672c\u5eb7\u5b8fA
\u5c0f\u6c50\u7531\u4ecbA
\u95a2\u8c37\u6d0b\u4e4bA
\u7af9\u7530\u6566A
\u4e2d\u7551\u96c5\u884cA
\u6a2a\u6fa4\u5b5d\u7ae0A
L.MartiA
\u7af9\u5185\u5eb7\u96c4B
L.LabargaC
K.BaysD
G.CarminatiD
A.RenshawD
M.SmyD
M.VaginsE
H.ZhangF
for the Super-K Collaboration<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670816\uff5e19\u65e5
\u5f18\u524d\u5927\u5b66<\/td>		\u8d85\u4f1d\u5c0e\u30d5\u30a9\u30ce\u30f3\u691c\u51fa\u5668\u306e\u958b\u767a2<\/td>\u77f3\u91ce\u5b8f\u548c
\u6a39\u6797\u6566\u5b50
\u670d\u90e8\u9999\u91cc
\u7f8e\u99ac\u899a
\u5c71\u7530\u8981\u4ecb
\u6e6f\u6d45\u6cf0\u6c17
\u7fbd\u6f84\u660c\u53f2A
\u5409\u7530\u5149\u5b8fA
\u4f50\u85e4\u4f38\u660eA
\u6e21\u8fba\u5e83\u8a18A\u3000\u4ed6\u3000KEK\u6e2c\u5b9a\u5668\u958b\u767a\u5ba4\uff1a\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668\u30b0\u30eb\u30fc\u30d7<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u79cb\u5b63\u5927\u4f1a<\/td>		9\u670816\uff5e19\u65e5
\u5f18\u524d\u5927\u5b66<\/td>		\u5b87\u5b99\u80cc\u666f\u653e\u5c04\u30ab\u30e1\u30e9\u958b\u767a\u306b\u304a\u3051\u308b\u30a2\u30eb\u30df\u8d85\u4f1d\u5c0e\u30c8\u30f3\u30cd\u30eb\u63a5\u5408\u7d20\u5b50(STJ)\u306e\u57fa\u790e\u7279\u6027\u8a55\u4fa1<\/td>\u7f8e\u99ac\u899a
\u77f3\u91ce\u5b8f\u548c
\u6a39\u6797\u6566\u5b50
\u670d\u90e8\u9999\u91cc
\u5c71\u7530\u8981\u4ecb
\u6e6f\u6d45\u6cf0\u6c17
\u7fbd\u6f84\u660c\u53f2A
\u5409\u7530\u5149\u5b8fA
\u4f50\u85e4\u4f38\u660eA
\u90fd\u4e38\u9686\u884cA
\u6e21\u8fba\u5e83\u8a18B
\u6709\u5409\u8aa0\u4e00\u90ceC
\u5927\u8c37\u77e5\u884cC
\u91ce\u53e3\u5353D
KEK\u6e2c\u5b9a\u5668\u958b\u767a\u5ba4\uff1a\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668\u30b0\u30eb\u30fc\u30d7<\/td><\/tr>
Neutrino Factories, Superbeams and Betabeams,
(NuFact11)<\/td>		August 2-6
CERN, Switzerland<\/td>		R&D of a Gd-loaded water Cherenkov
\nDetector.<\/td>		T. Mori (for the SuperK Gd project)<\/td><\/tr>
Hamburg Neutrinos
\nfrom Supernova Explosion,
(HAnSE11)<\/td>		July 19-23
DESY, Germany<\/td>		 Development of a Gd-loaded water
\nCherenkov Detector.<\/td>		M. Sakuda (for the SuperK Gd project)<\/td><\/tr>
RIBF and CNS Symposium on Frontier of gamma-ray spectroscopy
(Gamma11)<\/td>		June 30-July 2
Riken (Wako)<\/td>		Proposed experiment to measure gamma-rays from O(p,p’)O* in relation to O(nu,nu’).<\/td>M. Sakuda<\/td><\/tr>
TIPP2011<\/td>June 9-14
Chicago<\/td>		Development of Superconducting Detectors for Measurements of Cosmic Microwave Background and Other Applications.<\/td>Satoru Mima<\/td><\/tr>
TIPP2011
(poster)<\/td>		June 9-14
Chicago<\/td>		Developments of Aluminum Superconducting Tunnel Junction (STJ) detectors for millimeter wave and particle detections.<\/td>Hirokazu Ishino<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c66\u56de\u5e74\u6b21\u5927\u4f1a<\/td>		5\u67086\u65e5\uff5e8\u670831\u65e5
\u8b1b\u6f14\u8cc7\u6599\u516c\u958b\u30b5\u30a4\u30c8<\/td>		\u8d85\u4f1d\u5c0e\u30d5\u30a9\u30ce\u30f3\u691c\u51fa\u5668\u306e\u958b\u767a<\/td>\u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c66\u56de\u5e74\u6b21\u5927\u4f1a<\/td>		5\u67086\u65e5\uff5e8\u670831\u65e5
\u8b1b\u6f14\u8cc7\u6599\u516c\u958b\u30b5\u30a4\u30c8<\/td>		RCNP\u3067\u306e^16 O(p,p\u2019)\u5b9f\u9a13\u3067\u4f7f\u7528\u3059\u308b\u30ac\u30f3\u30de\u7dda\u691c\u51fa\u5668\u306e\u6027\u80fd\u8a55\u4fa1<\/td>\u6cc9\u5353\u5b8f\u3001\u68ee\u4fca\u5f70\u3001\u5c71\u53e3\u7adc\u592a\u3001\u4f5c\u7530\u8aa0\u3001\u6c11\u4e95\u6566\u3001\u9234\u6728\u667a\u548c\u3001\u571f\u5c90\u535a\u3001\u4e2d\u7551\u96c5\u884c\u3001\u4e0a\u91ce\u6602<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c66\u56de\u5e74\u6b21\u5927\u4f1a<\/td>		5\u67086\u65e5\uff5e8\u670831\u65e5
\u8b1b\u6f14\u8cc7\u6599\u516c\u958b\u30b5\u30a4\u30c8<\/td>		Super-Kamiokande Gadolinium R&D Project: Gd\u30c6\u30b9\u30c8\u5b9f\u8a3c\u65bd\u8a2d\u5efa\u8a2d\u306e\u73fe\u72b6<\/td>\u6a39\u6797\u6566\u5b50
\u77f3\u91ce\u5b8f\u548c
\u4f5c\u7530\u8aa0
\u8c4a\u7530\u82f1\u55e3
\u4e09\u91ce\u5c06\u609f
\u68ee\u4fca\u5f70
\u5c0f\u6c50\u7531\u4ecbA
\u95a2\u8c37\u6d0b\u4e4bA
\u7af9\u7530\u6566A
\u4e2d\u7551\u96c5\u884cA
\u7af9\u5185\u5eb7\u96c4B
L.LabargaC
L.MartiC
A.RenshawD
M.SmyD
M.VaginsE
for the Super-K Collaboration<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c66\u56de\u5e74\u6b21\u5927\u4f1a<\/td>		5\u67086\u65e5\uff5e8\u670831\u65e5
\u8b1b\u6f14\u8cc7\u6599\u516c\u958b\u30b5\u30a4\u30c8<\/td>		\u5b87\u5b99\u30de\u30a4\u30af\u30ed\u6ce2\u80cc\u666f\u653e\u5c04\u504f\u5149\u6e2c\u5b9a\u7528Microwave Kinetic Inductance Detectors(MKIDs) \u306b\u304a\u3051\u308b\u591a\u30c1\u30e3\u30f3\u30cd\u30eb\u8aad\u307f\u51fa\u3057\u306e\u958b\u767a<\/td>\u670d\u90e8\u9999\u91cc
\u77f3\u91ce\u5b8f\u548c
\u5c0f\u5009\u5178\u5b50
\u6a39\u6797\u6566\u5b50
\u4e09\u6fa4\u5c1a\u5178
\u7f8e\u99ac\u899a
\u4f50\u85e4\u4f38\u660eA
\u90fd\u4e38\u9686\u884cA
\u7fbd\u6f84\u660c\u53f2A
\u5409\u7530\u5149\u5b8fA
\u6e21\u8fba\u5e83\u8a18B
\u6709\u5409\u8aa0\u4e00\u90ceC
\u5927\u8c37\u77e5\u884cC\u4ed6 KEK\u6e2c\u5b9a\u5668\u958b\u767a\u5ba4\uff1a\u8d85\u4f1d\u5c0e\u30df\u30ea\u6ce2\u30ab\u30e1\u30e9\u958b\u767a\u30b0\u30eb\u30fc\u30d7<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c66\u56de\u5e74\u6b21\u5927\u4f1a<\/td>		5\u67086\u65e5\uff5e8\u670831\u65e5
\u8b1b\u6f14\u8cc7\u6599\u516c\u958b\u30b5\u30a4\u30c8<\/td>		CMB\u30ab\u30e1\u30e9\u958b\u767a\u306b\u304a\u3051\u308b\u30a2\u30eb\u30df\u8d85\u4f1d\u5c0e\u30c8\u30f3\u30cd\u30eb\u63a5\u5408\u7d20\u5b50(STJ)\u306e\u57fa\u790e\u7279\u6027\u8a55\u4fa1<\/td>\u7f8e\u99ac\u899a,\u77f3\u91ce\u5b8f\u548c,\u6a39\u6797\u6566\u5b50,\u670d\u90e8\u9999\u91cc,\u5c0f\u5009\u5178\u5b50,\u4e09\u6fa4\u5c1a\u5178,\u7fbd\u6f84\u660c\u53f2^A^,\u5409\u7530\u5149\u5b8f^A^,\u4f50\u85e4\u4f38\u660e^A^,\u90fd\u4e38\u9686\u884c^A^,\u6e21\u8fba\u5e83\u8a18^B^,\u6709\u5409\u8aa0\u4e00\u90ce^C^,\u5927\u8c37\u77e5\u884c^C^,KEK\u6e2c\u5b9a\u5668\u958b\u767a\u5ba4\uff1a\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668\u30b0\u30eb\u30fc\u30d7<\/td><\/tr>
NuInt11<\/td>March 7-11
Dehradun, India\n<\/td>		Review on gamma-ray production in NC neutrino-oxygen and -carbon interactions<\/td>M. Sakuda<\/td><\/tr>
NuInt11
(poster)<\/td>		March 7-11
Dehradun, India\n<\/td>		NC neutrino-oxygen interactions and the associated gamma-ray production <\/td>T. Mori, R.Yamaguchi, M.Sakuda<\/td><\/tr>
\u8d85\u65b0\u661f\u7814\u7a76\u4f1a2011<\/td>3\u67081-3\u65e5
\u56fd\u7acb\u5929\u6587\u53f0<\/td>		\u30b9\u30fc\u30d1\u30fc\u30ab\u30df\u30aa\u30ab\u30f3\u30c7\u3068\u8d85\u65b0\u661f\u7206\u767a\u30cb\u30e5\u30fc\u30c8\u30ea\u30ce<\/td>\u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
\u7b2c11\u56de\u3000\u5b87\u5b99\u79d1\u5b66\u30b7\u30f3\u30dd\u30b8\u30a6\u30e0
(poster) <\/td>		1\u67085\uff0d7\u65e5
JAXA \u5b87\u5b99\u79d1\u5b66\u7814\u7a76\u6240\u3000\u76f8\u6a21\u539f\u30ad\u30e3\u30f3\u30d1\u30b9<\/td>		LiteBIRD\u642d\u8f09\u7528\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668\u30ab\u30e1\u30e9\u306e\u958b\u767a<\/td>\u77f3\u91ce\u5b8f\u548c\u3001\u670d\u90e8\u9999\u91cc\u3001\u6a39\u6797\u6566\u5b50\u3001\u7f8e\u99ac\u899a\u3000\u4ed6\u8d85\u4f1d\u5c0e\u691c\u51fa\u5668\u958b\u767a\u30b0\u30eb\u30fc\u30d7<\/td><\/tr>
\u7b2c11\u56de\u3000\u5b87\u5b99\u79d1\u5b66\u30b7\u30f3\u30dd\u30b8\u30a6\u30e0
(poster) <\/td>		1\u67085\uff0d7\u65e5
JAXA \u5b87\u5b99\u79d1\u5b66\u7814\u7a76\u6240\u3000\u76f8\u6a21\u539f\u30ad\u30e3\u30f3\u30d1\u30b9<\/td>		LiteBIRD\u306b\u304a\u3051\u308b\u5168\u5929\u30b9\u30ad\u30e3\u30f3\u304a\u3088\u3073\u30c7\u30fc\u30bf\u30b5\u30a4\u30ba\u306e\u7814\u7a76<\/td>\u670d\u90e8\u9999\u91cc\u3001\u77f3\u91ce\u5b8f\u548c\u3001\u6a39\u6797\u6566\u5b50\u3001\u7f8e\u99ac\u899a\u3001\u4e09\u6fa4\u5c1a\u5178\u3000\u4ed6LiteBIRD\u30ef\u30fc\u30ad\u30f3\u30b0\u30b0\u30eb\u30fc\u30d7<\/td><\/tr><\/tbody><\/table><\/figure>\n\n\n\n

2010<\/font><\/a><\/h2>\n\n\n\n
NNN10
(poster)
<\/td>		Dec. 13-16
Toyama, Japan<\/td>		Status of the Super-Kamiokande Gd. R&D Project<\/td>Atsuko Kibayashi for the Super-Kamiokande Collaboration<\/td><\/tr>
The XII International Workshop on Neutrino Factories, Super beams and Beta beams<\/td>Oct. 20-25
Mumbai, India<\/td>		Pion production in neutrino-nucleus interaction<\/td>M.Sakuda<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u79cb\u5b63\u5927\u4f1a <\/td>		Sept. 11-14
\u4e5d\u5dde\u5de5\u696d\u5927\u5b66\uff08\u5ca1\u5317\u4e5d\u5dde\u5e02\uff09<\/td>		Super-Kamiokande Gadolinium R&D Project\uff1aGd\u30c6\u30b9\u30c8\u5b9f\u8a3c\u65bd\u8a2d\u5efa\u8a2d\u306e\u73fe\u72b6 <\/td>\u77f3\u91ce\u5b8f\u548c
\u4f5c\u7530\u8aa0, \u6a39\u6797\u6566\u5b50
\u4e09\u91ce\u5c06\u609f
\u68ee\u4fca\u5f70
\u8c4a\u7530\u82f1\u55e3
\u4ed6 the Super-Kamiokande Collaboration<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u79cb\u5b63\u5927\u4f1a <\/td>		Sept. 11-14
\u4e5d\u5dde\u5de5\u696d\u5927\u5b66\uff08\u5ca1\u5317\u4e5d\u5dde\u5e02\uff09<\/td>		Super-Kamiokande Gadolinium R&D project\uff1a\u786b\u9178Gd\u306b\u3088\u308b\u5b9f\u9a13\u88c5\u7f6e\u6750\u6599\u306b\u5bfe\u3059\u308b\u5f71\u97ff <\/td>\u8c4a\u7530\u82f1\u55e3
\u4f5c\u7530\u8aa0, \u77f3\u91ce\u5b8f\u548c
\u6a39\u6797\u6566\u5b50
\u4e09\u91ce\u5c06\u609f
\u68ee\u4fca\u5f70
\u4ed6 the Super-Kamiokande Collaboration<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u79cb\u5b63\u5927\u4f1a <\/td>		Sept. 11-14
\u4e5d\u5dde\u5de5\u696d\u5927\u5b66\uff08\u5ca1\u5317\u4e5d\u5dde\u5e02\uff09<\/td>		RCNP\u3067\u306e16O(p,p’)\u5b9f\u9a13\u306e\u30ac\u30f3\u30de\u7dda\u6e2c\u5b9a\u8a08\u753b <\/td>\u68ee\u4fca\u5f70
\u4f5c\u7530\u8aa0
\u6cc9\u5353\u5b8f
\u6c11\u4e95\u6df3A
\u571f\u5c90\u535aA
\u4e2d\u7551\u96c5\u884cB
\u4e0a\u91ce\u6602B<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u79cb\u5b63\u5927\u4f1a <\/td>		Sept. 11-14
\u4e5d\u5dde\u5de5\u696d\u5927\u5b66\uff08\u5ca1\u5317\u4e5d\u5dde\u5e02\uff09<\/td>		Super-Kamiokande Gadolinium R&D Project\uff1aGd\u30c6\u30b9\u30c8\u5b9f\u8a3c\u6a5f\u306b\u304a\u3051\u308b\u8f03\u6b63\u7528\u653e\u5c04\u7dda\u6e90\u306e\u30b7\u30df\u30e5\u30ec\u30fc\u30b7\u30e7\u30f3\u306b\u3088\u308b\u7814\u7a76 <\/td>\u4e09\u91ce\u5c06\u609f
\u4f5c\u7530\u8aa0, \u77f3\u91ce\u5b8f\u548c
\u6a39\u6797\u6566\u5b50
\u68ee\u4fca\u5f70
\u8c4a\u7530\u82f1\u55e3
\u4ed6 the Super-Kamiokande Collaboration<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u79cb\u5b63\u5927\u4f1a <\/td>		Sept. 11-14
\u4e5d\u5dde\u5de5\u696d\u5927\u5b66\uff08\u5ca1\u5317\u4e5d\u5dde\u5e02\uff09<\/td>		\u30a2\u30eb\u30df\u8d85\u4f1d\u5c0e\u30c8\u30f3\u30cd\u30eb\u63a5\u5408\u7d20\u5b50\uff08Al-STJ\uff09\u3092\u7528\u3044\u305fCMB\u504f\u5149\u30ab\u30e1\u30e9\u306e\u958b\u767a<\/td>\u7f8e\u99ac\u899a
\u77f3\u91ce\u5b8f\u548c
\u6a39\u6797\u6566\u5b50
\u670d\u90e8\u9999\u91cc
\u4ed6 KEK\u6e2c\u5b9a\u5668\u958b\u767a\u5ba4\uff1a\u8d85\u4f1d\u5c0e\u30df\u30ea\u6ce2\u30ab\u30e1\u30e9\u958b\u767a\u30b0\u30eb\u30fc\u30d7<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u79cb\u5b63\u5927\u4f1a <\/td>		Sept. 11-14
\u4e5d\u5dde\u5de5\u696d\u5927\u5b66\uff08\u5ca1\u5317\u4e5d\u5dde\u5e02\uff09<\/td>		\u5b87\u5b99\u80cc\u666f\u653e\u5c04\u504f\u5149\u7cbe\u5bc6\u6e2c\u5b9a\u5c0f\u578b\u885b\u661fLiteBIRD\u306e\u5168\u5929\u30b9\u30ad\u30e3\u30f3\u306e\u6700\u9069\u5316\u3068\u30c7\u30fc\u30bf\u30b5\u30a4\u30ba\u306e\u7814\u7a76<\/td>\u670d\u90e8\u9999\u91cc
\u77f3\u91ce\u5b8f\u548c
\u6a39\u6797\u6566\u5b50
\u7f8e\u99ac\u899a
\u4e09\u6fa4\u5c1a\u5178, \u4ed6LiteBIRD\u30ef\u30fc\u30ad\u30f3\u30b0\u30b0\u30eb\u30fc\u30d7<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u79cb\u5b63\u5927\u4f1a <\/td>		Sept. 11-14
\u4e5d\u5dde\u5de5\u696d\u5927\u5b66\uff08\u5ca1\u5317\u4e5d\u5dde\u5e02\uff09<\/td>		\u5c0f\u578b\u79d1\u5b66\u885b\u661fLiteBIRD\u306e\u30c7\u30fc\u30bf\u53ce\u96c6\u30b7\u30b9\u30c6\u30e0\u306e\u958b\u767a(1)<\/td>\u4e09\u6fa4\u5c1a\u5178
\u77f3\u91ce\u5b8f\u548c
\u670d\u90e8\u9999\u91cc
\u4ed6LiteBIRD \u30ef\u30fc\u30ad\u30f3\u30b0\u30b0\u30eb\u30fc\u30d7<\/td><\/tr>
The XXIV International Conference on Neutrino Physics and Astrophysics
(poster)<\/td>		Jun. 14-19
Athens, Greece<\/td>		Proposed experiment to measure g-rays in high resolution experiment O(p,p\u2019) and O(3He,t), and the g-rays production in neutral current neutrino-oxygen interaction\n<\/td>T.Mori,T.Izumi,M.Sakuda,
T.Suzuki,A.Tamii,H.Toki,
M.Nakahata,K.Ueno

<\/td><\/tr>
CMB\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d72010<\/td>Jun. 7-10
\u56fd\u7acb\u5929\u6587\u53f0\u4e09\u9df9\u30ad\u30e3\u30f3\u30d1\u30b9<\/td>		\u5c0f\u578b\u79d1\u5b66\u885b\u661fLiteBIRD\u306e\u5168\u5929\u30b9\u30ad\u30e3\u30f3\u306e\u6700\u9069\u5316\u3068\u30c7\u30fc\u30bf\u30b5\u30a4\u30ba\u306e\u7814\u7a76<\/td>\u670d\u90e8\u9999\u91cc
\u77f3\u91ce\u5b8f\u548c
\u6a39\u6797\u6566\u5b50
\u7f8e\u99ac\u899a
\u4ed6\u3000LiteBIRD\u30ef\u30fc\u30ad\u30f3\u30b0\u30b0\u30eb\u30fc\u30d7<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c65\u4f1a\u5e74\u6b21\u5927\u4f1a <\/td>		Mar. 20-23
\u5ca1\u5c71\u5927\u5b66\uff08\u5ca1\u5c71\uff09<\/td>		\u30a2\u30eb\u30df\u8d85\u4f1d\u5c0e\u30c8\u30f3\u30cd\u30eb\u63a5\u5408\u7d20\u5b50(Al-STJ)\u3092\u7528\u3044\u305fCMB\u504f\u5149\u30ab\u30e1\u30e9\u306e\u958b\u767a\uff0d\u30df\u30ea\u6ce2\u306b\u5bfe\u3059\u308b\u611f\u5ea6\u8a66\u9a13\uff0d <\/td>\u7f8e\u99ac\u899a
\u77f3\u91ce\u5b8f\u548c
\u6a39\u6797\u6566\u5b50
\u4ed6\u3000\u8d85\u4f1d\u5c0e\u30df\u30ea\u6ce2\u30ab\u30e1\u30e9\u958b\u767a\u30b0\u30eb\u30fc\u30d7<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c65\u4f1a\u5e74\u6b21\u5927\u4f1a <\/td>		Mar. 20-23
\u5ca1\u5c71\u5927\u5b66\uff08\u5ca1\u5c71\uff09<\/td>		200MeV\u304b\u30891000MeV\u9818\u57df\u3067\u306e\u96fb\u5b50\u539f\u5b50\u6838\u6e96\u5f3e\u6027\u6563\u4e71\u53ca\u3073\u30d1\u30a4\u751f\u6210\u53cd\u5fdc\u306e\u7814\u7a76 <\/td>\u68ee\u4fca\u5f70
\u4f5c\u7530\u8aa0
\u5c0f\u91ce\u54f2\u4e5f<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c65\u4f1a\u5e74\u6b21\u5927\u4f1a <\/td>		Mar. 20-23
\u5ca1\u5c71\u5927\u5b66\uff08\u5ca1\u5c71\uff09<\/td>		Super-Kamiokande Gadolinium R&D Project\uff1aGd\u30c6\u30b9\u30c8\u5b9f\u8a3c\u5668\u306e\u6821\u6b63\u7528\u653e\u5c04\u7dda\u6e90\u306e\u30c7\u30b6\u30a4\u30f3 <\/td>\u4e09\u91ce\u5c06\u609f
\u77f3\u91ce\u5b8f\u548c
\u6a39\u6797\u6566\u5b50
\u8c4a\u7530\u82f1\u55e3, \u68ee\u4fca\u5f70, \u4f5c\u7530\u8aa0\u4ed6 the Super-Kamiokande Collaboration<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c65\u4f1a\u5e74\u6b21\u5927\u4f1a <\/td>		Mar. 20-23
\u5ca1\u5c71\u5927\u5b66\uff08\u5ca1\u5c71\uff09<\/td>		Super-Kamiokande Gadolinium R&D project\uff1a\u5b9f\u9a13\u88c5\u7f6e\u6750\u6599\u306b\u5bfe\u3059\u308b\u5f71\u97ff <\/td>\u8c4a\u7530\u82f1\u55e3
\u77f3\u91ce\u5b8f\u548c
\u6a39\u6797\u6566\u5b50
\u4e09\u91ce\u5c06\u609f, \u68ee\u4fca\u5f70, \u4f5c\u7530\u8aa0\u4ed6 the Super-Kamiokande Collaboration<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c65\u4f1a\u5e74\u6b21\u5927\u4f1a <\/td>		Mar. 20-23
\u5ca1\u5c71\u5927\u5b66\uff08\u5ca1\u5c71\uff09<\/td>		BS\u30a2\u30f3\u30c6\u30ca\u3092\u7528\u3044\u305f\u5b87\u5b99\u80cc\u666f\u653e\u5c04\u306e\u89b3\u6e2c\u5b9f\u7fd2 <\/td>\u5c0f\u5009\u5178\u5b50
\u77f3\u91ce\u5b8f\u548c
\u6a39\u6797\u6566\u5b50
\u7f8e\u99ac\u899a
\u4e09\u6fa4\u5c1a\u5178
\u4ed6<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c65\u4f1a\u5e74\u6b21\u5927\u4f1a <\/td>		Mar. 20-23
\u5ca1\u5c71\u5927\u5b66\uff08\u5ca1\u5c71\uff09<\/td>		\u5b87\u5b99\u7dda\u30fb\u5b87\u5b99\u7269\u7406\u9818\u57df
\u7d20\u7c92\u5b50\u8ad6\u9818\u57df\u5408\u540c\u30b7\u30f3\u30dd\u30b8\u30a6\u30e0
\n\u4e3b\u984c\uff1a\u5b87\u5b99\u80cc\u666f\u653e\u5c04\u306e\u504f\u5149\u304b\u3089\u3055\u3050\u308b\u521d\u671f\u5b87\u5b99\u3068\u8d85\u9ad8\u30a8\u30cd\u30eb\u30ae\u30fc\u7269\u7406\u3000\u300c\u306f\u3058\u3081\u306b\u300d <\/td>		\u77f3\u91ce\u5b8f\u548c<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\u7b2c65\u4f1a\u5e74\u6b21\u5927\u4f1a <\/td>		Mar. 20-23
\u5ca1\u5c71\u5927\u5b66\uff08\u5ca1\u5c71\uff09<\/td>		\u5168\u56fd\u5b66\u90e8\u751f\u306b\u3088\u308b\u7b2c\u4e00\u56de\u6570\u7269\u30bb\u30df\u30ca\u30fc\u5b9f\u65bd\u5831\u544a <\/td>\u4e95\u4e0a\u512a\u8cb4,\u91d1\u5ddd\u6d69\u5e73,\u4f5c\u7530\u8aa0,\u5473\u91ce\u9053\u4fe1,\u4ed6<\/td><\/tr>
The 10th International Symposium on Origin of Matter and Evolution of the
\nGalaxies <\/td>		Mar. 8-10, Osaka (Japan)<\/td>Study of gamma-ray production from neutrino-Oxygen interaction and the detection of the neutrino from Supernova explosion. <\/td>T.Mori*, M.Sakuda, A.Tamii,H.Toki(RCNP),
M.Nakahata,
K.Ueno(ICRR)<\/td><\/tr>
International Symposium on New Facet of Spin-Isospin Responses <\/td>Feb. 19-21, Tokyo (Japan)<\/td>Study of neutrino-Oxygen cross section including gamma production for the detection of neutrinos from Supernova explosion <\/td>T.Mori*, M\/Sakuda<\/td><\/tr>
International Symposium on New Facet of Spin-Isospin Responses <\/td>Feb. 19-21, Tokyo (Japan)<\/td>Study of gamma-ray production in neutrino-Oxygen interactions and the relavance to the detection of neutrinos from Supernova<\/td> M.Sakuda*, T.Mori <\/td><\/tr><\/tbody><\/table><\/figure>\n\n\n\n

2009<\/font><\/a><\/h2>\n\n\n\n
\u6771\u4eac\u5927\u5b66\u5b87\u5b99\u7dda\u7814\u7a76\u6240
\n \u5171\u540c\u5229\u7528\u8005\u4f1a\u8b70<\/td>		12\u670819\u65e5
\n \u5343\u8449\u770c\u67cf\u5e02<\/td>		\u30b9\u30fc\u30d1\u30fc\u30ab\u30df\u30aa\u30ab\u30f3\u30c7<\/td>Hirokazu Ishino<\/td><\/tr>
Asia-Pacific Geant4 Workshop and Training Course<\/td>Dec. 7-12,
\n Tsukuba (Japan)<\/td>		Super-Kamiokande Gadolinium R&D Project: Status of test tank simulation<\/td>Atsuko Kibayashi<\/td><\/tr>
Asia-Pacific Geant4 Workshop and Training Course<\/td>Dec. 7-12,
\n Tsukuba (Japan) <\/td>		Questions from a beginner developing a Gd-loaded water Cherenkov detector simulation<\/td>Shogo Mino<\/td><\/tr>
\u79cb\u5b63\u4f4e\u6e29\u5de5\u5b66\u30fb\u8d85\u96fb\u5c0e\u5b66\u4f1a  <\/td>11\u670818\uff0d20\u65e5
\n \u5ca1\u5c71\u5927\u5b66\uff08\u5ca1\u5c71) <\/td>		\u30a2\u30f3\u30c6\u30ca\u7d50\u5408\u30a2\u30eb\u30df\u8d85\u4f1d\u5c0e\u30c8\u30f3\u30cd\u30eb\u63a5\u5408\u7d20\u5b50(Al-STJ)\u3092\u7528\u3044\u305f\uff23\uff2d\uff22\u504f\u5149\u691c\u51fa\u5668\u306e\u958b \u767a<\/td>\u7f8e\u99ac\u899a\u3001\u77f3\u91ce\u5b8f\u548c\u3000\u4ed6 STJ group<\/td><\/tr>
TOURS Symposium on Nuclear Physics and Astrophysics VII<\/td>Nov.16-20, Kobe (Japan)<\/td>Development of a Gd-loaded water Cherenkov detector capable of tagging neutrons<\/td>Makoto Sakuda<\/td><\/tr>
KEK theory center workshop on Short-range correlations and tensor structure at J-PARC<\/td>Sept. 25, Tsukuba (Japan)<\/td>Effect of spectral function in neutrino-nucleus interactions in the MeV-GeV region: Experimental View<\/td>Makoto Sakuda<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a\u3000
\n \u79cb\u5b63\u5927\u4f1a <\/td>		9\u670810\uff0d13\u65e5
\n \u7532\u5357\u5927\u5b66\uff08\u795e\u6238\uff09<\/td>		CMB\u30ab\u30e1\u30e9\u958b\u767a\u306b\u304a\u3051\u308b\u30a2\u30eb\u30df\u8d85\u4f1d\u5c0e\u30c8\u30f3\u30cd\u30eb\u63a5\u5408\u7d20\u5b50(STJ)\u306e\u57fa\u790e\u7279\u6027\u8a55\u4fa1<\/td>\u7f8e\u99ac\u899a\u3001\u77f3\u91ce\u5b8f\u548c\u3000\u4ed6 STJ group <\/td><\/tr>
Meeting of the Division of Particles and Fields of the American Physical Society<\/td>July 26-31,
\n Detroit (USA)<\/td>		Gadolinium study for a water Cherenkov detector<\/td>Atsuko Kibayashi<\/td><\/tr>
31st International Cosmic Ray Conference<\/td>14th, July
\n Lodz (Poland)<\/td>		Gadolinium Study for Super-Kamiokande<\/td>Hirokazu Ishino<\/td><\/tr>
\u7b2c64\u56de\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\n \u5e74\u6b21\u5927\u4f1a<\/td>		3\u670827\uff0d30\u65e5\u3001
\n \u7acb\u6559\u5927\u5b66\uff08\u6771\u4eac\uff09<\/td>		CMB\u30ab\u30e1\u30e9\u958b\u767a\u306b\u304a\u3051\u308b\u30a2\u30eb\u30df\u8d85\u4f1d\u5c0e\u30c8\u30f3\u30cd\u30eb\u7d50\u5408\u7d20\u5b50(STJ)\u306e\u57fa\u790e\u7279\u6027\u8a55\u4fa1 <\/td>\u7f8e\u99ac\u899a\u3001\u77f3\u91ce\u5b8f\u548c\u3000\u4ed6 STJ group <\/td><\/tr>
Technology and Instrument in Particle Physics 2009<\/td>Mar. 12-17, Tsukuba (Japan)<\/td>Development of an Antenna-coupled Al Superconducting Tunnel Junction for a detection of cosmic microwave background B-mode polarization (poster presentation) <\/td>Hirokazu Ishino et al. (STJ group) <\/td><\/tr><\/tbody><\/table><\/figure>\n\n\n\n

2008<\/font><\/a><\/h2>\n\n\n\n
13th Geant4 Collaboration Workshop <\/td>October 6-11, Kobe (Japan)<\/td>Simulation for Gadolinium dissolved Water Cerenkov Detector<\/td>A.Kibayashi, H.Ishino, Y.Koshio, M.Nakahata,H.Sekiya, M.Smy, M.Vagins <\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a
\n \u79cb\u5b63\u5927\u4f1a <\/td>		9\u670820-23\u65e5
\n \u5c71\u5f62\u5927\u5b66(\u5c71\u5f62) <\/td>		\uff23\uff2d\uff22\u30ab\u30e1\u30e9\u958b\u767a\u306b\u304a\u3051\u308b\u30a2\u30eb\u30df\u8d85\u4f1d\u5c0e\u30c8\u30f3\u30cd\u30eb\u7d50\u5408\u7d20\u5b50\uff08\uff33\uff34\uff2a)\u306e\u57fa\u790e\u7279\u88fd\u8a55\u4fa1 <\/td>\u7f8e\u99ac\u899a
\u77f3\u91ce\u5b8f\u548c
\u6a39\u6797\u6566\u5b50
\u7fbd\u6f84\u660c\u53f2
\u4f4f\u6fa4\u4e00\u9ad8
\u6a0b\u53e3\u5cb3\u96c4
\u5409\u7530\u5149\u5b8f
\u7530\u5cf6\u6cbb
\u4f50\u85e4\u5e83\u6d77 <\/td><\/tr><\/tbody><\/table><\/figure>\n\n\n\n

2007<\/font><\/a><\/h2>\n\n\n\n
Neutrino Workshop<\/td>May 3-5, Jefferson Lab(USA)<\/td>Importance of low Q2  region  in neutrino-nucleus interactions<\/td>Makoto Sakuda<\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a 2006\u5e74\u6625\u5b63\u5927\u4f1a<\/td>3\u670827\u65e5-30\u65e5 \u611b\u5a9b\u5927\u5b66(\u611b\u5a9b\uff09<\/td>\u30b9\u30fc\u30d1\u30fc\u30ab\u30df\u30aa\u30ab\u30f3\u30c7 III\u3000\u306b\u304a\u3051\u308b\u5149\u96fb\u5b50\u5897\u500d\u7ba1\u306e\u5fdc\u7b54\u6642\u9593\u88dc\u6b63\u306e\u6539\u826f<\/td>\u6c60\u7530\u4e00\u5f97\u3001\u51fa\u539f\u7531\u898f\u3001\u6749\u539f\u771f\u592e\u3001\u4f5c\u7530\u8aa0\u4ed6\u3001SK \u8f03\u6b63\u30b0\u30eb\u30fc\u30d7 <\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a 2006\u5e74\u6625\u5b63\u5927\u4f1a<\/td>3\u670827\u65e5-30\u65e5 \u611b\u5a9b\u5927\u5b66(\u611b\u5a9b\uff09<\/td>\u30b9\u30fc\u30d1\u30fc\u30ab\u30df\u30aa\u30ab\u30f3\u30c7III\u306b\u304a\u3051\u308b20\u30a4\u30f3\u30c1\u5149\u96fb\u5b50\u5897\u500d\u7ba1\u306e\u7cbe\u5bc6\u30b2\u30a4\u30f3\u6e2c\u5b9a <\/td>\u6749\u539f\u771f\u592e\u3001\u6c60\u7530\u4e00\u5f97\u3001\u51fa\u539f\u7531\u898f\u3001\u4f5c\u7530\u8aa0\u4ed6\u3001SK \u8f03\u6b63\u30b0\u30eb\u30fc\u30d7 <\/td><\/tr>
\u65e5\u672c\u7269\u7406\u5b66\u4f1a 2006\u5e74\u6625\u5b63\u5927\u4f1a<\/td>3\u670827\u65e5-30\u65e5 \u611b\u5a9b\u5927\u5b66(\u611b\u5a9b\uff09<\/td>\u30b9\u30fc\u30d1\u30fc\u30ab\u30df\u30aa\u30ab\u30f3\u30c7\u306b\u304a\u3051\u308b\u8fd1\u508d\u9280\u6cb3\u8d85\u65b0\u661f\u7206\u767a\u8d77\u6e90\u30cb\u30e5\u30fc\u30c8\u30ea\u30ce\u30d0\u30fc\u30b9\u30c8\u63a2\u7d22 <\/td>\u6c60\u7530\u4e00\u5f97\u3001\u51fa\u539f\u7531\u898f\u3001\u6749\u539f\u771f\u592e\u3001\u4f5c\u7530\u8aa0\u4ed6\u3001 SK \u5b9f\u9a13\u30b0\u30eb\u30fc\u30d7 <\/td><\/tr><\/tbody><\/table><\/figure>\n","protected":false},"excerpt":{"rendered":"

2025 Second International Conference on the Physics of the Two Infinities 11\u670817\u65e5 – 11\u670821\u65e5Koshiba Hall Ho … <\/p>\n

“\u5b66\u4f1a\u767a\u8868” \u306e<\/span>\u7d9a\u304d\u3092\u8aad\u3080<\/a><\/p>\n","protected":false},"author":1,"featured_media":0,"parent":42,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"_locale":"ja","_original_post":"https:\/\/www.physics.okayama-u.ac.jp\/ishino-lab\/details\/wordpress\/product\/web\/?page_id=147","footnotes":""},"class_list":["post-147","page","type-page","status-publish","hentry","ja"],"aioseo_notices":[],"_links":{"self":[{"href":"https:\/\/www.physics.okayama-u.ac.jp\/ishino-lab\/details\/wordpress\/product\/web\/wp-json\/wp\/v2\/pages\/147","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.physics.okayama-u.ac.jp\/ishino-lab\/details\/wordpress\/product\/web\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/www.physics.okayama-u.ac.jp\/ishino-lab\/details\/wordpress\/product\/web\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/www.physics.okayama-u.ac.jp\/ishino-lab\/details\/wordpress\/product\/web\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/www.physics.okayama-u.ac.jp\/ishino-lab\/details\/wordpress\/product\/web\/wp-json\/wp\/v2\/comments?post=147"}],"version-history":[{"count":26,"href":"https:\/\/www.physics.okayama-u.ac.jp\/ishino-lab\/details\/wordpress\/product\/web\/wp-json\/wp\/v2\/pages\/147\/revisions"}],"predecessor-version":[{"id":3236,"href":"https:\/\/www.physics.okayama-u.ac.jp\/ishino-lab\/details\/wordpress\/product\/web\/wp-json\/wp\/v2\/pages\/147\/revisions\/3236"}],"up":[{"embeddable":true,"href":"https:\/\/www.physics.okayama-u.ac.jp\/ishino-lab\/details\/wordpress\/product\/web\/wp-json\/wp\/v2\/pages\/42"}],"wp:attachment":[{"href":"https:\/\/www.physics.okayama-u.ac.jp\/ishino-lab\/details\/wordpress\/product\/web\/wp-json\/wp\/v2\/media?parent=147"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}