{"id":1075,"date":"2018-02-02T15:54:30","date_gmt":"2018-02-02T06:54:30","guid":{"rendered":"http:\/\/core-u.hiroshima-u.ac.jp\/?page_id=1075"},"modified":"2018-02-02T15:54:30","modified_gmt":"2018-02-02T06:54:30","slug":"1075-2","status":"publish","type":"page","link":"https:\/\/core-u.hiroshima-u.ac.jp\/en\/1075-2.html","title":{"rendered":""},"content":{"rendered":"<p style=\"text-align: center;\">[<a href=\"#publications_H26\">\u8ad6\u6587 Publications<\/a>] [<a href=\"#presentations_H26\">\u5b66\u4f1a\u30fb\u7814\u7a76\u4f1a\u767a\u8868 Presentations<\/a>] [<a href=\"#events_H26\">Core-U\u30a4\u30d9\u30f3\u30c8 Core-U Events<\/a>]<\/p>\n<p><a id=\"publications_H26\"><\/a><\/p>\n<h2>\u8ad6\u6587 Publications<\/h2>\n<ul style=\"list-style-type: disc;\">\n<li>Y.T.Tanaka, <span class=\"underline\">Y.Fukazawa<\/span>(11\u756a\u76ee), \u4ed610\u540d, &ldquo;Extreme Blazars Studied with Fermi-LAT and Suzaku: 1ES 0347-121 andBlazar Candidate HESS J1943+213,&rdquo; <em>ApJ<\/em>, <strong>787<\/strong>(2014) 155.<\/li>\n<li>T.-D.Brandt, <span class=\"underline\">S.Miyama<\/span>(38\u756a\u76ee), \u4ed653\u540d, &ldquo;The Moving Group Targets of the SEEDS High-contrast Imaging Survey ofExoplanets and Disks: Results and Observations from the First ThreeYears,&rdquo; <em>ApJ<\/em>, <strong>786<\/strong> (2014) 1.<\/li>\n<li>E.S.Waker, <span class=\"underline\">M.Ohno<\/span>(22\u756a\u76ee), \u4ed624\u540d, &ldquo;Optical follow-up observations of PTF10qts, a luminous broad-linedType Ic supernova found by the Palomar Transient Factory,&rdquo; <em>MNRAS<\/em>, <strong>442<\/strong> (2014) 2768.<\/li>\n<li>M.Serino, <span class=\"underline\">M.Ohno<\/span>(5\u756a\u76ee), \u4ed642\u540d, &ldquo;MAXIobservations of gamma-ray bursts,&rdquo; <em>PASJ<\/em> <strong>66<\/strong>(2014) 87.<\/li>\n<li>N.Okabe, <span class=\"underline\">Y.Fukazawa<\/span>(9\u756a\u76ee), \u4ed617\u540d, &ldquo;Universal profiles of the intracluster medium from Suzaku X-ray andSubaru weak-lensing observations,&rdquo; <em>PASJ<\/em>, <strong>66<\/strong>(2014) 99.<\/li>\n<li>Y.Hanabata, <span class=\"underline\">Y.Fukazawa<\/span>(5\u756a\u76ee), \u4ed610\u540d, &ldquo;Detailed Investigation of the Gamma-Ray Emission in the Vicinity ofSNR W28 with FERMI-LAT,&rdquo; <em>ApJ<\/em>, <strong>786<\/strong> (2014) 145.<\/li>\n<li>E.Rivers, A.Markowitz, R.Rothschild, A.Bamba, <span class=\"underline\">Y.Fukazawa<\/span>, T.Okajima, J.Reeves, Y.Terashima, andY.Ueda, &ldquo;Tracking the Complex Absorption in NGC 2110 with Two SuzakuObservations,&rdquo; <em>ApJ<\/em>, <strong>786<\/strong> (2014) 126.<\/li>\n<li>K.Maeda, S.Katsuda, A.Bamba, Y.Terada, <span class=\"underline\">Y.Fukazawa<\/span>, &ldquo;Long-lasting X-Ray Emission from TypeIIb Supernova 2011dh and Mass-loss History of the Yellow SupergiantProgenitor,&rdquo; <em>ApJ<\/em>, <strong>785<\/strong> (2014) 95.<\/li>\n<li>T.Tamura, <span class=\"underline\">Y.Fukazawa<\/span>(4\u756a\u76ee), \u4ed69\u540d, &ldquo;GasBulk Motion in the Perseus Cluster Measured with Suzaku,&rdquo; <em>ApJ<\/em>,<strong>782<\/strong> (2014) 38.<\/li>\n<li>T.Morokuma, R.Itoh(30\u756a\u76ee), <span class=\"underline\">K.S.Kawabata<\/span>(32\u756a\u76ee), \u4ed656\u540d, &ldquo;Kiso Supernova Survey(KISS): Survey strategy,&rdquo; <em>PASJ<\/em>, <strong>66<\/strong> (2014)11416.<\/li>\n<li>R.Itoh, Y.T.Tanaka, H.Akitaya, <span class=\"underline\">M.Uemura<\/span>(4\u756a\u76ee), <span class=\"underline\">Y.Fukazawa<\/span>(5\u756a\u76ee), <span class=\"underline\">M.Yoshida<\/span>(38\u756a\u76ee), \u4ed632\u540d, &ldquo;Variable optical polarizationduring high state in gamma-ray loud, narrow-line Seyfert 1 galaxy 1H0323+342,&rdquo; <em>PASJ<\/em>, <strong>66<\/strong> (2014) 1088.<\/li>\n<li><span class=\"underline\">K.S.Kawabata<\/span>(1\u756a\u76ee), H.Akitaya,R.Itoh, <span class=\"underline\">M.Yoshida<\/span>(32\u756a\u76ee), <span class=\"underline\">Y.Fukazawa<\/span>(35\u756a\u76ee) \u4ed644\u540d, &ldquo;Optical and Near-infraredPolarimetry of Highly Reddened Type Ia Supernova 2014J: PeculiarProperties of Dust in M82,&rdquo; <em>ApJ<\/em>, <strong>795<\/strong> (2014) L4.<\/li>\n<li>M.Tanaka(1\u756a\u76ee), R.Itoh, H.Akitaya, Y.T.Tanaka, <span class=\"underline\">K.S.Kawabata<\/span>(18\u756a\u76ee), \u4ed653\u540d, &ldquo;Discovery of DramaticOptical Variability in SDSS J1100+4421: A Peculiar Radio-loudNarrow-line Seyfert 1 Galaxy?,&rdquo; <em>ApJ<\/em>, <strong>793<\/strong>(2014) L26.<\/li>\n<li>K.V.Sokolovsky, Y.T.Tanaka, <span class=\"underline\">Y.Fukazawa<\/span>(17\u756a\u76ee), R.Itoh, <span class=\"underline\">K.S.Kawabata<\/span>(22\u756a\u76ee) \u4ed647\u540d, &ldquo;Two active states of thenarrow-line gamma-ray-loud AGN GB 1310+487,&rdquo; <em>Astronomy &amp;Astrophysics<\/em>, <strong>565<\/strong> (2014) A26.<\/li>\n<li>M.Sasada, <span class=\"underline\">M.Uemura<\/span>(2\u756a\u76ee),<span class=\"underline\">Y.Fukazawa(<\/span>3\u756a\u76ee), R.Itoh(5\u756a\u76ee), <span class=\"underline\">M.Yoshida<\/span>(8\u756a\u76ee), <span class=\"underline\">K.S.Kawabata(<\/span>9\u756a\u76ee), H.Akitaya \u4ed612\u540d, &ldquo;Extremely High Polarization in the 2010Outburst of Blazar 3C 454.3,&rdquo; <em>ApJ<\/em>, <strong>784<\/strong> (2014)141.<\/li>\n<li>Y.T.Tanaka, A.Doi, Y.Inoue, C.C.Cheung, L.Stawarz, <span class=\"underline\">Y.Fukazawa,<\/span> M.A.Gurwell, M.Tahara, J.Kataoka, andR.Itoh, &ldquo;Six Years of Fermi-LAT and Multi-Wavelength Monitoring of theBroad-Line Radio Galaxy 3c 120: Jet Dissipation At Sub-Parsec Scalesfrom the Central Engine,&rdquo; <em>ApJ<\/em>, <strong>799<\/strong> (2014)L18.<\/li>\n<li>M.Ajello, <span class=\"underline\">Y.Fukazawa<\/span>(41\u756a\u76ee),<span class=\"underline\">T.Mizuno<\/span>(83\u756a\u76ee), <span class=\"underline\">M.Ohno<\/span>(94\u756a\u76ee), T.Ohsugi, <span class=\"underline\">H.Takahashi<\/span>(119\u756a\u76ee), \u4ed6130\u540d, &ldquo;Impulsive and LongDuration High-energy Gamma-Ray Emission from the Very Bright 2012 March 7Solar Flares,&rdquo; <em>ApJ<\/em>, <strong>789<\/strong> (2014) 20.<\/li>\n<li>M.Ackermann, <span class=\"underline\">T.Mizuno<\/span>(78\u756a\u76ee),T.Ohsugi(85\u756a\u76ee), <span class=\"underline\">H.Takahashi<\/span>(109\u756a\u76ee), \u4ed6123\u540d, &ldquo;Search for Cosmic-Ray-induced Gamma-Ray Emission in Galaxy Clusters,&rdquo; <em>ApJ<\/em>, <strong>787<\/strong> (2014) 18.<\/li>\n<li>M.Ackermann, <span class=\"underline\">Y.Fukazawa(<\/span>39\u756a\u76ee),<span class=\"underline\">T.Mizuno<\/span>(69\u756a\u76ee), T.Ohsugi, <span class=\"underline\">H.Takahashi<\/span> (95\u756a\u76ee), \u4ed6286\u540d, &ldquo;Multifrequency Studies ofthe Peculiar Quasar 4C +21.35 during the 2010 Flaring Activity,&rdquo; <em>ApJ<\/em>, <strong>786<\/strong> (2014) 157.<\/li>\n<li>M.Ackermann, <span class=\"underline\">Y.Fukazawa<\/span>(48\u756a\u76ee),<span class=\"underline\">T.Mizuno<\/span>(89\u756a\u76ee), <span class=\"underline\">M.Ohno<\/span>(100\u756a\u76ee), T.Ohsugi, <span class=\"underline\">H.Takahashi<\/span> (126\u756a\u76ee), Y.Tanaka, \u4ed6140\u540d, &ldquo;High-energyGamma-Ray Emission from Solar Flares: Summary of Fermi Large AreaTelescope Detections and Analysis of Two M-class Flares,&rdquo; <em>ApJ<\/em>,<strong>787<\/strong> (2014) 15.<\/li>\n<li>M.Ackermann, <span class=\"underline\">Y.Fukazawa<\/span>(49\u756a\u76ee),<span class=\"underline\">T.Mizuno<\/span>(96\u756a\u76ee), T.Ohsugi, <span class=\"underline\">H.Takahashi<\/span> (132\u756a\u76ee) \u4ed6148\u540d, &ldquo;Inferred cosmic-rayspectrum from Fermi-LAT gamma-ray observations of the Earth's limb,&rdquo; <em>Physical Review Letters<\/em>, <strong>112<\/strong> (2014) 1103.<\/li>\n<li>M.Ackermann, <span class=\"underline\">Y.Fukazawa<\/span>(40\u756a\u76ee),<span class=\"underline\">T.Mizuno<\/span>(73\u756a\u76ee), T.Ohsugi, <span class=\"underline\">H.Takahashi<\/span>(102\u756a\u76ee), \u4ed6117\u540d, &ldquo;Dark matter constraintsfrom observations of 25 MilkyA Way satellite galaxies with the FermiLarge Area Telescope,&rdquo; <em>Physical Review<\/em> D<strong>89<\/strong>(2014) 042001.<\/li>\n<li>Y.Inoue, <span class=\"underline\">Y.T.Tanaka<\/span>, G.Madejski,A.Dominguez, &ldquo;Upper Bound on the First Star Formation History,&rdquo; <em>TheAstrophysical Journal Letters<\/em>, <strong>781<\/strong> (2014) L35.<\/li>\n<li>R.Preece, <span class=\"underline\">Y.Fukazawa<\/span>(72\u756a\u76ee),<span class=\"underline\">T.Mizuno<\/span>(105\u756a\u76ee), <span class=\"underline\">M.Ohno<\/span>(103\u756a\u76ee), T.Ohsugi, <span class=\"underline\">H.Takahashi<\/span> (143\u756a\u76ee), \u4ed6153\u540d, &ldquo;The First Pulse of theExtremely Bright GRB 130427A: A Test Lab for Synchrotron Shocks,&rdquo; <em>Science<\/em>, <strong>343<\/strong> (2014) 51.<\/li>\n<li><span class=\"underline\">Y.Utsumi<\/span>, S.Miyazaki, M.J.Geller,I.P.Dell'Antonio, M.Oguri, M.J.Kurtz, T.Hamana, and D.G.Fabricant, &ldquo;Reducing Systematic Error in Weak Lensing Cluster Surveys,&rdquo; <em>ApJ<\/em>, <strong>786<\/strong> (2014) 93.<\/li>\n<li>M.Ackermann, <span class=\"underline\">Y.Fukazawa<\/span>(58\u756a\u76ee),<span class=\"underline\">T.Mizuno<\/span>(101\u756a\u76ee), <span class=\"underline\">M.Ohno<\/span>(110\u756a\u76ee), T.Ohsugi, <span class=\"underline\">H.Takahashi<\/span>(144\u756a\u76ee), \u4ed6176\u540d, &ldquo;Fermi-LAT Observations ofthe Gamma-Ray Burst GRB 130427A,&rdquo; <em>Science<\/em>, <strong>343<\/strong>(2014) 42.<\/li>\n<li>M.Ackermann, <span class=\"underline\">Y.Fukazawa<\/span>(45\u756a\u76ee),<span class=\"underline\">T.Mizuno<\/span>(86\u756a\u76ee), <span class=\"underline\">H.Takahashi<\/span>(122\u756a\u76ee) \u4ed6 131\u540d, &ldquo;The Spectrum andMorphology of the Fermi Bubbles,&rdquo; <em>ApJ<\/em>, <strong>793<\/strong>(2014) 64.<\/li>\n<li>M.Ackermann, <span class=\"underline\">Y.Fukazawa<\/span>(50\u756a\u76ee),<span class=\"underline\">T.Mizuno<\/span>(94\u756a\u76ee), <span class=\"underline\">H.Takahashi<\/span>(128\u756a\u76ee) \u4ed6149\u540d, &ldquo;Fermi Establishes ClassicalNovae as a Distinct Class of Gamma-Ray Sources,&rdquo; <em>Science<\/em>,<strong>345<\/strong> (2014) 554.<\/li>\n<li>Y.T.Tanaka, <span class=\"underline\">Y.Fukazawa<\/span>(11\u756a\u76ee) \u4ed610\u540d, &ldquo;Extreme Blazars Studied with Fermi-LAT and Suzaku: 1ES 0347-121 andBlazar Candidate HESS J1943+213,&rdquo; <em>ApJ<\/em>, <strong>787<\/strong>(2014) 155.<\/li>\n<li>K.Hamaguchi, M.Corcoran, <span class=\"underline\">H.Takahashi,<\/span> T.Yuasa, M.Ishida, T.R.Gull,J.M.Pittard, M.P.Russell, T.I.Madura, &ldquo;Suzaku Monitoring of Hard X-RayEmission from eta Carinae over a Single Binary Orbital Cycle,&rdquo; <em>ApJ<\/em>, <strong>795<\/strong> (2014) 119.<\/li>\n<li><span class=\"underline\">M.Ohno<\/span>(1\u756a\u76ee), <span class=\"underline\">H.Takahashi<\/span>(6\u756a\u76ee), <span class=\"underline\">Y.Fukazawa<\/span>(8\u756a\u76ee), \u4ed632\u540d, &ldquo;Development and verificationof signal processing system of BGO active shield onboard Astro-H,&rdquo; Proc.SPIE 9144, 91445G, (2014).<\/li>\n<li>H.Noda, <span class=\"underline\">M.Ohno<\/span>(12\u756a\u76ee), <span class=\"underline\">Y.Fukazawa<\/span>(13\u756a\u76ee), \u4ed615\u540d, &ldquo;Thermal design of the hardx-ray imager and the soft gamma-ray detector onboard ASTRO-H,&rdquo; SPIE 9144,91445E, (2014).<\/li>\n<li><span class=\"underline\">Y.Fukazawa<\/span>(1\u756a\u76ee), <span class=\"underline\">T.Mizuno<\/span>(15\u756a\u76ee), <span class=\"underline\">M.Ohno<\/span>(21\u756a\u76ee), <span class=\"underline\">H.Takahashi<\/span>(27\u756a\u76ee), Y.Tanaka, \u4ed635\u540d, &ldquo;Soft gamma-raydetector (SGD) onboard the ASTRO-H mission,&rdquo; SPIE 9144, 91442C, (2014).<\/li>\n<li>G.Sato, <span class=\"underline\">Y.Fukazawa(<\/span>5\u756a\u76ee), J.Katsuta,<span class=\"underline\">T.Mizuno<\/span>(15\u756a\u76ee), <span class=\"underline\">M.Ohno<\/span>(20\u756a\u76ee), <span class=\"underline\">H.Takahashi<\/span>(25\u756a\u76ee) <em>et al.<\/em> (\u8a0834\u540d), &ldquo;The HardX-ray Imager (HXI) for the ASTRO-H Mission,&rdquo; SPIE 9144, 914427, (2014).<\/li>\n<li>T.Takahashi, <span class=\"underline\">Y.Fukazawa<\/span>(43\u756a\u76ee),<span class=\"underline\">T.Mizuno<\/span>(126\u756a\u76ee), <span class=\"underline\">M.Ohno<\/span>(154\u756a\u76ee), <span class=\"underline\">H.Takahashi<\/span>(199\u756a\u76ee), Y.Tanaka <em>et al.<\/em> (\u8a08248\u540d), &ldquo;The ASTRO-H X-ray astronomy satellite,&rdquo; SPIE 9144, 914425, (2014).<\/li>\n<li><span class=\"underline\">T.Mizuno<\/span>, <span class=\"underline\">Y.Fukazawa<\/span>(3\u756a\u76ee), \u4ed627\u540d, &ldquo;Development and calibration offine collimators for the ASTRO-H Soft Gamma-ray Detector,&rdquo; SPIE 9144,91445F, (2014).<\/li>\n<li><span class=\"underline\">M.Ohno<\/span>(16\u756a\u76ee), \u4ed620\u540d, &ldquo;ASTRO-H WhitePaper - Accreting Pulsars, Magnetars, and Related Sources,&rdquo; arXiv:1412.1165, (2014).<\/li>\n<li>C.Done, <span class=\"underline\">H.Takahashi<\/span>(19\u756a\u76ee) <em>etal.<\/em> (\u8a0823\u540d), &ldquo;ASTRO-H White Paper ? Low-mass X-ray Binaries,&rdquo; arXiv:1412.1164, (2014).<\/li>\n<li>M.Miller, <span class=\"underline\">T.Mizuno<\/span>(10\u756a\u76ee) <em>etal<\/em>. (\u8a0813\u540d), &ldquo;ASTRO-H White Paper ? Stellar-Mass Black Holes,&rdquo; arXiv:1412.1173, (2014).<\/li>\n<li>J.S.Kaastra, <span class=\"underline\">Y.Fukazawa<\/span>(7\u756a\u76ee) <em>etal.<\/em> (\u8a0826\u540d), &ldquo;ASTRO-H White Paper ? AGN Winds,&rdquo; arXiv:1412.1171,(2014).<\/li>\n<li>R.K.Smith, <span class=\"underline\">Y.Tanaka<\/span>, <em>etal.<\/em> (\u8a0830\u540d), &ldquo;ASTRO-H White Paper ? New Spectral Features,&rdquo; arXiv:1412.1172, (2014).<\/li>\n<li>P.Coppi, <span class=\"underline\">Y.Fukazawa<\/span>(4\u756a\u76ee),<span class=\"underline\">T.Mizuno<\/span>(10\u756a\u76ee), Y.Tanaka <em>et al.<\/em>(\u8a0816\u540d), &ldquo;ASTRO-H White Paper ? Broad-band Spectroscopy and Polarimetry,&rdquo; arXiv:1412.1190, (2014).<\/li>\n<li>M.S.Tashiro, <span class=\"underline\">M.Ohno<\/span>(3\u756a\u76ee) <em>etal.<\/em> (\u8a0810\u540d), &ldquo;ASTRO-H White Paper ? Chemical Evolution in High-zUniverse,&rdquo; arXiv:1412.1190, (2014).<\/li>\n<li>R.Itoh, <span class=\"underline\">Y.Fukazawa<\/span>, K.Kawaguchi,Y.Kanda, Y.T.Tanaka, <span class=\"underline\">M.Uemura<\/span>,<span class=\"underline\">K.S.Kawabata<\/span>, H.Akitaya, &ldquo;Study forrelation between direction of relativistic jet and optical polarizationangle with multi-wavelength observation,&rdquo; Proc. 5th Fermi Symposium,arXiv:1502.02802, (2014).<\/li>\n<li>Y.T.Tanaka, <span class=\"underline\">Y.Fukazawa<\/span>(6\u756a\u76ee),R.Itoh, \u4ed66\u540d, &ldquo;Fermi-LAT and Multi-wavelength Monitoring of the BroadLine Radio Galaxy 3C 120,&rdquo; Proc. 5th Fermi Symposium, arXiv:1503.04248,(2014).<\/li>\n<li><span class=\"underline\">Y.Fukazawa<\/span>, S.Tokuda, R.Itoh,Y.T.Tanaka, J.Finke, L.Stawarz, &ldquo;Suzaku and Fermi Observations ofGamma-Ray Bright Radio Galaxies: Origin of the X-ray Emission andBroad-Band Modeling,&rdquo; Proc. 5th Fermi Symposium, arXiv:1504.01908,(2014).<\/li>\n<li>T.Kawano, <span class=\"underline\">H.Takahashi<\/span>, <em>etal<\/em>, &ldquo;Pathfinder flight of the Polarized Gamma-ray Observer(PoGOLite) in 2013,&rdquo; Proc. 5th Fermi Symposium, arXiv:1503.01300,(2014).<\/li>\n<li><span class=\"underline\">M.Ohno,<\/span> T.Kawano, <em>et al.<\/em>, &ldquo;Observations of Gamma-ray Bursts with ASTRO-H and Fermi,&rdquo; Proc. 5thFermi Symposium, arXiv:1503.01182, (2014).<\/li>\n<li>H.Akitaya, Y.Moritani, T.Ui, T.Urano, Y.Ohashi, <span class=\"underline\">K.S.Kawabata<\/span>, A.Nakashima, M.Sasada, K.Sakimoto,T.Harao, H.Miyamoto, R.Matsui, R.Itoh, K.Takaki, I.Ueno, T.Ohsugi,H.Nakaya, T.Yamashita, <span class=\"underline\">M.Yoshida<\/span>, &ldquo;HONIR:an optical and near-infrared simultaneous imager, spectrograph, andpolarimeter for the 1.5-m Kanata telescope,&rdquo; SPIE 9147, 91474O (2014).<\/li>\n<li>T.Ui, S.Sako, T.Yamashita, H.Akitaya, <span class=\"underline\">K.S.Kawabata,<\/span> H.Nakaya, Y.Moritani, R.Itoh, K.Takaki,T.Urano, I.Ueno, T.Ohsugi, <span class=\"underline\">M.Yoshida,<\/span>H.Nakao, Y.Hashiba, &ldquo;Development of a new readout system for thenear-infrared detector of HONIR,&rdquo; SPIE 9147, 94176C (2014).<\/li>\n<li>L.Wang, <span class=\"underline\">M.Yoshida<\/span>(12\u756a\u76ee) \u4ed615\u540d, &ldquo;Along-period eccentric substellar companion to the evolvedintermediate-mass star HD 14067,&rdquo; <em>PASJ<\/em>, <strong>66<\/strong>(2014) 118.<\/li>\n<li>Y.Itoh, <span class=\"underline\">S.Miyama<\/span>(28\u756a\u76ee) \u4ed648\u540d, &ldquo;Near-infrared polarimetry of the GG Tauri A binary system,&rdquo; <em>Research in Astronomy and Astrophysics<\/em>, <strong>14<\/strong>(2014) 1438.<\/li>\n<li>M.Takami, <span class=\"underline\">S.Miyama<\/span>(43\u756a\u76ee) \u4ed659\u540d, &ldquo;Surface Geometry of Protoplanetary Disks Inferred From Near-InfraredImaging Polarimetry,&rdquo; <em>ApJ<\/em>,<strong>795<\/strong> (2014) 71.<\/li>\n<li>M.Honma, K.Akiyama, <span class=\"underline\">M.Uemura,<\/span> andS.Ikeda, &ldquo;Super-resolution imaging with radio interferometry usingsparse modeling,&rdquo; <em>PASJ<\/em>, <strong>66<\/strong> (2014) 95.<\/li>\n<li>T.D.Brandt, <span class=\"underline\">S.Miyama<\/span>(36\u756a\u76ee) \u4ed651\u540d, &ldquo;AStatistical Analysis of SEEDS and Other High-contrast ExoplanetSurveys: Massive Planets or Low-mass Brown Dwarfs?,&rdquo; <em>ApJ<\/em>,<strong>794<\/strong> (2014) 159.<\/li>\n<li>A.Fukui, <span class=\"underline\">M.Yoshida<\/span>(24\u756a\u76ee) \u4ed623\u540d, &ldquo;Multi-band, Multi-epoch Observations of the Transiting Warm JupiterWASP-80b,&rdquo; <em>ApJ<\/em>, <strong>790<\/strong> (2014) 108.<\/li>\n<li>L.Pacciani, F.Tavecchio, I.Donnarumma, A.Stamerra, L.Carrasco,E.Recillas, A.Porras, and <span class=\"underline\">M.Uemura<\/span>, &ldquo;Exploring the Blazar Zone in High-energy Flares of FSRQs,&rdquo; <em>ApJ<\/em>, <strong>790<\/strong> (2014) 45.<\/li>\n<li>M.Shidatsu, Y.Ueda, S.Yamada, C.Done, T.Hori, K.Yamaoka, A.Kubota,T.Nagayama, and <span class=\"underline\">Y.Moritani<\/span>, &ldquo;Spectraland Timing Properties of the Black Hole X-Ray Binary H1743-322 in theLow\/Hard State Studied with Suzaku,&rdquo; <em>ApJ<\/em>, <strong>789<\/strong>(2014) 100.<\/li>\n<li>S.Hasegawa, <span class=\"underline\">M.Yoshida<\/span>(9\u756a\u76ee) \u4ed618\u540d, &ldquo;Lightcurve survey of V-type asteroids in the inner asteroid belt,&rdquo; <em>PASJ<\/em>, <strong>66<\/strong> (2014) 54.<\/li>\n<li>M.Ishiguro, <span class=\"underline\">M.Yoshida<\/span>(8\u756a\u76ee) \u4ed611\u540d, &ldquo;Outbursting Comet P\/2010 V1 (Ikeya-Murakami): A Miniature CometHolmes,&rdquo; <em>ApJ<\/em>, <strong>787<\/strong> (2014) 55.<\/li>\n<li>N.Oshita, <span class=\"underline\">K.Yamamoto<\/span>, and S.Zhang, &ldquo;Thermal property in Brownian motion of a particle coupled to vacuumfluctuations,&rdquo; <em>Physical Review<\/em> D<strong>89<\/strong> (2014)124028.<\/li>\n<li>Y.Takushima, A.Terukina, and <span class=\"underline\">K.Yamamoto<\/span>, &ldquo;Bispectrum of cosmological densityperturbations in the most general second-order scalar-tensor theory,&rdquo; <em>Physical Review<\/em> D<strong>89<\/strong> (2014) 104007-1-13.<\/li>\n<li>A.Terukina, L.Lombriser, <span class=\"underline\">K.Yamamoto<\/span>,D.Bacon, K.Koyama, and R.C.Nichol, &ldquo;Testing chameleon gravity with theComa cluster,&rdquo; <em>Journal of Cosmology and Astroparticle Physics<\/em>,<strong>04<\/strong> (2014) 013.<\/li>\n<li>L.Heisenberg, R.Kimura, <span class=\"underline\">K.Yamamoto<\/span>, &ldquo;Cosmology of the proxy theory to massive gravity,&rdquo; <em>PhysicalReview<\/em> D<strong>89<\/strong> (2014) 103008.<\/li>\n<li>A.Oka, S.Saito, T.Nishimichi, A.Taruya, <span class=\"underline\">K.Yamamoto<\/span>, &ldquo;Simultaneous constraints on the growth ofstructure and cosmic expansion from the multipole power spectra of theSDSS DR7 LRG,&rdquo; <em>Monthly Notice of the Royal Astronomical Society<\/em><strong>439<\/strong> (2014) 2515.<\/li>\n<li>J.Adam, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Two-pion femtoscopy inp-Pb collisions at \u221as<sub>NN<\/sub> = 5.02 TeV,&rdquo; <em>Phys. Rev. C<\/em><strong>91<\/strong>, 034906, 2015.<\/li>\n<li>B.Abelev, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Production of inclusive\u03a5(1S) and \u03a5(2S) in p-Pb collisions at \u221as<sub>NN<\/sub> = 5.02 TeV,&rdquo; <em>Phys. Lett.<\/em> <strong>B740<\/strong>, 105-117, 2015.<\/li>\n<li>B.Abelev, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Multiplicity dependenceof jet-like two-particle correlations in p-Pb collisions at\u221as<sub>NN<\/sub> = 5.02 TeV,&rdquo; <em>Phys. Lett.<\/em> <strong>B741<\/strong>,38-50, 2015.<\/li>\n<li>B.Abelev, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Production of\u03a3(1385)<sup>\u00b1<\/sup> and \u039e(1530)<sup>0<\/sup> in proton-proton collisionsat \u221as = 7 TeV,&rdquo; <em>Eur. Phys. J.<\/em> <strong>C75<\/strong>, 1, 2015.<\/li>\n<li>B.Abelev, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Measurement of electronsfrom semileptonic heavy-flavor hadron decays in pp collisions at \u221as =2.76 TeV,&rdquo; <em>Phys. Rev. D<\/em> <strong>91<\/strong>, 012001, 2015.<\/li>\n<li>B.Abelev, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;K*(892)<sup>0<\/sup> and\u03c6(1020) production in Pb-Pb collisions at \u221as<sub>NN<\/sub> = 2.76 TeV,&rdquo; <em>Phys. Rev. C<\/em> <strong>91<\/strong>, 024609, 2015.<\/li>\n<li>B.Abelev, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Event-by-event meanp<sub>T<\/sub> fluctuations in pp and Pb-Pb collisions at the LHC,&rdquo; <em>Eur. Phys. J.<\/em> <strong>C74<\/strong>, 3077, 2014.<\/li>\n<li>B.Abelev, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Exclusive J\/\u03a8photoproduction off protons in ultra-peripheral p-Pb collisions at\u221as<sub>NN<\/sub> = 5.02 TeV,&rdquo; <em>Phys. Rev. Lett.<\/em><strong>113<\/strong>, 232504, 2014.<\/li>\n<li>B.Abelev, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Multiparticle azimuthalcorrelations in p-Pb and Pb-Pb collisions at the CERN Large HadronCollider,&rdquo; <em>Phys. Rev. C<\/em> <strong>90<\/strong>, 054901, 2014.<\/li>\n<li>B.Abelev, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Suppression of \u03a5(1S) atforward rapidity in Pb-Pb collisions at \u221as<sub>NN<\/sub> = 2.76 TeV,&rdquo; <em>Phys. Lett.<\/em> <strong>B738<\/strong>, 361-372, 2014.<\/li>\n<li>B.Abelev, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Beauty production in ppcollisions at \u221as = 2.76 TeV measured via semi-electronic decays,&rdquo; <em>Phys. Lett.<\/em> <strong>B738<\/strong>, 97-108, 2014.<\/li>\n<li>B.Abelev, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Suppression of \u03a8(2S)production in p-Pb collisions at \u221as<sub>NN<\/sub> = 5.02 TeV,&rdquo; <em>JHEP<\/em> <strong>1412<\/strong>, 073, 2014.<\/li>\n<li>B.Abelev, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Neutral pion productionat midrapidity in pp and Pb-Pb collisions at \u221as<sub>NN<\/sub> = 2.76 TeV,&rdquo; <em>Eur. Phys. J.<\/em> <strong>C74<\/strong>, 3108, 2014.<\/li>\n<li>B.Abelev, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Measurement of promptD-meson production in p-Pb collisions at \u221as<sub>NN<\/sub> = 5.02 TeV,&rdquo; <em>Phys. Rev. Lett.<\/em> <strong>113<\/strong>, 232301, 2014.<\/li>\n<li>B.Abelev, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Transverse momentumdependence of inclusive primary charged-particle production in p-Pbcollisions at \u221as<sub>NN<\/sub> = 5.02 TeV,&rdquo; <em>Eur. Phys. J.<\/em><strong>C74<\/strong>, 3054, 2014.<\/li>\n<li>B.Abelev, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Azimuthal anisotropy ofD meson production in Pb-Pb collisions at \u221as<sub>NN<\/sub> = 2.76 TeV,&rdquo; <em>Phys. Rev. C<\/em> <strong>90<\/strong>, 034904, 2014.<\/li>\n<li>B.Abelev, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Measurement of visiblecross sections in proton-lead collisions at \u221as<sub>NN<\/sub> = 5.02 TeV invan der Meer scans with the ALICE detector,&rdquo; <em>JINST<\/em><strong>9<\/strong>, P11003, 2014.<\/li>\n<li>B.Abelev, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Freeze-out radiiextracted from three-pion cumulants in pp, p-Pb and Pb-Pb collisions atthe LHC,&rdquo; <em>Phys. Lett.<\/em> <strong>B739<\/strong>, 139-151, 2014.<\/li>\n<li>B.Abelev, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Measurement ofquarkonium production at forward rapidity in pp collisions at \u221as = 7TeV,&rdquo; <em>Eur. Phys. J.<\/em> <strong>C74<\/strong>, 2974, 2014.<\/li>\n<li>B.Abelev, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Production of chargedpions, kaons and protons at large transverse momenta in pp and Pb-Pbcollisions at \u221as<sub>NN<\/sub> =2.76 TeV,&rdquo; <em>Phys. Lett.<\/em><strong>B736<\/strong>, 196-207, 2014.<\/li>\n<li>B.Abelev, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Measurement of chargedjet suppression in Pb-Pb collisions at \u221as<sub>NN<\/sub> = 2.76 TeV,&rdquo; <em>JHEP<\/em> <strong>1403<\/strong>, 013, 2014.<\/li>\n<li>B.Abelev, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Centrality, rapidity andtransverse momentum dependence of J\/\u03a8 suppression in Pb-Pb collisions at\u221as<sub>NN<\/sub> = 2.76 TeV,&rdquo; <em>Phys. Lett.<\/em> <strong>B734<\/strong>,314-327, 2014.<\/li>\n<li>A.Adare, <span class=\"underline\">K.Homma<\/span>, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>,<em>et al.<\/em>, &ldquo;Charged-pion cross sections and double-helicityasymmetries in polarized p+p collisions at \u221as =200\u2009\u2009GeV,&rdquo; <em>Phys. Rev.D<\/em><strong>91<\/strong>, 032001, 2015.<\/li>\n<li>A.Adare, <span class=\"underline\">K.Homma<\/span>, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>,<em>et al.<\/em>, &ldquo;Search for dark photons from neutral meson decays inp+p and d + Au collisions at \u221as<sub>NN<\/sub> = 200 GeV,&rdquo; <em>Phys.Rev.C<\/em><strong>91<\/strong>, 031901, 2015.<\/li>\n<li>A.Adare, <span class=\"underline\">K.Homma<\/span>, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>,<em>et al.<\/em>, &ldquo;Cross section and transverse single-spin asymmetry of \u03b7mesons in p\u2191+p collisions at \u221as =200 GeV at forward rapidity,&rdquo; <em>Phys.Rev. D<\/em><strong>90<\/strong>, 072008, 2014.<\/li>\n<li>A.Adare, <span class=\"underline\">K.Homma<\/span>, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>,<em>et al.<\/em>, &ldquo;Cross section for <span class=\"math inline\">$b\\overline{b}$<\/span> production via dielectrons in d+Aucollisions at \u221as<sub>NN<\/sub> =200 GeV,&rdquo; <em>Phys. Rev.C<\/em><strong>91<\/strong>, 014907, 2015.<\/li>\n<li>A.Adare, <span class=\"underline\">K.Homma<\/span>, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>,<em>et al.<\/em>, &ldquo;Low-mass vector-meson production at forward rapidity inp+p collisions at \u221as =200 GeV,&rdquo; <em>Phys. Rev. D<\/em><strong>90<\/strong>,052002, 2014.<\/li>\n<li>A.Adare, <span class=\"underline\">K.Homma<\/span>, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>,<em>et al.<\/em>, &ldquo;Measurement of K<sub>s<\/sub><sup>0<\/sup> and<span class=\"math inline\"><em>K<\/em><sup>*<\/sup><\/span><sup>0<\/sup> inp+p, d+Au, and Cu+Cu collisions at \u221as<sub>NN<\/sub> =200 GeV,&rdquo; <em>Phys.Rev. C<\/em><strong>90<\/strong>, 054905, 2014.<\/li>\n<li>A.Adare, <span class=\"underline\">K.Homma<\/span>, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>,<em>et al.<\/em>, &ldquo;Measurement of \u03a5(1S+2S+3S) production in p+p and Au+Aucollisions at \u221as<sub>NN<\/sub> =200 GeV,&rdquo; <em>Phys. Rev.C<\/em><strong>91<\/strong>, 024913, 2015.<\/li>\n<li>A.Adare, <span class=\"underline\">K.Homma<\/span>, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>,<em>et al.<\/em>, &ldquo;Inclusive double-helicity asymmetries in neutral-pionand eta-meson production in <span class=\"math inline\"><em>p\u20d7<\/em><\/span>+ <span class=\"math inline\"><em>p\u20d7<\/em><\/span> collisions at \u221as =200GeV,&rdquo; <em>Phys. Rev. D<\/em><strong>90<\/strong>, 012007, 2014.<\/li>\n<li>A.Adare, <span class=\"underline\">K.Homma<\/span>, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>,<em>et al.<\/em>, &ldquo;Azimuthal-angle dependence ofcharged-pion-interferometry measurements with respect to second- andthird-order event planes in Au+Au collisions at \u221as<sub>NN<\/sub> =200GeV,&rdquo; <em>Phys. Rev. Lett.<\/em> <strong>112<\/strong>, 222301, 2014.<\/li>\n<li>S.S.Adler, <span class=\"underline\">K.Homma<\/span>, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>,<em>et al.<\/em>, &ldquo;Transverse-energy distributions at midrapidity in p+p ,d+Au , and Au+Au collisions at \u221as<sub>NN<\/sub> =62.4\u2013200 GeV andimplications for particle-production models,&rdquo; <em>Phys. Rev.C<\/em><strong>89<\/strong><em>,<\/em> 044905, 2014.<\/li>\n<li>A.Adare, <span class=\"underline\">K.Homma<\/span>, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>,<em>et al.<\/em>, &ldquo;Measurement of transverse-single-spin asymmetries formidrapidity and forward-rapidity production of hadrons in polarized p+pcollisions at \u221as =200 and 62.4 GeV,&rdquo; <em>Phys. Rev.D<\/em><strong>90<\/strong><em>,<\/em> 012006, 2014<em>.<\/em>.<\/li>\n<li>A.Adare, <span class=\"underline\">K.Homma<\/span>, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>,<em>et al.<\/em>, &ldquo;System-size dependence of open-heavy-flavor productionin nucleus-nucleus collisions at \u221as<sub>NN<\/sub> =200 GeV,&rdquo; <em>Phys.Rev. C<\/em><strong>90<\/strong><em>, 034903, 2014<\/em>.<\/li>\n<li>A.Adare, <span class=\"underline\">K.Homma<\/span>, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>,<em>et al.<\/em>, &ldquo;Centrality categorization for R<sub>p(d)+A<\/sub> inhigh-energy collisions,&rdquo; <em>Phys. Rev.C<\/em><strong>90<\/strong><em>,<\/em> 034902, 2014.<\/li>\n<li>A.Adare, <span class=\"underline\">K.Homma<\/span>, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>,<em>et al.<\/em>, &ldquo;Cold-Nuclear-Matter Effects on Heavy-Quark Productionat Forward and Backward Rapidity in d+Au Collisions at \u221as<sub>NN<\/sub>=200\u2009\u2009GeV,&rdquo; <em>Phys. Rev. Lett.<\/em> <strong>112<\/strong>, 252301, 2014.<\/li>\n<li><span class=\"underline\">K.Homma<\/span>, &ldquo;Perspective to search forsub-eV neutral boson resonances with stimulated laser colliders,&rdquo; <em>Eur.Phys.J.ST<\/em> <strong>223<\/strong>, 1131-1137, 2014.<\/li>\n<li><span class=\"underline\">K.Homma<\/span>, <em>et al.<\/em>, &ldquo;The firstsearch for sub-eV scalar fields via four-wave mixing at a quasi-parallellaser collider,&rdquo; <em>Prog. Theor. Exp. Phys.,<\/em> 083C01, 2014<em>.<\/em>.<\/li>\n<li>M.Garcia Perez, A.Gonzalez-Arroyo and <span class=\"underline\">M.Okawa<\/span>, &ldquo;Volume independence for Yang\u2013Mills fieldson the twisted torus,&rdquo; <em>Int. J. Mod. Phys.<\/em> A<strong>29<\/strong>(2014) 25, 1445001.<\/li>\n<li>A.Gonzalez-Arroyo and <span class=\"underline\">M.Okawa<\/span>, &ldquo;Testing volume independence of SU(N) pure gauge theories at large N,&rdquo; <em>JHEP<\/em> <strong>1412<\/strong> (2014) 106.<\/li>\n<li>M.Garcia Perez, A.Gonzalez-Arroyo, L.Keegan and <span class=\"underline\">M.Okawa<\/span>, &ldquo;The <em>SU<\/em>(\u221e)&#160;twisted gradientflow running coupling,&rdquo; <em>JHEP<\/em> <strong>1501<\/strong> (2015) 038.<\/li>\n<li><span class=\"underline\">T.Morozumi<\/span>, H.Okane, H.Umeeda, &ldquo;Precise Discussion of Time-Reversal Asymmetries in B-meson decays,&rdquo; <em>Journal of High Energy Physics<\/em> (JHEP) <strong>1502<\/strong>(2015) 174.<\/li>\n<li>R.Hotta, <span class=\"underline\">T.Morozumi<\/span>, H.Takata, &ldquo;Timevariation of particle and antiparticle asymmetry in an expandinguniverse,&rdquo; <em>Phys.Rev.<\/em> D<strong>90<\/strong> (2014) 1, 016008.<\/li>\n<li><span class=\"underline\">K.-I.Ishikawa<\/span>, Y.Iwasaki, YuNakayama, T.Yoshie, &ldquo;Global Structure of Conformal Theories in theSU(3) Gauge Theory,&rdquo; <em>Phys. Rev.<\/em> D<strong>89<\/strong> (2014)114503.<\/li>\n<\/ul>\n\n<p><a id=\"presentations_H26\"><\/a><\/p>\n<h2>\u5b66\u4f1a\u30fb\u7814\u7a76\u4f1a\u3067\u306e\u767a\u8868 Presentations<\/h2>\n<ul style=\"list-style-type: disc;\">\n<li><span class=\"underline\">Y.Fukazawa<\/span>: &ldquo;ASTRO-H&rdquo;, Workshop onSynergy of HSC and Hiroshima CORE=U prospects for Galacy Clusters andAstronomical Transients, (27,August, Hiroshima University, \u53c2\u52a0\u4eba\u657060\u540d).<\/li>\n<li><span class=\"underline\">Y.T.Tanaka<\/span>: &ldquo;Fermi Large AreaTelescope detection of two Very-High-Energy (<em>E<\/em>&gt;100GeV)Gamma-ray Photons from the z=1.1 blazar PKS 0426-380&rdquo;, UCLA Symposiumon Particle Astrophysics and Cosmology Including FundamentalInteraCtions (15-20, Sept., Moorea, Polynesia, \u53c2\u52a0\u4eba\u657030\u540d).<\/li>\n<li><span class=\"underline\">T.Mizuno<\/span>: &ldquo;Suzaku Observation of theFermi Cygnus Cocoon&rdquo;, 5th Fermi Symposium, (20-24 Oct.2014,Nagoya,\u53c2\u52a0\u4eba\u6570180\u540d).<\/li>\n<li><span class=\"underline\">H.Takahashi<\/span>: &ldquo;X-ray View ofAndromeda Galaxy, M31&rdquo;, (20-24 Oct.2014, Nagoya,\u53c2\u52a0\u4eba\u6570180\u540d).<\/li>\n<li><span class=\"underline\">M.Ohno<\/span>: &ldquo;Observations of Gamma-rayBursts with ASTRO-H and Fermi&rdquo;, (20-24 Oct.2014, Nagoya,\u53c2\u52a0\u4eba\u6570180\u540d).<\/li>\n<li><span class=\"underline\">Y.Fukazawa<\/span>: &ldquo;Suzaku and FermiObservations of Gamma-Ray Bright Radio Galaxies: Origin of the X-rayEmission and Broad-Band Modeling&rdquo;, (20-24 Oct.2014, Nagoya,\u53c2\u52a0\u4eba\u6570180\u540d).<\/li>\n<li>J.Katsuta: &ldquo;Fermi-LAT Observation of Extended Gamma-ray Emissionfrom the G25.0+0.0 Region&rdquo;, (20-24 Oct.2014, Nagoya,\u53c2\u52a0\u4eba\u6570180\u540d).<\/li>\n<li>I.Edahiro: &ldquo;Suzaku X-Ray Monitoring of Gamma-Ray-Emitting RadioGalaxy, NGC 1275&rdquo;, (20-24 Oct.2014, Nagoya,\u53c2\u52a0\u4eba\u6570180\u540d).<\/li>\n<li>Y.T.Tanaka: &ldquo;Six-years of Fermi-LAT and Multi-wavelength Monitoringof the Broad Line Radio Galaxy 3C 120&rdquo;, (20-24 Oct.2014,Nagoya,\u53c2\u52a0\u4eba\u6570180\u540d).<\/li>\n<li>R.Itoh: &ldquo;Study For Relation Between Direction of Relativistic jetand Optical Polarization Angle With Multi-wavelenght Observation&rdquo;,(20-24 Oct.2014, Nagoya,\u53c2\u52a0\u4eba\u6570180\u540d).<\/li>\n<li>T.Kawano: &ldquo;Pathfinder Flight of the Polarized Gamma-ray Observer(PoGOLite) in 2013&rdquo;, (20-24 Oct.2014, Nagoya,\u53c2\u52a0\u4eba\u6570180\u540d).<\/li>\n<li>K.Kawaguchi: &ldquo;Kanata optical and X-ray monitoring of Gamma-rayemitting Narrow-Line Seyfert 1 and Radio galaxies&rdquo;, (20-24 Oct.2014,Nagoya,\u53c2\u52a0\u4eba\u6570180\u540d).<\/li>\n<li>H.Shirakawa: &ldquo;Study of the X-ray Emission Mechanism of Radio-loudNarrow-line Seyfert 1 Galaxy 1H0323+342&rdquo;, (20-24 Oct.2014,Nagoya,\u53c2\u52a0\u4eba\u6570180\u540d).<\/li>\n<li>Y.T.Tanaka: &ldquo;Cen A Core and Lobes, and 3C 120 (Fermi + VLBA)&rdquo;,Fermi LAT Collaboration Meeting, (1-5 Sept, 2014, Monpellier, France,\u53c2\u52a0\u4eba\u6570120\u540d).<\/li>\n<li>R.Itoh: &ldquo;CTA 102&rdquo;, Fermi LAT Collaboration Meeting, (1-5 Sept,2014, Monpellier, France, \u53c2\u52a0\u4eba\u6570120\u540d).<\/li>\n<li>Y.T.Tanaka: &ldquo;Centaurus A with Pass 8&rdquo;, Fermi LAT CollaborationMeeting, (15-19, March, 2015, SLAC, USA, \u53c2\u52a0\u4eba\u6570110\u540d).<\/li>\n<li>J.Katsuta: &ldquo;Star forming region NGC 3603&rdquo;, Fermi LAT CollaborationMeeting, (15-19, March, 2015, SLAC, USA, \u53c2\u52a0\u4eba\u6570110\u540d).<\/li>\n<li>R.Itoh: &ldquo;Kanata Optical Monitoring&rdquo;, Fermi LAT CollaborationMeeting, (15-19, March, 2015, SLAC, USA, \u53c2\u52a0\u4eba\u6570110\u540d).<\/li>\n<li>T.Kawano: &ldquo;TeV gamma-ray binary HESS J0632+057&rdquo;, Fermi LATCollaboration Meeting, (15-19, March, 2015, SLAC, USA, \u53c2\u52a0\u4eba\u6570110\u540d).<\/li>\n<li>K.Kawaguchi: &ldquo;NLSy1 Optical Monitoring&rdquo;, Fermi LAT CollaborationMeeting, (15-19, March, 2015, SLAC, USA, \u53c2\u52a0\u4eba\u6570110\u540d).<\/li>\n<li><span class=\"underline\">Y.Fukazawa<\/span>: &ldquo;Soft gamma-raydetector (SGD) onboard the ASTRO-H mission&rdquo;, SPIE AstronomicalTelescope+Instrumentation, (22-27, June, 2014, Montreal, Canada,\u53c2\u52a0\u4eba\u65702,500\u540d).<\/li>\n<li><span class=\"underline\">T.Mizuno<\/span>: &ldquo;Development andcalibration of Fine Collimators for the ASTRO-H Soft Gamma-rayDetector&rdquo;, SPIE Astronomical Telescope+Instrumentation, (22-27, June,2014, Montreal, Canada, \u53c2\u52a0\u4eba\u65702,500\u540d).<\/li>\n<li><span class=\"underline\">M.Ohno<\/span>: &ldquo;Hard X-ray and SoftGamma-ray Observations of Solar Flares with Suzaku Wide-band All-skyMonitor&rdquo;, 13th RHESSI Workshop, (1-4, April, 2014, \u53c2\u52a0\u4eba\u6570100\u540d).<\/li>\n<li><span class=\"underline\">M.Ohno<\/span>: &ldquo;Development andVerification of Signal Processing System of BGO Active Shield onboardAstro-H&rdquo;, SPIE Astronomical Telescope+Instrumentation, (22-27, June,2014, Montreal, Canada, \u53c2\u52a0\u4eba\u65701,000\u540d).<\/li>\n<li><span class=\"underline\">H.Takahashi<\/span>: &ldquo;Data AcquisitionSystem and Ground Calibration of Polaized Gamma-ray Observer(PoGOLite)&rdquo;, SPIE Astronomical Telescope+Instrumentation, (22-27, June,2014, Montreal, Canada, \u53c2\u52a0\u4eba\u65702,500\u540d).<\/li>\n<li><span class=\"underline\">M.Uemura<\/span>: &ldquo;Variable Selection forModeling the Absolute Magnitude at Maximum of Type Ia Supernovae&rdquo;,Tools for Astronomical Big Data, (9-11 Mar, 2015, Arizona, USA, \u4eba\u6570150\u540d).<\/li>\n<li><span class=\"underline\">M.Ohno<\/span>: &ldquo;Future ASTRO-Hobservations of chemical evolution in high-z universe&rdquo;, AmericanAstronomical Society 225th meeting, (4-8, Jan., 2015, USA, \u53c2\u52a0\u4eba\u65702,500\u540d).<\/li>\n<li>H.Akitaya: &ldquo;HONIR: an optical and near-infrared simultaneousimager, spectrograph, and polarimeter for the 1.5-m Kanata telescope&rdquo;,American Astronomical Society 225th meeting, (4-8, Jan., 2015, USA,\u53c2\u52a0\u4eba\u65702,500\u540d).<\/li>\n<li>T.Ui: &ldquo;Development of a new readout system for the near-infrareddetector of HONIR&rdquo;, American Astronomical Society 225th meeting, (4-8,Jan., 2015, USA, \u53c2\u52a0\u4eba\u65702,500\u540d).<\/li>\n<li><span class=\"underline\">H.Takahashi<\/span>: &ldquo;Suzaku Observation ofthe Symbiotic X-ray Binary IGR J16194-2810&rdquo;, COSPAR2014, (2-10, August,2014, Russia, \u53c2\u52a0\u4eba\u6570500\u540d).<\/li>\n<li><span class=\"underline\">H.Takahashi<\/span>: &ldquo;Development ofPortable Compact Gamma-Ray Spectrometer with CsI(Tl+MPPC&rdquo;, IEEENSS\/MIC, (8-16, Nov., 2014, \u53c2\u52a0\u4eba\u6570500\u540d).<\/li>\n<li>S.Furui: &ldquo;Geant4 simulation of X-ray Reflection by AGN Torus&rdquo;, 5thASTRO-H Summer School (8-9, Jully, 2014, University of Paris 7, France,\u53c2\u52a0\u4eba\u657040\u540d).<\/li>\n<li>I.Edahiro: &ldquo;Study of Fe-K\u03b1 Line Resonance Scattering in theIntracluster Medium with Monte-Carlo Simulation for Suzaku andASTRO-H&rdquo;, 5th ASTRO-H Summer School (8-9, Jully, 2014, University ofParis 7, France, \u53c2\u52a0\u4eba\u657040\u540d).<\/li>\n<li>T.Kawano: &ldquo;SGD BGO Wide--field All--sky Monitor&rdquo;, 5th ASTRO-HSummer School (8-9, Jully, 2014, University of Paris 7, France,\u53c2\u52a0\u4eba\u657040\u540d).<\/li>\n<li>K.Takaki: &ldquo;Polarization observations of 5 GRB afterglows&rdquo;,Astronomical Polarimetry 2014, (26-30, May, 2014, MINATEC, France,\u53c2\u52a0\u4eba\u657050\u4eba).<\/li>\n<li>H.Akitaya: &ldquo;Optical and Near-infrared Simultaneous PolarimeterHONIR&rdquo;, Astronomical Polarimetry 2014, (26-30, May, 2014, MINATEC,France, \u53c2\u52a0\u4eba\u657050\u4eba).<\/li>\n<li><span class=\"underline\">K.S.Kawabata<\/span>: &ldquo;SGMAP: An OpticalPolarimetric Survey Project in Hiroshima&rdquo;, Astronomical Polarimetry2014, (26-30, May, 2014, MINATEC, France, \u53c2\u52a0\u4eba\u657050\u4eba).<\/li>\n<li><span class=\"underline\">M.Yoshida<\/span>: &ldquo;Spectropolarimetry ofNearby Starburst Galaxies: Kinematics of the Dust Wind&rdquo;, AstronomicalPolarimetry 2014, (26-30, May, 2014, MINATEC, France, \u53c2\u52a0\u4eba\u657050\u4eba).<\/li>\n<li><span class=\"underline\">K.S.Kawabata<\/span>: &ldquo;SGMAP: OpticalPolarimetric Survey Project&rdquo;, Asia Oceania Geosciences Society, (28Jul-1 Aug 2014, Sapporo, Japan, \u53c2\u52a0\u4eba\u65701,500\u4eba).<\/li>\n<li><span class=\"underline\">M.Uemura<\/span>: &ldquo;Optical-infrared andHigh-energy Astronomy Collaboration at Hiroshima Astrophysical ScienceCenter&rdquo;, 12th Asia-Pacific Regional IAU Meeting, (18-22 Aug., 2014,Daejeon, Korea).<\/li>\n<li><span class=\"underline\">K.S.Kawabata<\/span>: &ldquo;SGMAP - opticalpolarimetry survey project&rdquo;, Workshop on Synergy of HSC and HiroshimaCORE-U Projects for Galaxy Clusters and Astronomical Transients, (27Aug 2014, Hiroshima University, \u53c2\u52a0\u800560\u540d).<\/li>\n<li>Y.Utsumi: &ldquo;The Current Status of HSC&rdquo;, Evolution of SMBHs withHSC: First Results from Initial Dataset, (18-20 Dec., 2014, Taipei,Taiwan, \u4eba\u657030\u4eba).<\/li>\n<li><span class=\"underline\">M.Yoshida<\/span>: &ldquo;Spectropolarimetry ofNearby Starburst Galaxies: Kinematics of the Dust Wind&rdquo;, China-SubaruWorkshop, (29 Nov.-1 Dec. 2014, Shanghai, China, \u4eba\u657050\u540d).<\/li>\n<li><span class=\"underline\">M.Uemura<\/span>: &ldquo;Sparse Modeling forImage Reconstruction in Astronomy&rdquo;, HIRES 2014: Astronomy at highangular resolution - cross-disciplinary approach, (24-28 Nov, 2014,ESO, Garching, Germany, \u4eba\u6570100\u540d).<\/li>\n<li>K.Takaki: &ldquo;Polarimetric observations of GRB afterglows&rdquo;, Supernovaand Gamma-ray Burst 2014, (25-27, August, 2014, RIKEN, \u53c2\u52a0\u4eba\u657050\u4eba).<\/li>\n<li>M.Kawabata: &ldquo;Observations of Type IIb Supernovae 2013df withBright Shock Breakout&rdquo;, Supernova and Gamma-ray Burst 2014, (25-27,August, 2014, RIKEN, \u53c2\u52a0\u4eba\u657050\u4eba).<\/li>\n<li><span class=\"underline\">Y.Kojima<\/span>; &ldquo;Black hole electromagneticstructure examined by two-fluid plasma flow&rdquo;, Olomouc Synergy in CzechRepublic\uff0811\u670822-24\u65e5 Olomouc, Czech\uff09\uff08\u53c2\u52a0\u8005100\u540d\uff09.<\/li>\n<li><span class=\"underline\">K.Yamamoto<\/span>; &ldquo;Testing modified gravitywith cluster of galaxies&rdquo;, Workshop on Synergy of HSC and HiroshimaCORE-U projects for Galaxy Clusters and Astronomical Transients \uff088\u670827\u65e5Hiroshima University, Higashi-hiroshima\uff09\uff08\u53c2\u52a0\u800572\u540d\uff09.<\/li>\n<li><span class=\"underline\">N.Okabe<\/span>; &ldquo;Subaru Weak-lensing MassMeasurements for Galaxy Clusters&rdquo;, Astroparticle View of GalaxyClusters\uff08March 24-26,2015, Hiroshima Univ.\uff09.<\/li>\n<li>A.Terukina, <span class=\"underline\">K.Yamamoto<\/span>;&ldquo;Observational constraint on a modified gravity model from the gas andshear profiles of a cluster of galaxies&rdquo;, 24th Workshop on GeneralRelativity and Gravitation (JGRG24) (11\u670812\u65e5,Kavli IPMU, The University ofTokyo, Kashiwa).<\/li>\n<li><span class=\"underline\">Y.Kojima<\/span>; &ldquo;Magneto-shear Oscillationsof Magnetars II&rdquo;, (\u65b0\u5b66\u8853\u9818\u57df\uff08\u91cd\u529b\u6ce2\u5929\u4f53\uff09\u7814\u7a76\u4f1a, 2015\u5e742\u670819 -21\u65e5, \u5e83\u5cf6\u5927\u5b66\uff09.<\/li>\n<li><span class=\"underline\">K.Yamamoto<\/span>; &ldquo;Gravity Tests on ClusterHalo Scales with Redshift-space Distortions&rdquo;, Astroparticle View ofCluster of Galaxies, (2015\u5e743\u670826\u65e5,Hiroshima University).<\/li>\n<li>A.Terukina, <span class=\"underline\">N.Okabe<\/span>, <span class=\"underline\">K.Yamamoto<\/span>, K.Matsushita, T.Sasaki; &ldquo;Observationalconstraint on a modified gravity model from the gas and shear profiles ofa cluster of galaxies&rdquo;, Astroparticle View of Cluster of Galaxies,(2015\u5e743\u670826\u65e5,Hiroshima University).<\/li>\n<li>T.Sasaki,K.Matsushita, K.Sato, and <span class=\"underline\">N.Okabe<\/span>; &ldquo;Suzaku Observations of Subhalos in the ComaCluster&rdquo; Astroparticle View of Galaxy Clusters, (2015\u5e743\u670826\u65e5,HiroshimaUniversity).<\/li>\n<li><span class=\"underline\">K.Homma<\/span>, &ldquo;TDR3: Combined Laser-Gammaexperiments&rdquo;, ELI-NP TDRs at Midway-High Power Laser System,(Bucharest-Magurele, Romania, 2014.04.02).<\/li>\n<li><span class=\"underline\">K.Shigaki<\/span>, &ldquo;Physics at High EnergyNucleus-Nucleus Colliders: Prospect and Relevance to Hadron Physics&rdquo;,Hadron Physics Symposium (Nagoya, Japan, 2014.4.17-19).<\/li>\n<li><span class=\"underline\">K.Homma<\/span>, &ldquo;Toward laboratory searchfor sub-eV netural bosons via resonances by stimulated photon-photoncollider&rdquo;, 23rd ANNUAL INTERNATIONAL LASER PHYSICS WORKSHOP, (Sofia,Bulgaria, 2014.07.16).<\/li>\n<li><span class=\"underline\">K.Shigaki<\/span>, &ldquo;Next Stages of PHENIX forEnhanced Physics with Jets, Quarkonia, and Photons&rdquo;, Asian Triangle HeavyIon Conference 2014 (Osaka, Japan, 2014.8.5-8).<\/li>\n<li><span class=\"underline\">K.Homma<\/span>, &ldquo;Quantum Optics in theVacuum&rdquo;, 3rd International Conference on New Frontiers in Physics,(Crete, Greece, 2014.08.05).<\/li>\n<li><span class=\"underline\">T.Sugitate<\/span>, &ldquo;ALICE Tier-2 atHiroshima&rdquo;, LHCONE workshop at the 38th APAN Meeting (Nantou, Taiwan,2014.8.11-15).<\/li>\n<li><span class=\"underline\">K.Homma<\/span>, &ldquo;A strategy of searching fordark fields via resonances coupling to two photons with high-intensitylaser facilities&rdquo;, IZEST ELI-NP Conference \"Extreme Light's NewHorizons\", (Embassy of Romania, Paris, France, 2014.09.18).<\/li>\n<li><span class=\"underline\">K.Homma<\/span>, &ldquo;HPLS TDR3&rdquo;, ELI-NP ScienceProgram and Instruments: Technical Design Reports, (Bucharest-Magurele,Romania, 2015.02.18).<\/li>\n<li><span class=\"underline\">K.Shigaki<\/span>, &ldquo;Search for IntenseMagnetic Field via Di-Electron Asymmetry in Pb-Pb Collisions at\u221as<sub>NN<\/sub> = 2.76 TeV with ALICE at LHC&rdquo; (poster), Quark Matter 2014(Darmstadt, Germany, 2014.5.19-24).<\/li>\n<li><span class=\"underline\">K.Shigaki<\/span>, &ldquo;MFT and Low Mass Di-MuonStatus and Plan&rdquo;, ALICE Japan-France Workshop (St.Maxime, France,2015.3.15-16).<\/li>\n<li><span class=\"underline\">M.Okawa<\/span>; &ldquo;Creutz Ratio in theContinuum Limit&rdquo;, HET-RBRC Symposium, CreutzFest, (4 September-5September, 2014), New York, USA.<\/li>\n<li>D.Kimura, <span class=\"underline\">T.Morozumi,<\/span> H.Umeeda;&ldquo;Study of an anomalous tau lepton decay using chiral Lagrangian withvector mesons&rdquo;, Tau2014 The 13 th International Workshop on Tau leptonPhysics (Sep16 \/2014, RWTH Archen University, Germany) Nuclear andParticle Physics, Proceedings 260 (2015) 75-78, (Elsevier).<\/li>\n<li>D.Kimura, <span class=\"underline\">T.Morozumi,<\/span> H.Umeeda;&ldquo;Isospin violation and intrinsic parity violation of hadronic taulepton decay&rdquo;, Belle II Theory interface Platform (B2TIP) meeting (Oct.31.2014, KEK Tsukuba).<\/li>\n<li>M.Garcia-Perez, A.Gonzalez-Arroyo, M.Koren, and <span class=\"underline\">M.Okawa<\/span>; &ldquo;Glueball masses in 2+1 dimensional SU(N)gauge theories with twisted boundary conditions&rdquo;, PoS LATTICE2014(2014) 059.<\/li>\n<li>M.Garcia-Perez, A.Gonzalez-Arroyo, L.Keegan and <span class=\"underline\">M.Okawa<\/span>; &ldquo;TEK twisted gradient flow runningcoupling&rdquo;, PoS LATTICE2014 (2014) 300.<\/li>\n<li>A.Gonzalez-Arroyo and <span class=\"underline\">M.Okawa<\/span>;&ldquo;Testing volume independence of large N gauge theories on the lattice&rdquo;,PoS LATTICE2014 (2014) 301.<\/li>\n<li>A.Gonzalez-Arroyo and <span class=\"underline\">M.Okawa<\/span>;&ldquo;String tension from smearing and Wilson flow methods&rdquo;, PoS LATTICE2014(2014) 327. .<\/li>\n<li>D.Kimura, <span class=\"underline\">T.Morozumi,<\/span> H.Umeeda;&ldquo;Chiral Lagrangian with vector mesons, power counting with chiralbreaking&rdquo;, Hadron and Hadron interactions in QCD 2015 \u2013 effectivetheories and lattice \u2013 Yukawa Institute (Feb.19th, 2015, KyotoUniversirty).<\/li>\n<li>Y.Murakami, <span class=\"underline\">K-I.Ishikawa<\/span>; &ldquo;Aconstruction of the Schr\u00f6dinger Functional for M\u00f6bius Domain WallFermions,&rdquo; PoS LATTICE2014 (2014) 331, 32nd Inter. Sym. on LatticeField Theory (Lattice 2014) (June 23-28, 2014, Brookhaven, NY, USA).<\/li>\n<li><span class=\"underline\">K-I.Ishikawa<\/span>, Y.Murakami; &ldquo;Mebiusdomainwall fermion with the Schroedinger functional scheme&rdquo;,Mini-workshop on QCD, (2014\u5e7411\u670824\u65e5, Institute of Physics, AcademiaSinica, Taiwan).<\/li>\n<li>N.Ishizuka, <span class=\"underline\">K.I.Ishikawa<\/span>, A.Ukawa,T.Yoshi\u00e9; &ldquo;Calculation of K\u2192\u03c0\u03c0 decay amplitudes with improved Wilsonfermion in 2+1 flavor lattice QCD&rdquo;, PoS LATTICE2014 (2014) 364, 32ndInter. Sym. on Lattice Field Theory (Lattice 2014) (June 23-28, 2014,Brookhaven, NY, USA).<\/li>\n<li><span class=\"underline\">\u6c34\u91ce\u6052\u53f2<\/span>\uff1a&rdquo;Synergy of Gamma-ray andmm-Radio Observations in Studying Molecular Clouds&rdquo;,\u91ce\u8fba\u5c71\u30e6\u30fc\u30b6\u30fc\u30ba\u30df\u30fc\u30c6\u30a3\u30f3\u30b0\uff082014\u5e746\u670823\u65e5,\u91ce\u8fba\u5c71\uff09.<\/li>\n<li><span class=\"underline\">\u6c34\u91ce\u6052\u53f2<\/span>\uff1a&rdquo;Soft Gamma-ray Polarimetrywith ASTRO-H SGD&rdquo;, \u9ad8\u5b87\u9023\u5c06\u6765\u8a08\u753b\u30b7\u30f3\u30dd\u30b8\u30a6\u30e0\uff082014\u5e748\u670823-24\u65e5,\u5b87\u5b99\u7814\uff09.<\/li>\n<li>\u4f0a\u85e4\u4eae\u4ecb\uff1a\u300c\u5927\u5b66\u9593\u9023\u643a\u306b\u3088\u308bAGN\u30b8\u30a7\u30c3\u30c8\u306e\u591a\u6ce2\u9577\u89b3\u300d, \u65e5\u672c\u5929\u6587\u5b66\u4f1a2014\u5e74\u79cb\u5b63\u5e74\u4f1a\uff089\u670811-13\u65e5,\u5c71\u5f62\u5927\u5b66\u5c0f\u767d\u5ddd\u30ad\u30e3\u30f3\u30d1\u30b9\uff09.<\/li>\n<li>\u79cb\u7530\u8c37\u6d0b\uff1a\u300c\u5149\u8d64\u5916\u7dda\u5927\u5b66\u9593\u9023\u643a\u89b3\u6e2c\u306e\u5186\u6ed1\u306a\u9042\u884c\u306b\u5411\u3051\u305f\u74b0\u5883\u6574\u5099\u300d,\u65e5\u672c\u5929\u6587\u5b66\u4f1a2014\u5e74\u79cb\u5b63\u5e74\u4f1a\uff089\u670811-13\u65e5,\u5c71\u5f62\u5927\u5b66\u5c0f\u767d\u5ddd\u30ad\u30e3\u30f3\u30d1\u30b9\uff09.<\/li>\n<li><span class=\"underline\">\u6c34\u91ce\u6052\u53f2<\/span>\uff1a\u300cGeV\u30ac\u30f3\u30de\u7dda\u89b3\u6e2c\u306b\u3088\u308b\u661f\u9593\u30ac\u30b9\u30fb\u5b87\u5b99\u7dda\u7814\u7a76\u306e\u73fe\u72b6\u300d,\u65e5\u672c\u5929\u6587\u5b66\u4f1a2014\u5e74\u79cb\u5b63\u5e74\u4f1a\uff089\u670811-13\u65e5,\u5c71\u5f62\u5927\u5b66\u5c0f\u767d\u5ddd\u30ad\u30e3\u30f3\u30d1\u30b9\uff09.<\/li>\n<li><span class=\"underline\">\u6c34\u91ce\u6052\u53f2<\/span>\uff1a&rdquo;Dark Matter Search with FermiLarge Area Telescope&rdquo; , \u8d85\u9ad8\u30a8\u30cd\u30eb\u30ae\u30fc\u30ac\u30f3\u30de\u7dda\u3067\u898b\u308b\u6975\u9650\uff082014\u5e7411\u67082-3\u65e5,\u5b87\u5b99\u7dda\u7814\u7a76\u6240\uff09.<\/li>\n<li>\u7530\u4e2d\u5eb7\u4e4b\uff1a\u300cRecent Fermi-LAT results of Active GalacticNuclei\u300d\u8d85\u9ad8\u30a8\u30cd\u30eb\u30ae\u30fc\u30ac\u30f3\u30de\u7dda\u3067\u898b\u308b\u6975\u9650\uff082014\u5e7411\u67082-3\u65e5,\u5b87\u5b99\u7dda\u7814\u7a76\u6240\uff09.<\/li>\n<li><span class=\"underline\">\u6c34\u91ce\u6052\u53f2<\/span>\uff1a&rdquo;Galactic Cosmic Rays Seen byFermi LAT&rdquo; , \u4eca\u5f8c10\u5e74\u306e\u5b87\u5b99\u7dda\u7814\u7a76\uff082014\u5e7411\u67086\u65e5,\u5b87\u5b99\u7dda\u7814\u7a76\u6240\uff09.<\/li>\n<li>\u7530\u4e2d\u5eb7\u4e4b\uff1a\u300c\u30ac\u30f3\u30de\u7dda\u30d6\u30ec\u30fc\u30b6\u30fc\u300d,\u4eca\u5f8c10\u5e74\u306e\u5b87\u5b99\u7dda\u7814\u7a76\uff082014\u5e7411\u670806\u65e5,\u5b87\u5b99\u7dda\u7814\u7a76\u6240\uff09.<\/li>\n<li>\u7530\u4e2d\u5eb7\u4e4b\uff1a\u300c\u30d5\u30a7\u30eb\u30df\u885b\u661f\u306b\u3088\u308b\u6d3b\u52d5\u9280\u6cb3\u6838\u30b8\u30a7\u30c3\u30c8\u306e\u6700\u8fd1\u306e\u7d50\u679c\u3068\u4eca\u5f8c\u306e\u9023\u643a\u89b3\u6e2c\u306e\u5c55\u671b\u300d,2014\u5e74\u5ea6\u9ad8\u5b87\u9023\u7814\u7a76\u4f1a\uff082015\u5e743\u67089-11\u65e5,\u5e83\u5cf6\u5927\u5b66\uff09.<\/li>\n<li><span class=\"underline\">\u6df1\u6ca2\u6cf0\u53f8<\/span>\uff1a\u300cGeV\u30ac\u30f3\u30de\u7dda\u89b3\u6e2c\uff08Fermi\u30ac\u30f3\u30de\u7dda\u5b87\u5b99\u671b\u9060\u93e1\uff09\u3068CTA\u300d,\u65e5\u672c\u5929\u6587\u5b66\u4f1a2015\u5e74\u6625\u5b63\u5e74\u4f1a\uff082015\u5e743\u670821-24\u65e5,\u5927\u962a\u5927\u5b66\u8c4a\u4e2d\u30ad\u30e3\u30f3\u30d1\u30b9\uff09.<\/li>\n<li><span class=\"underline\">\u6df1\u6ca2\u6cf0\u53f8<\/span>\uff1a\u300c\u3059\u3056\u304f\u885b\u661f\u306b\u3088\u308b\u6d3b\u52d5\u9280\u6cb3\u6838\u306e\u786cX\u7dda\u8edf\u30ac\u30f3\u30de\u7dda\u30b9\u30da\u30af\u30c8\u30eb\u306e\u6642\u9593\u5909\u52d5\u300d\u65e5\u672c\u5929\u6587\u5b66\u4f1a2014\u5e74\u79cb\u5b63\u5e74\u4f1a\uff082014\u5e749\u670811-13\u65e5,\u5c71\u5f62\u5927\u5b66\u5c0f\u767d\u5ddd\u30ad\u30e3\u30f3\u30d1\u30b9\uff09.<\/li>\n<li><span class=\"underline\">\u9ad8\u6a4b\u5f18\u5145<\/span>\uff1a\u300cPoGOLite\u6c17\u7403\u5b9f\u9a13:2013\u5e74\u306e\u30d1\u30b9\u30d5\u30a1\u30a4\u30f3\u30f3\u30c0\u30fc\u30d5\u30e9\u30a4\u30c8(2)\u300d\u65e5\u672c\u5929\u6587\u5b66\u4f1a2014\u5e74\u79cb\u5b63\u5e74\u4f1a\uff082014\u5e749\u670811-13\u65e5,\u5c71\u5f62\u5927\u5b66\u5c0f\u767d\u5ddd\u30ad\u30e3\u30f3\u30d1\u30b9\uff09.<\/li>\n<li>\u7530\u4e2d\u5eb7\u4e4b\uff1a\u300c\u5149\u8d64\u5916\u5927\u5b66\u9593\u9023\u643a\u3068\u304b\u306a\u305f\u671b\u9060\u93e1\u306b\u3088\u308b Narrow Line Seyfert 1 Galaxy1H~0323+342\u306e\u53ef\u8996\u89b3\u6e2c\u300d\u65e5\u672c\u5929\u6587\u5b66\u4f1a2014\u5e74\u79cb\u5b63\u5e74\u4f1a\uff082014\u5e749\u670811-13\u65e5,\u5c71\u5f62\u5927\u5b66\u5c0f\u767d\u5ddd\u30ad\u30e3\u30f3\u30d1\u30b9\uff09.<\/li>\n<li>\u7530\u4e2d\u5eb7\u4e4b\uff1a\u300c\u3059\u3056\u304f\u885b\u661f\u306b\u3088\u308b Centaurus~A NorthernLobe\u306eX\u7dda\u89b3\u6e2c\u300d\u65e5\u672c\u5929\u6587\u5b66\u4f1a2014\u5e74\u79cb\u5b63\u5e74\u4f1a\uff082014\u5e749\u670811-13\u65e5,\u5c71\u5f62\u5927\u5b66\u5c0f\u767d\u5ddd\u30ad\u30e3\u30f3\u30d1\u30b9\uff09.<\/li>\n<li>\u52dd\u7530\u96bc\u4e00\u90ce,\uff1a\u300c\u30d5\u30a7\u30eb\u30df\u30fb\u30ac\u30f3\u30de\u7dda\u5b87\u5b99\u671b\u9060\u93e1\u306b\u3088\u308bG25.0+0.0\u9818\u57df\u304b\u3089\u306e\u5e83\u304c\u3063\u305f\u30ac\u30f3\u30de\u7dda\u653e\u5c04\u306e\u89b3\u6e2c\u300d\u65e5\u672c\u5929\u6587\u5b66\u4f1a2014\u5e74\u79cb\u5b63\u5e74\u4f1a\uff082014\u5e749\u670811-13\u65e5,\u5c71\u5f62\u5927\u5b66\u5c0f\u767d\u5ddd\u30ad\u30e3\u30f3\u30d1\u30b9\uff09.<\/li>\n<li>\u6cb3\u91ce\u8cb4\u6587\uff1a\u300c\u53cd\u5c04\u6210\u5206\u304c\u5353\u8d8a\u3057\u305f\u6d3b\u52d5\u9280\u6cb3\u6838 NGC6552\u306e\u300c\u3059\u3056\u304f\u300d\u306b\u3088\u308b\u89b3\u6e2c\u300d\u65e5\u672c\u5929\u6587\u5b66\u4f1a2014\u5e74\u79cb\u5b63\u5e74\u4f1a\uff082014\u5e749\u670811-13\u65e5,\u5c71\u5f62\u5927\u5b66\u5c0f\u767d\u5ddd\u30ad\u30e3\u30f3\u30d1\u30b9\uff09.<\/li>\n<li>\u6cb3\u53e3\u8ce2\u81f3\uff1a\u300c\u304b\u306a\u305f\u671b\u9060\u93e1\u306b\u3088\u308b\u6d3b\u52d5\u9280\u6cb3\u6838\u306e\u53ef\u8996\u5149\u30fbX\u7dda\u30fb\u30ac\u30f3\u30de\u7dda\u3067\u306e\u76f8\u95a2\u306e\u63a2\u67fb\u300d\u65e5\u672c\u5929\u6587\u5b66\u4f1a2014\u5e74\u79cb\u5b63\u5e74\u4f1a\uff082014\u5e749\u670811-13\u65e5,\u5c71\u5f62\u5927\u5b66\u5c0f\u767d\u5ddd\u30ad\u30e3\u30f3\u30d1\u30b9\uff09.<\/li>\n<li>\u53e4\u4e95\u4fca\u4e5f\uff1a\u300c\u30d5\u30ec\u30fc\u30e0\u30ef\u30fc\u30afMONACO\u3092\u7528\u3044\u305f\u6d3b\u52d5\u9280\u6cb3\u6838\u30c8\u30fc\u30e9\u30b9\u306eX\u7dda\u30b9\u30da\u30af\u30c8\u30eb\u30b7\u30df\u30e5\u30ec\u30fc\u30b7\u30e7\u30f3\u300d\u65e5\u672c\u5929\u6587\u5b66\u4f1a2014\u5e74\u79cb\u5b63\u5e74\u4f1a\uff082014\u5e749\u670811-13\u65e5,\u5c71\u5f62\u5927\u5b66\u5c0f\u767d\u5ddd\u30ad\u30e3\u30f3\u30d1\u30b9\uff09.<\/li>\n<li>\u679d\u5ee3\u80b2\u5b9f\uff1a\u300cX\u7dda\u9244\u8f1d\u7dda\u5171\u9cf4\u6563\u4e71\u3092\u7528\u3044\u305f\u9280\u6cb3\u56e3\u5185\u9ad8\u6e29\u30d7\u30e9\u30ba\u30de\u3067\u306e\u4e71\u6d41\u306e\u5927\u304d\u3055\u306e\u5236\u9650\u300d\u65e5\u672c\u5929\u6587\u5b66\u4f1a2014\u5e74\u79cb\u5b63\u5e74\u4f1a\uff082014\u5e749\u670811-13\u65e5,\u5c71\u5f62\u5927\u5b66\u5c0f\u767d\u5ddd\u30ad\u30e3\u30f3\u30d1\u30b9\uff09.<\/li>\n<li>\u767d\u5ddd\u88d5\u7ae0\uff1a\u300c\u3059\u3056\u304f\u885b\u661f\u306b\u3088\u308bradio-loud\u306a\u72ed\u8f1d\u7dda\u30bb\u30a4\u30d5\u30a1\u30fc\u30c81\u578b\u9280\u6cb31H~0323+342\u306eX\u7dda\u89b3\u6e2c\u300d\u65e5\u672c\u5929\u6587\u5b66\u4f1a2014\u5e74\u79cb\u5b63\u5e74\u4f1a\uff082014\u5e749\u670811-13\u65e5,\u5c71\u5f62\u5927\u5b66\u5c0f\u767d\u5ddd\u30ad\u30e3\u30f3\u30d1\u30b9\uff09.<\/li>\n<li>\u4e2d\u5ca1\u7adc\u4e5f\uff1a\u300cMPPC\u3068\u30d7\u30e9\u30b9\u30c1\u30c3\u30af\u30b7\u30f3\u30c1\u30ec\u30fc\u30bf\u306e\u7d44\u307f\u5408\u308f\u305b\u3092\u7528\u3044\u305f\u5929\u4f53\u504f\u5149X\u7dda\u691c\u51fa\u5668\u306e\u691c\u8a0e\u300d\u65e5\u672c\u5929\u6587\u5b66\u4f1a2014\u5e74\u79cb\u5b63\u5e74\u4f1a\uff082014\u5e749\u670811-13\u65e5,\u5c71\u5f62\u5927\u5b66\u5c0f\u767d\u5ddd\u30ad\u30e3\u30f3\u30d1\u30b9\uff09.<\/li>\n<li>\u68ee\u8c37\u53cb\u7531\u5e0c\uff1a\u300cTeV \u03b3\u7dda\u9023\u661fHESSJ0632+057\u306b\u304a\u3051\u308b\u9060\u661f\u70b9\u5f8c\u306e\u76f8\u4e92\u4f5c\u7528\u300d\u65e5\u672c\u5929\u6587\u5b66\u4f1a2014\u5e74\u79cb\u5b63\u5e74\u4f1a\uff082014\u5e749\u670811-13\u65e5,\u5c71\u5f62\u5927\u5b66\u5c0f\u767d\u5ddd\u30ad\u30e3\u30f3\u30d1\u30b9\uff09.<\/li>\n<li><span class=\"underline\">\u5ddd\u7aef\u5f18\u6cbb<\/span>\uff1a\u300c\u8fd1\u508d\u9280\u6cb3M82\u306b\u73fe\u308c\u305f\u8d64\u5316\u306e\u5927\u304d\u306aIa\u578b\u8d85\u65b0\u661fSN2014J\u306e\u504f\u5149\u7279\u6027\u300d\u65e5\u672c\u5929\u6587\u5b66\u4f1a2014\u5e74\u79cb\u5b63\u5e74\u4f1a\uff082014\u5e749\u670811-13\u65e5,\u5c71\u5f62\u5927\u5b66\u5c0f\u767d\u5ddd\u30ad\u30e3\u30f3\u30d1\u30b9\uff09.<\/li>\n<li>\u5185\u6d77\u6d0b\u8f14\uff1a\u300c\u30c1\u30d9\u30c3\u30c8\u30ed\u30dc\u30c3\u30c8\u4e09\u8272\u64ae\u50cf\u30ab\u30e1\u30e9\uff08HinOTORI\uff09\uff1a\u4ed5\u69d8\u8a55\u4fa1\u300d\u65e5\u672c\u5929\u6587\u5b66\u4f1a2014\u5e74\u79cb\u5b63\u5e74\u4f1a\uff082014\u5e749\u670811-13\u65e5,\u5c71\u5f62\u5927\u5b66\u5c0f\u767d\u5ddd\u30ad\u30e3\u30f3\u30d1\u30b9\uff09.<\/li>\n<li>\u79cb\u7530\u8c37\u6d0b\uff1a\u300c\u53ef\u8996\u8d64\u5916\u7dda\u540c\u6642\u30ab\u30e1\u30e9HONIR\uff1a\u76f4\u7dda\u504f\u5149\u89b3\u6e2c\u6a5f\u80fd\u306e\u5c0e\u5165\u3068\u6027\u80fd\u8a55\u4fa1\u300d\u65e5\u672c\u5929\u6587\u5b66\u4f1a2014\u5e74\u79cb\u5b63\u5e74\u4f1a\uff082014\u5e749\u670811-13\u65e5,\u5c71\u5f62\u5927\u5b66\u5c0f\u767d\u5ddd\u30ad\u30e3\u30f3\u30d1\u30b9\uff09.<\/li>\n<li><span class=\"underline\">\u5409\u7530\u9053\u5229<\/span>\uff1a\u300c\u30b9\u30bf\u30fc\u30d0\u30fc\u30b9\u30c8\u9280\u6cb3M82\u306e\u30b9\u30fc\u30d1\u30fc\u30a6\u30a3\u30f3\u30c9\u504f\u5149\u5206\u5149\u89b3\u6e2c\u306b\u3088\u308b\u30c0\u30b9\u30c8\u30d5\u30ed\u30fc\u306e\u7814\u7a76 II.\u300d\u65e5\u672c\u5929\u6587\u5b66\u4f1a2014\u5e74\u79cb\u5b63\u5e74\u4f1a\uff082014\u5e749\u670811-13\u65e5,\u5c71\u5f62\u5927\u5b66\u5c0f\u767d\u5ddd\u30ad\u30e3\u30f3\u30d1\u30b9\uff09.<\/li>\n<li>\u5317\u53e3\u8cb4\u96c4\uff1a\u300cSPring-8\u306b\u3088\u308b\u30de\u30a4\u30af\u30ed\u30d1\u30bf\u30fc\u30f3\u30ac\u30b9\u504f\u5149\u8a08\u306e\u8a73\u7d30\u306a\u6027\u80fd\u8a55\u4fa1\u300d\u65e5\u672c\u5929\u6587\u5b66\u4f1a2015\u5e74\u6625\u5b63\u5e74\u4f1a\uff082015\u5e743\u670818-21\u65e5,\u5927\u962a\u5927\u5b66\u8c4a\u4e2d\u30ad\u30e3\u30f3\u30d1\u30b9\uff09.<\/li>\n<li>\u53e4\u4e95\u4fca\u4e5f\uff1a\u300c\u30d5\u30ec\u30fc\u30e0\u30ef\u30fc\u30afMONACO\u3092\u7528\u3044\u305f\u6d3b\u52d5\u9280\u6cb3\u6838\u30c8\u30fc\u30e9\u30b9\u306eX\u7dda\u30b9\u30da\u30af\u30c8\u30eb\u30b7\u30df\u30e5\u30ec\u30fc\u30b7\u30e7\u30f32\u300d\u65e5\u672c\u5929\u6587\u5b66\u4f1a2015\u5e74\u6625\u5b63\u5e74\u4f1a\uff082015\u5e743\u670818-21\u65e5,\u5927\u962a\u5927\u5b66\u8c4a\u4e2d\u30ad\u30e3\u30f3\u30d1\u30b9\uff09.<\/li>\n<li>\u679d\u5ee3\u80b2\u5b9f\uff1a\u300cASTRO-H\u885b\u661f\u642d\u8f09\u8edf\u30ac\u30f3\u30de\u7dda\u691c\u51fa\u5668(SGD)\u306e\u642d\u8f09\u54c1\u3092\u7528\u3044\u305f\u8ecc\u9053\u4e0a\u74b0\u5883\u3067\u306e\u52d5\u4f5c\u691c\u8a3c\u300d\u65e5\u672c\u5929\u6587\u5b66\u4f1a2015\u5e74\u6625\u5b63\u5e74\u4f1a\uff082015\u5e743\u670818-21\u65e5,\u5927\u962a\u5927\u5b66\u8c4a\u4e2d\u30ad\u30e3\u30f3\u30d1\u30b9\uff09.<\/li>\n<li><span class=\"underline\">\u6c34\u91ce\u6052\u53f2<\/span>\uff1a\u300c\u3059\u3056\u304f\u300d\u306b\u3088\u308b\u767d\u9ce5\u5ea7\u306b\u767a\u898b\u3055\u308c\u305f\u30ac\u30f3\u30de\u7dda\u8d85\u904e\u306eX\u7dda\u63a2\u67fb(2)\u300d\u65e5\u672c\u5929\u6587\u5b66\u4f1a2015\u5e74\u6625\u5b63\u5e74\u4f1a\uff082015\u5e743\u670818-21\u65e5,\u5927\u962a\u5927\u5b66\u8c4a\u4e2d\u30ad\u30e3\u30f3\u30d1\u30b9\uff09.<\/li>\n<li><span class=\"underline\">\u9ad8\u6a4b\u5f18\u5145<\/span>\uff1a\u300c\u786cX\u7dda\u504f\u5149\u691c\u51fa\u5668PoGOLite\u6c17\u7403\u5b9f\u9a13\uff1a2016\u5e74\u306e\u518d\u30d5\u30e9\u30a4\u30c8\u3078\u5411\u3051\u3066\u300d\u65e5\u672c\u5929\u6587\u5b66\u4f1a2015\u5e74\u6625\u5b63\u5e74\u4f1a\uff082015\u5e743\u670818-21\u65e5,\u5927\u962a\u5927\u5b66\u8c4a\u4e2d\u30ad\u30e3\u30f3\u30d1\u30b9\uff09.<\/li>\n<li><span class=\"underline\">\u5927\u91ce\u96c5\u529f<\/span>\uff1a\u300cASTRO-H\u885b\u661f\u642d\u8f09\u786cX\u7dda\u8edf\u30ac\u30f3\u30de\u7dda\u691c\u51fa\u5668\u306b\u304a\u3051\u308bBGO\u30a2\u30af\u30c6\u30a3\u30d6\u30b7\u30fc\u30eb\u30c9\u306e\u5730\u4e0a\u8f03\u6b63\u8a66\u9a13\u300d\u65e5\u672c\u5929\u6587\u5b66\u4f1a2015\u5e74\u6625\u5b63\u5e74\u4f1a\uff082015\u5e743\u670818-21\u65e5,\u5927\u962a\u5927\u5b66\u8c4a\u4e2d\u30ad\u30e3\u30f3\u30d1\u30b9\uff09.<\/li>\n<li>\u7530\u4e2d\u5eb7\u4e4b\uff1a\u300c\u30d5\u30a7\u30eb\u30df\u885b\u661f\u306b\u3088\u308bBroad Line Radio Galaxy3C120\u306e\u30e2\u30cb\u30bf\u30fc\u89b3\u6e2c\u3068\u591a\u6ce2\u9577\u30c7\u30fc\u30bf\u306b\u3088\u308bMeV\/GeV\u30ac\u30f3\u30de\u7dda\u653e\u5c04\u4f4d\u7f6e\u3068\u653e\u5c04\u6a5f\u69cb\u306e\u63a2\u67fb\u300d\u65e5\u672c\u5929\u6587\u5b66\u4f1a2015\u5e74\u6625\u5b63\u5e74\u4f1a\uff082015\u5e743\u670818-21\u65e5,\u5927\u962a\u5927\u5b66\u8c4a\u4e2d\u30ad\u30e3\u30f3\u30d1\u30b9\uff09.<\/li>\n<li>\u6cb3\u91ce\u8cb4\u6587\uff1a\u300cTeV \u30ac\u30f3\u30de\u7dda\u9023\u661f HESS J0632+057\u306b\u304a\u3051\u308bBe\u661f\u3068\u30b3\u30f3\u30d1\u30af\u30c8\u5929\u4f53\u306e\u76f8\u4e92\u4f5c\u7528\u300d\u65e5\u672c\u5929\u6587\u5b66\u4f1a2015\u5e74\u6625\u5b63\u5e74\u4f1a\uff082015\u5e743\u670818-21\u65e5,\u5927\u962a\u5927\u5b66\u8c4a\u4e2d\u30ad\u30e3\u30f3\u30d1\u30b9\uff09.<\/li>\n<li>\u767d\u5ddd\u88d5\u7ae0\uff1a\u300c\u65b0\u578bSi-pad\u691c\u51fa\u5668\u306e\u57fa\u790e\u7279\u6027\u6e2c\u5b9a\u304a\u3088\u3073\u6027\u80fd\u8a55\u4fa1\u300d\u65e5\u672c\u5929\u6587\u5b66\u4f1a2015\u5e74\u6625\u5b63\u5e74\u4f1a\uff082015\u5e743\u670818-21\u65e5,\u5927\u962a\u5927\u5b66\u8c4a\u4e2d\u30ad\u30e3\u30f3\u30d1\u30b9\uff09.<\/li>\n<li>\u5185\u6d77\u6d0b\u8f14\uff1a\u300c\u30c1\u30d9\u30c3\u30c8\u30ed\u30dc\u30c3\u30c8\u4e09\u8272\u64ae\u50cf\u30ab\u30e1\u30e9\uff08HinOTORI\uff09\uff1a\u6027\u80fd\u8a55\u4fa1\u300d\u65e5\u672c\u5929\u6587\u5b66\u4f1a2015\u5e74\u6625\u5b63\u5e74\u4f1a\uff082015\u5e743\u670818-21\u65e5,\u5927\u962a\u5927\u5b66\u8c4a\u4e2d\u30ad\u30e3\u30f3\u30d1\u30b9\uff09.<\/li>\n<li><span class=\"underline\">\u690d\u6751\u8aa0<\/span>\uff1a\u300cLASSO\u306b\u57fa\u3065\u3044\u305fIa\u578b\u8d85\u65b0\u661f\u306e\u6975\u5927\u7b49\u7d1a\u306e\u5909\u6570\u9078\u629e\u300d\u65e5\u672c\u5929\u6587\u5b66\u4f1a2015\u5e74\u6625\u5b63\u5e74\u4f1a\uff082015\u5e743\u670818-21\u65e5,\u5927\u962a\u5927\u5b66\u8c4a\u4e2d\u30ad\u30e3\u30f3\u30d1\u30b9\uff09.<\/li>\n<li><span class=\"underline\">\u6df1\u6ca2\u6cf0\u53f8<\/span>\uff1a\u300c\u3059\u3056\u304f\u885b\u661f\u3068\u30d5\u30a7\u30eb\u30df\u885b\u661f\u306b\u3088\u308b\u30ac\u30f3\u30de\u7dda\u96fb\u6ce2\u9280\u6cb3PKS0625-354\u30683C78\u306e\u89b3\u6e2c\u300d\u65e5\u672c\u7269\u7406\u5b66\u4f1a2014\u5e74\u79cb\u5b63\u5e74\u4f1a\uff082014\u5e749\u670818-21\u65e5,\u4f50\u8cc0\u5927\u5b66\u672c\u5e84\u30ad\u30e3\u30f3\u30d1\u30b9\uff09.<\/li>\n<li><span class=\"underline\">\u9ad8\u6a4b\u5f18\u5145<\/span>\uff1a\u300c\u3059\u3056\u304f\u885b\u661f\u306b\u3088\u308b\u5171\u751fX\u7dda\u9023\u661fIGRJ16194-2810\u306e\u89b3\u6e2c\u300d\u65e5\u672c\u7269\u7406\u5b66\u4f1a2014\u5e74\u79cb\u5b63\u5e74\u4f1a\uff082014\u5e749\u670818-21\u65e5,\u4f50\u8cc0\u5927\u5b66\u672c\u5e84\u30ad\u30e3\u30f3\u30d1\u30b9\uff09.<\/li>\n<li><span class=\"underline\">\u9ad8\u6a4b\u5f18\u5145<\/span>\uff1a\u300cPoGOLite\u6c17\u7403\u5b9f\u9a13\u306e2013\u5e74\u30d1\u30b9\u30d5\u30a1\u30a4\u30f3\u30c0\u30fc\u30d5\u30e9\u30a4\u30c8\u306e\u72b6\u6cc1\u30682016\u5e74\u306e\u518d\u30d5\u30e9\u30a4\u30c8\u3078\u5411\u3051\u3066\u300d\u5927\u6c17\u7403\u30b7\u30f3\u30dd\u30b8\u30a6\u30e0\uff082014\u5e7411\u67086-7\u65e5,JAXA\u5b87\u5b99\u79d1\u5b66\u7814\u7a76\u6240\uff09.<\/li>\n<li><span class=\"underline\">\u9ad8\u6a4b\u5f18\u5145<\/span>\uff1a\u300c\u786cX\u7dda\u504f\u5149\u691c\u51fa\u5668 PoGOLite\u6c17\u7403\u5b9f\u9a13\uff1a2016\u5e74\u306e\u518d\u30d5\u30e9\u30a4\u30c8\u3078\u5411\u3051\u3066\u300d\u5b87\u5b99\u79d1\u5b66\u30b7\u30f3\u30dd\u30b8\u30a6\u30e0\uff082015\u5e741\u67086-7\u65e5\uff09.<\/li>\n<li><span class=\"underline\">\u9ad8\u6a4b\u5f18\u5145<\/span>\uff1a\u300cX\u7dda\u30fb\u30ac\u30f3\u30de\u7dda\u306b\u3088\u308b\u5927\u8cea\u91cf\u661f\u9023\u661f\u7cfb\u306e\u89b3\u6e2c\u300d\u5927\u8cea\u91cf\u661f\u306e\u9032\u5316\u30fb\u6d3b\u52d5\u73fe\u8c61\u3068\u661f\u306e\u56de\u8ee2\uff082015\u5e742\u670818-20\u65e5\uff09.<\/li>\n<li><span class=\"underline\">\u6df1\u6ca2\u6cf0\u53f8<\/span>\uff1a\u300cASTRO=H\u642d\u8f09\u8edf\u30ac\u30f3\u30de\u7dda\u691c\u51fa\u5668(SGD)\u306e\u958b\u767a\u73fe\u72b6\u300d\u5b87\u5b99\u79d1\u5b66\u30b7\u30f3\u30dd\u30b8\u30a6\u30e0\uff082015\u5e741\u67087-8\u65e5,ISAS\/JAXA\uff09.<\/li>\n<li>\u5ddd\u7aef\u7f8e\u7a42\uff1a\u300c\u660e\u308b\u3044\u30b7\u30e7\u30c3\u30af\u30d6\u30ec\u30a4\u30af\u30a2\u30a6\u30c8\u304c\u898b\u3089\u308c\u305fIIb \u578b\u8d85\u65b0\u661fSN 2013df\u306e\u6e2c\u5149\u5206\u5149\u89b3\u6e2c\u300d2014\u5e74\u5ea6\u5929\u6587\u30fb\u5929\u4f53\u7269\u7406\u82e5\u624b\u590f\u306e\u5b66\u6821\uff082014\u5e747\u670828-31\u65e5,\u4fe1\u5dde\u30fb\u6238\u5009\u4e0a\u5c71\u7530\u6e29\u6cc9\u30db\u30c6\u30eb\u5713\u5c71\u8358,400\u4eba\uff09.<\/li>\n<li>\u9ad8\u6728\u52dd\u4fca\uff1a\u300cGRB\u521d\u671f\u6b8b\u5149\u306e\u53ef\u8996\u504f\u5149\u89b3\u6e2c\u300d2014\u5e74\u5ea6\u5ca1\u5c71\u30e6\u30fc\u30b6\u30fc\u30ba\u30df\u30fc\u30c6\u30a3\u30f3\u30b0\uff082014\u5e748\u670811-12\u65e5,\u56fd\u7acb\u5929\u6587\u53f0\u4e09\u9df9\u30ad\u30e3\u30f3\u30d1\u30b9,50\u4eba\uff09.<\/li>\n<li>\u4e2d\u5ca1\u7adc\u4e5f\uff1a\u300c\u6771\u5e83\u5cf6\u5929\u6587\u53f0\u306b\u304a\u3051\u308b\u8fd1\u8d64\u5916sky\u8f1d\u5ea6\u306e\u5b63\u7bc0\u5909\u5316\u300d2014\u5e74\u5ea6\u5ca1\u5c71\u30e6\u30fc\u30b6\u30fc\u30ba\u30df\u30fc\u30c6\u30a3\u30f3\u30b0\uff082014\u5e748\u670812-13\u65e5,\u56fd\u7acb\u5929\u6587\u53f0\u4e09\u9df9\u30ad\u30e3\u30f3\u30d1\u30b9,50\u4eba\uff09.<\/li>\n<li>\u5ddd\u7aef\u7f8e\u7a42\uff1a\u300c\u660e\u308b\u3044\u30b7\u30e7\u30c3\u30af\u30d6\u30ec\u30a4\u30af\u30a2\u30a6\u30c8\u304c\u898b\u3089\u308c\u305fIIb\u578b\u8d85\u65b0\u661fSN2013df\u306e\u6e2c\u5149\u5206\u5149\u89b3\u6e2c\u300d2014\u5e74\u5ea6\u5ca1\u5c71\u30e6\u30fc\u30b6\u30fc\u30ba\u30df\u30fc\u30c6\u30a3\u30f3\u30b0\uff082014\u5e748\u670811-12\u65e5,\u56fd\u7acb\u5929\u6587\u53f0\u4e09\u9df9\u30ad\u30e3\u30f3\u30d1\u30b9,50\u4eba\uff09.<\/li>\n<li>\u5b87\u4e95\u5d07\u7d18\uff1a\u300c\u53ef\u8996\u8d64\u5916\u7dda\u540c\u6642\u30ab\u30e1\u30e9HONIR\u306e\u8fd1\u8d64\u5916\u7dda\u8aad\u307f\u51fa\u3057\u30b7\u30b9\u30c6\u30e0\u306e\u958b\u767a\u3068\u8a55\u4fa1\u300d2014\u5e74\u5ea6\u5ca1\u5c71\u30e6\u30fc\u30b6\u30fc\u30ba\u30df\u30fc\u30c6\u30a3\u30f3\u30b0\uff082014\u5e748\u670811-12\u65e5,\u56fd\u7acb\u5929\u6587\u53f0\u4e09\u9df9\u30ad\u30e3\u30f3\u30d1\u30b9,50\u4eba\uff09.<\/li>\n<li>\u9ad8\u7530\u7d18\u53f8\uff1a\u300c128\u00d7128\u753b\u7d20InGaAs\u8fd1\u8d64\u5916\u7dda\u691c\u51fa\u5668\u306e\u51b7\u5374\u4e0b\u3067\u306e\u6027\u80fd\u8a55\u4fa1\u300d2014\u5e74\u5ea6\u5ca1\u5c71\u30e6\u30fc\u30b6\u30fc\u30ba\u30df\u30fc\u30c6\u30a3\u30f3\u30b0\uff082014\u5e748\u670811-12\u65e5,\u56fd\u7acb\u5929\u6587\u53f0\u4e09\u9df9\u30ad\u30e3\u30f3\u30d1\u30b9,50\u4eba\uff09.<\/li>\n<li>\u6cb3\u53e3\u8ce2\u81f3\uff1a\u300c\u304b\u306a\u305f\u671b\u9060\u93e1\u306b\u3088\u308b\u6d3b\u52d5\u9280\u6cb3\u6838\u306e\u53ef\u8996\u5149\u30fbX\u7dda\u30fb\u30ac\u30f3\u30de\u7dda\u3067\u306e\u76f8\u95a2\u306e\u63a2\u67fb\u300d2014\u5e74\u5ea6\u5ca1\u5c71\u30e6\u30fc\u30b6\u30fc\u30ba\u30df\u30fc\u30c6\u30a3\u30f3\u30b0\uff082014\u5e748\u670811-12\u65e5,\u56fd\u7acb\u5929\u6587\u53f0\u4e09\u9df9\u30ad\u30e3\u30f3\u30d1\u30b9,50\u4eba\uff09.<\/li>\n<li>\u795e\u7530\u512a\u82b1\uff1a\u300c\u304b\u306a\u305f\u671b\u9060\u93e1\u3092\u4f7f\u3063\u305f\u53ef\u8996\u30fb\u8fd1\u8d64\u5916\u9818\u57df\u306b\u308f\u305f\u308bX\u7dda\u9023\u661f\u306e\u504f\u5149\u89b3\u6e2c\u300d2014\u5e74\u5ea6\u5ca1\u5c71\u30e6\u30fc\u30b6\u30fc\u30ba\u30df\u30fc\u30c6\u30a3\u30f3\u30b0\uff082014\u5e748\u670811-12\u65e5,\u56fd\u7acb\u5929\u6587\u53f0\u4e09\u9df9\u30ad\u30e3\u30f3\u30d1\u30b9,50\u4eba\uff09.<\/li>\n<li><span class=\"underline\">\u690d\u6751\u8aa0<\/span>\uff1a\u300c\u304b\u306a\u305f\u671b\u9060\u93e1\u30fb\u89b3\u6e2c\u88c5\u7f6e\u4f7f\u7528\u72b6\u6cc1\u300d2014\u5e74\u5ea6\u5ca1\u5c71\u30e6\u30fc\u30b6\u30fc\u30ba\u30df\u30fc\u30c6\u30a3\u30f3\u30b0\uff082014\u5e748\u670811-12\u65e5,\u56fd\u7acb\u5929\u6587\u53f0\u4e09\u9df9\u30ad\u30e3\u30f3\u30d1\u30b9,50\u4eba\uff09.<\/li>\n<li>\u5b87\u4e95\u5d07\u7d18\uff1a\u300c\u53ef\u8996\u8d64\u5916\u540c\u6642\u30ab\u30e1\u30e9HONIR\u306e\u8fd1\u8d64\u5916\u7dda\u691c\u51fa\u5668\u8aad\u307f\u51fa\u3057\u30b7\u30b9\u30c6\u30e0\u306e\u958b\u767a\u3068\u8a55\u4fa1\u300d\u7b2c\uff14\u56de\u53ef\u8996\u8d64\u5916\u7dda\u89b3\u6e2c\u88c5\u7f6e\u6280\u8853\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d7\uff082014\u5e7412\u67083-4\u65e5,\u56fd\u7acb\u5929\u6587\u53f0\u4e09\u9df9\u30ad\u30e3\u30f3\u30d1\u30b9,50\u4eba\uff09.<\/li>\n<li>\u9ad8\u6728\u52dd\u4fca\uff1a\u300c\u304b\u306a\u305f\u671b\u9060\u93e1\u3067\u306eGRB\u89b3\u6e2c\u300d\u7b2c5\u56de\u5927\u5b66\u9593\u9023\u643a\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d7\uff082015\u5e741\u67087-8\u65e5,\u6771\u4eac\u5de5\u696d\u5927\u5b66,50\u4eba\uff09.<\/li>\n<li>\u4e2d\u5ca1\u7adc\u4e5f\uff1a\u300c\u6771\u5e83\u5cf6\u5929\u6587\u53f0\u306b\u304a\u3051\u308b\u8fd1\u8d64\u5916\u9650\u754c\u7b49\u7d1a\u306e\u5b63\u7bc0\u5909\u5316\u300d\u7b2c5\u56de\u5927\u5b66\u9593\u9023\u643a\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d7\uff082015\u5e741\u67087-8\u65e5,\u6771\u4eac\u5de5\u696d\u5927\u5b66,50\u4eba\uff09.<\/li>\n<li>\u5ddd\u7aef\u7f8e\u7a42\uff1a\u300c\u660e\u308b\u3044\u30b7\u30e7\u30c3\u30af\u30d6\u30ec\u30a4\u30af\u30a2\u30a6\u30c8\u304c\u898b\u3089\u308c\u305fSN2013df\u306e\u53ef\u8996\u89b3\u6e2c\u300d\u7b2c5\u56de\u5927\u5b66\u9593\u9023\u643a\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d7\uff082015\u5e741\u67087-8\u65e5,\u6771\u4eac\u5de5\u696d\u5927\u5b66,50\u4eba\uff09.<\/li>\n<li>\u5927\u6a4b\u4f51\u99ac\uff1a\u300c\u521d\u3081\u3066\u5f97\u3089\u308c\u305fSS433\u306e\u53ef\u8996\u504f\u5149\u30b9\u30da\u30af\u30c8\u30eb\u300d\u7b2c20\u56de\u5929\u4f53\u30b9\u30da\u30af\u30c8\u30eb\u7814\u7a76\u4f1a\uff082015\u5e743\u67087-8\u65e5,\u6d45\u53e3\u5e02\u5065\u5eb7\u798f\u7949\u30bb\u30f3\u30bf\u30fc,\u53c2\u52a0\u4eba\u657040\u540d\uff09.<\/li>\n<li><span class=\"underline\">\u690d\u6751\u8aa0<\/span>\uff1a\u300cIa\u578b\u8d85\u65b0\u661f\u306e\u6975\u5927\u7b49\u7d1a\u306e\u5909\u6570\u9078\u629e\u300d\u5929\u6587\u5b66\u30fb\u5b87\u5b99\u7269\u7406\u5b66\u3068\u30b9\u30d1\u30fc\u30b9\u30e2\u30c7\u30ea\u30f3\u30b0\uff082014\u5e7411\u670819-20\u65e5,\u4eac\u90fd\u5927\u5b66\uff09.<\/li>\n<li><span class=\"underline\">\u690d\u6751\u8aa0<\/span>\uff1a\u300c\u30b9\u30d1\u30fc\u30b9\u30e2\u30c7\u30ea\u30f3\u30b0\u306e\u5b87\u5b99\u7269\u7406\u5b66\u3078\u306e\u5fdc\u7528\u300d\u56fd\u7acb\u5929\u6587\u53f0\u8ac7\u8a71\u4f1a\uff082014\u5e745\u670823\u65e5,\u56fd\u7acb\u5929\u6587\u53f0\u4e09\u9df9\uff09.<\/li>\n<li><span class=\"underline\">\u5c0f\u5d8c\u5eb7\u53f2<\/span>\uff1a\u300c\u78c1\u6c17\u661f\u306e\u8ef8\u6027\u3068\u6975\u6027\u65b9\u5411\u632f\u52d5\u306e\u6642\u9593\u767a\u5c55\u306b\u3088\u308b\u6570\u5024\u89e3\u6790\u300d\u65e5\u672c\u5929\u6587\u5b66\u4f1a\u79cb\u5b63\u5e74\u4f1a\uff089\u67089-12\u65e5,\u5c71\u5f62\u5927\u5b66\uff09.<\/li>\n<li>\u7167\u559c\u540d\u6b69,<span class=\"underline\">\u5c71\u672c\u4e00\u535a<\/span>\uff1a\u300c\u4e00\u822c\u5316\u3055\u308c\u305f\u30ac\u30ea\u30ec\u30aa\u30f3\u91cd\u529b\u6a21\u578b\u306b\u5bfe\u3059\u308b\u9280\u6cb3\u56e3\u306e\u30ac\u30b9\u3068\u30b7\u30a2\u30fc  \u30d7\u30ed\u30d5\u30a1\u30a4\u30eb\u3092\u7d44\u307f\u5408\u308f\u305b\u305f\u89b3\u6e2c\u7684\u5236\u9650\u300d\u65e5\u672c\u7269\u7406\u5b66\u4f1a2014\u5e74\u79cb\u5b63\u5927\u4f1a\uff089\u670819\u65e5,\u4f50\u8cc0\u5927\u5b66\uff09.<\/li>\n<li>\u5927\u4e0b\u7fd4\u8a89,<span class=\"underline\">\u5c71\u672c\u4e00\u535a<\/span>,\u5f35\u68ee\uff1a\u300c\u771f\u7a7a\u306e\u91cf\u5b50\u63fa\u3089\u304e\u3068\u76f8\u4e92\u4f5c\u7528\u3059\u308b\u7c92\u5b50\u306e\u30e9\u30f3\u30c0\u30e0\u904b\u52d5\u306b\u304a\u3051\u308b\u71b1\u7684\u6027\u8cea\u300d\u65e5\u672c\u7269\u7406\u5b66\u4f1a2014\u5e74\u79cb\u5b63\u5927\u4f1a\uff089\u670820\u65e5,\u4f50\u8cc0\u5927\u5b66\uff09.<\/li>\n<li><span class=\"underline\">\u5c0f\u5d8c\u5eb7\u53f2<\/span>\uff1a\u300c\u30d6\u30e9\u30c3\u30af\u30db\u30fc\u30eb\u78c1\u6c17\u570f\u306e\u56de\u8ee2\u99c6\u52d5\u306b\u3088\u308b\u96fb\u6d41\u3068\u96fb\u8377\u306e\u5206\u5e03\u69cb\u9020\u300d\u65e5\u672c\u5929\u6587\u5b66\u4f1a\u6625\u5b63\u5e74\u4f1a\uff082015\u5e743\u670818-21\u65e5,\u5927\u962a\u5927\u5b66\uff09.<\/li>\n<li><span class=\"underline\">\u6749\u7acb \u5fb9<\/span>\uff1a\u300cLHC-ALICE\u5b9f\u9a13\u3068\u5149\u5b50\u6e2c\u5b9a\u300d\u7b51\u6ce2\u5927\u5b66\u6570\u7406\u7269\u8cea\u878d\u5408\u79d1\u5b66\u30bb\u30f3\u30bf\u30fc\u7814\u7a76\u4f1a\uff08\u7b51\u6ce2\u5927\u5b66,2015\u5e743\u670812-13\u65e5\uff09.<\/li>\n<li><span class=\"underline\">\u5fd7\u57a3\u8ce2\u592a<\/span>\uff1a\u300c\u9ad8\u30a8\u30cd\u30eb\u30ae\u30fc\u539f\u5b50\u6838\u885d\u7a81\u3067\u63a2\u308b\u30cf\u30c9\u30ed\u30f3\u306e\u57fa\u790e\u69cb\u9020\u300d\u65e5\u672c\u7269\u7406\u5b66\u4f1a\u30b7\u30f3\u30dd\u30b8\u30a6\u30e0\uff1a\u591a\u5f69\u306a\u5b9f\u9a13\u30d7\u30e9\u30c3\u30c8\u30d5\u30a9\u30fc\u30e0\u306b\u3088\u308b\u30cf\u30c9\u30ed\u30f3\u306e\u672c\u8cea\u7684\u81ea\u7531\u5ea6\u306e\u63a2\u6c42\uff08\u65e9\u7a32\u7530\u5927\u5b66,2015\u5e743\u670822\u65e5\uff09.<\/li>\n<li><span class=\"underline\">\u4e09\u597d\u9686\u535a<\/span>\uff1a\u300c\u5727\u7e2e\u6027MHD\u306b\u5bfe\u3059\u308b\u30ed\u30d0\u30b9\u30c8\u306a\u6570\u5024\u8a08\u7b97\u6cd5\u306e\u958b\u767a\u300d\u7b2c20\u56deNEXT\u7814\u7a76\u4f1a\uff08\u4eac\u90fd\u30c6\u30eb\u30b5,2015\u5e74\uff11\u670813-15\u65e5\uff09.<\/li>\n<li><span class=\"underline\">\u672c\u9593\u8b19\u8f14<\/span>\uff1a\u300c\u8d85\u9ad8\u5f37\u5ea6\u30ec\u30fc\u30b6\u30fc\u5834\u3092\u7528\u3044\u305f\u771f\u7a7a\u69cb\u9020\u63a2\u6c42\u3078\u306e\u30a2\u30d7\u30ed\u30fc\u30c1\u300d(\u30dd\u30b9\u30bf\u30fc\u8b1b\u6f14),\u30ec\u30fc\u30b6\u30fc\u7814\u30b7\u30f3\u30dd\u30b8\u30a6\u30e0201 \u2212\u5e73\u621025\u5e74\u5ea6\u5171\u540c\u7814\u7a76\u6210\u679c\u5831\u544a\u4f1a\u2212 \uff084\u670816\u65e5,\u5927\u962a\u5927\u5b66\uff09.<\/li>\n<li><span class=\"underline\">\u5fd7\u57a3\u8ce2\u592a<\/span>\uff1a\u300c\u9ad8\u30a8\u30cd\u30eb\u30ae\u30fc\u539f\u5b50\u6838\u885d\u7a81\u306b\u304a\u3051\u308b\u30ec\u30d7\u30c8\u30f3\u5bfe\u6e2c\u5b9a\u300d,\u30c1\u30e5\u30fc\u30c8\u30ea\u30a2\u30eb\u7814\u7a76\u4f1a \u91cd\u30a4\u30aa\u30f3\u885d\u7a81\u306e\u7269\u7406\uff1a\u57fa\u790e\u304b\u3089\u6700\u5148\u7aef\u307e\u3067\uff08\u7406\u5316\u5b66\u7814\u7a76\u6240,2015\u5e743\u670825-27\u65e5\uff09.<\/li>\n<li><span class=\"underline\">\u672c\u9593\u8b19\u8f14<\/span>\uff1a\u300cExtreme Light Infrastructure(ELI-NP)\u306e\u7269\u7406\u300d, \u65e5\u672c\u7269\u7406\u5b66\u4f1a\u7b2c70\u56de\u5e74\u6b21\u5927\u4f1a (2015\u5e743\u670824\u65e5,\u65e9\u7a32\u7530\u5927\u5b66).<\/li>\n<li>\u5927\u517c\u82f1\u6717,<span class=\"underline\">\u4e21\u89d2\u5353\u4e5f<\/span>,\u6885\u679d\u5b8f\u4e4b\uff1a\u300cPrecise Discussion onBaBar Measurement verifying TimeReversal asymmetry, taking uncertaintyof CP tagging into account\u300d\u7b2c14\u56de B\u30d5\u30a1\u30af\u30ea\u30fc\u52c9\u5f37\u4f1a\uff087\u6708,\u5e83\u5cf6\u5927\u5b66\uff09.<\/li>\n<li>\u6885\u679d\u5b8f\u4e4b,<span class=\"underline\">\u4e21\u89d2\u5353\u4e5f<\/span>,\u5927\u517c\u82f1\u6717\uff1a\u300cPrecise Discussionon BaBar Measurement verifying Time Reversal Asymmetry, takinguncertainty of CP tagging into account\u300dSummerInstitute poster\uff088\u670827\u65e5,\u5bcc\u58ebCalm,\u5bcc\u58eb\u5409\u7530\u5e02\uff09.<\/li>\n<li>\u6751\u4e0a\u7950\u5b50,<span class=\"underline\">\u77f3\u5ddd\u5065\u4e00<\/span>\uff1a\u300cMebius Domain WallFermion\u306b\u304a\u3051\u308bSchroedinger \u6c4e\u95a2\u6570\u6cd5\u306e\u69cb\u6210\u306b  \u3064\u3044\u3066\u306e\u7814\u7a76\u300d,\u65e5\u672c\u7269\u7406\u5b66\u4f1a2014\u5e74\u79cb\u5b63\u5927\u4f1a\uff089\u670818\u65e5,\u4f50\u8cc0\u5927\u5b66,\u4f50\u8cc0\u5e02\uff09.<\/li>\n<li>\u5927\u517c\u82f1\u6717,<span class=\"underline\">\u4e21\u89d2\u5353\u4e5f<\/span>,\u6885\u679d\u5b8f\u4e4b\uff1a\u300cPrecise Discussionon BaBar Measurement verifying Time Reversalasymmetry\u300d,\u65e5\u672c\u7269\u7406\u5b66\u4f1a2014\u5e74\u79cb\u5b63\u5927\u4f1a\uff089\u670818\u65e5, \u4f50\u8cc0\u5927\u5b66,\u4f50\u8cc0\u5e02\uff09.<\/li>\n<li>\u6885\u679d\u5b8f\u4e4b,<span class=\"underline\">\u4e21\u89d2\u5353\u4e5f<\/span>,\u5927\u517c\u82f1\u6717\uff1a\u300cPrecise Discussionon BaBar Measurement verifying Time ReversalAsymmetry\u300d,\u65e5\u672c\u7269\u7406\u5b66\u4f1a2014\u5e74\u79cb\u5b63\u5927\u4f1a\uff089\u670820\u65e5, \u4f50\u8cc0\u5927\u5b66,\u4f50\u8cc0\u5e02\uff09.<\/li>\n<li>\u6751\u4e0a\u7950\u5b50,<span class=\"underline\">\u77f3\u5ddd\u5065\u4e00<\/span>\uff1a\u300cM\u00f6biusDomain WallFermion\u306b\u304a\u3051\u308bSchr\u00f6dinger\u6c4e\u95a2\u6570\u6cd5\u306e\u69cb\u6210\u306b\u3064 \u3044\u3066\u306e\u7814\u7a76\u300d,\u702c\u6238\u5185SummerInstitute\uff089\u6708,\u725b\u7a93\u7814\u4fee\u30bb\u30f3\u30bf\u30fc\u30ab\u30ea\u30e8\u30f3\u30cf\u30a6\u30b9\uff09.<\/li>\n<li>\u5927\u517c\u82f1\u6717,<span class=\"underline\">\u4e21\u89d2\u5353\u4e5f<\/span>,\u6885\u679d\u5b8f\u4e4b\uff1a\u300cPrecise Discussionon BaBar Measurement verifying Time Reversal asymmetry\u300d,\u702c\u6238\u5185SummerInstitute\uff089\u6708,\u725b\u7a93\u7814\u4fee\u30bb\u30f3\u30bf\u30fc\u30ab\u30ea\u30e8\u30f3\u30cf\u30a6\u30b9\uff09.<\/li>\n<li>\u6885\u679d\u5b8f\u4e4b,<span class=\"underline\">\u4e21\u89d2\u5353\u4e5f<\/span>,\u5927\u517c\u82f1\u6717\uff1a\u300cPrecise Discussionon BaBar Asymmetry verifying T-violation\u300dKEK-PH\uff0810\u670821\u65e5,KEK Tsukuba\uff09.<\/li>\n<li>\u6885\u679d\u5b8f\u4e4b,<span class=\"underline\">\u4e21\u89d2\u5353\u4e5f<\/span>,\u5927\u517c\u82f1\u6717\uff1a\u300cPrecise Discussionon BaBar Asymmetry verifying T-violation\u300d \u7b2c2\u56de\u677e\u6c5f\u73fe\u8c61\u8ad6\u7814\u7a76\u4f1a\uff0811\u670828\u65e5\uff09.<\/li>\n<li>\u5800\u7530\u9f8d\u4e00,<span class=\"underline\">\u4e21\u89d2\u5353\u4e5f<\/span>,\u9ad8\u7530\u6d69\u884c\uff1a\u300cTime variation ofparticle number asymmetry in anexpanding  universe\u300d,\u7b2c2\u56de\u677e\u6c5f\u73fe\u8c61\u8ad6\u7814\u7a76\u4f1a\uff0811\u670830\u65e5\uff09 .<\/li>\n<li>\u5927\u517c\u82f1\u6717,<span class=\"underline\">\u4e21\u89d2\u5353\u4e5f<\/span>,\u6885\u679d\u5b8f\u4e4b\uff1a\u300cImplication of theTime reversal asymmetry in B meson system  and constraints on CPTviolation and wrong sign decays\u300d,\u65e5\u672c\u7269\u7406\u5b66\u4f1a\u7b2c70\u56de\u5e74\u6b21\u5927\u4f1a\uff082015\u5e743\u6708,\u65e9\u7a32\u7530\u5927\u5b66\uff09.<\/li>\n<li>\u6885\u679d\u5b8f\u4e4b,<span class=\"underline\">\u4e21\u89d2\u5353\u4e5f<\/span>,\u5927\u517c\u82f1\u6717\uff1a\u300cTime ReversalAsymmetry with B Meson Decays:Introduction\u300d  \u65e5\u672c\u7269\u7406\u5b66\u4f1a\u7b2c70\u56de\u5e74\u6b21\u5927\u4f1a\uff082015\u5e743\u670824\u65e5,\u65e9\u7a32\u7530\u5927\u5b66\uff09.<\/li>\n<\/ul>\n\n<p><a id=\"events_H26\"><\/a><\/p>\n<h2>\u6975\u9650\u5b87\u5b99\u7814\u7a76\u62e0\u70b9\u4e3b\u50ac\uff0f\u5171\u50ac\u30a4\u30d9\u30f3\u30c8 CORE-U Events<\/h2>\n\n","protected":false},"excerpt":{"rendered":"<p>[\u8ad6\u6587 Publications] [\u5b66\u4f1a\u30fb\u7814\u7a76\u4f1a\u767a\u8868 Presentations] [Core-U\u30a4\u30d9\u30f3\u30c8 Core-U Events] \u8ad6\u6587 Publications \u5b66\u4f1a\u30fb\u7814\u7a76\u4f1a\u3067\u306e\u767a\u8868 Presentations \u6975\u9650\u5b87\u5b99\u7814\u7a76\u62e0\u70b9\u4e3b\u50ac\uff0f\u5171\u50ac\u30a4\u30d9\u30f3\u30c8 CORE-U Events<\/p>\n","protected":false},"author":2,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"_exactmetrics_skip_tracking":false,"footnotes":""},"class_list":["post-1075","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/core-u.hiroshima-u.ac.jp\/en\/wp-json\/wp\/v2\/pages\/1075","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/core-u.hiroshima-u.ac.jp\/en\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/core-u.hiroshima-u.ac.jp\/en\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/core-u.hiroshima-u.ac.jp\/en\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/core-u.hiroshima-u.ac.jp\/en\/wp-json\/wp\/v2\/comments?post=1075"}],"version-history":[{"count":1,"href":"https:\/\/core-u.hiroshima-u.ac.jp\/en\/wp-json\/wp\/v2\/pages\/1075\/revisions"}],"predecessor-version":[{"id":1076,"href":"https:\/\/core-u.hiroshima-u.ac.jp\/en\/wp-json\/wp\/v2\/pages\/1075\/revisions\/1076"}],"wp:attachment":[{"href":"https:\/\/core-u.hiroshima-u.ac.jp\/en\/wp-json\/wp\/v2\/media?parent=1075"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}