{"id":1073,"date":"2018-02-02T15:54:08","date_gmt":"2018-02-02T06:54:08","guid":{"rendered":"http:\/\/core-u.hiroshima-u.ac.jp\/?page_id=1073"},"modified":"2018-02-02T15:54:08","modified_gmt":"2018-02-02T06:54:08","slug":"1073-2","status":"publish","type":"page","link":"https:\/\/core-u.hiroshima-u.ac.jp\/en\/1073-2.html","title":{"rendered":""},"content":{"rendered":"<p style=\"text-align: center;\">[<a href=\"#publications_H25\">\u8ad6\u6587 Publications<\/a>] [<a href=\"#presentations_H25\">\u5b66\u4f1a\u30fb\u7814\u7a76\u4f1a\u767a\u8868 Presentations<\/a>] [<a href=\"#events_H25\">Core-U\u30a4\u30d9\u30f3\u30c8 Core-U Events<\/a>]<\/p>\n<p><a id=\"publications_H25\"><\/a><\/p>\n<h2>\u8ad6\u6587 Publications<\/h2>\n<ul style=\"list-style-type: disc;\">\n<li>T.Mizuno(105\u756a\u76ee), <span style=\"text-decoration: underline;\">H.Takahashi<\/span>(141\u756a\u76ee), \u5168159\u4eba; \u201cThe First Fermi-LAT Catalog of Sources above 10 GeV\u201d, Fermi LAT Collaboration, <em>ApJS<\/em>, <strong>209<\/strong>, 34, (2013).<\/li>\n<li><span style=\"text-decoration: underline;\">Y.Fukazawa<\/span>(56\u756a\u76ee), T.Mizuno(109\u756a\u76ee), <span style=\"text-decoration: underline;\">M.Ohno<\/span>(119\u756a\u76ee), <span style=\"text-decoration: underline;\">H.Takahashi<\/span>(156\u756a\u76ee),\u5168180\u4eba; \u201cThe First Fermi-LAT Gamma-Ray Burst Catalog\u201d, Fermi LAT Collaboration, <em>ApJS<\/em>, <strong>209<\/strong>, 11, (2013).<\/li>\n<li>T.Mizuno(69\u756a\u76ee), <span style=\"text-decoration: underline;\">H.Takahashi<\/span>(99\u756a\u76ee), \u5168114\u4eba; \u201cPSR J2021+4026 in the Gamma Cygni Region: The First Variable Gamma-Ray Pulsar Seen by the Fermi LAT\u201d, Fermi LAT Collaboration, <em>ApJ<\/em>, <strong>777<\/strong>, L2, (2013).<\/li>\n<li><span style=\"text-decoration: underline;\">Y.Fukazawa<\/span>(48\u756a\u76ee), T.Mizuno(88\u756a\u76ee), <span style=\"text-decoration: underline;\">H.Takahashi<\/span>(125\u756a\u76ee),\u5168144\u4eba; \u201cSearch for gamma-ray spectral lines with the Fermi Large Area Telescope and dark matter implications\u201d,Fermi LAT Collaboration, <em>Phys. Rev.<\/em> D<strong>88<\/strong>, 082002, (2013).<\/li>\n<li>T.Mizuno (117\u756a\u76ee), <span style=\"text-decoration: underline;\">M.Ohno<\/span> (127\u756a\u76ee), <span style=\"text-decoration: underline;\">H.Takahashi<\/span> (179\u756a\u76ee), \u5168211\u4eba; \u201cThe Second Fermi Large Area Telescope Catalog of Gamma-Ray Pulsars\u201d, Fermi LAT Collaboration,<em> ApJS<\/em>, <strong>208<\/strong>, 17, (2013).<\/li>\n<li>T.Mizuno(84\u756a\u76ee), <span style=\"text-decoration: underline;\">H.Takahashi<\/span>(114\u756a\u76ee), \u5168129\u4eba; \u201cAssociating Long-term Gamma-Ray Variability with the Superorbital Period of LS I +61deg303\u201d, Fermi LAT Collaboration, <em>ApJ<\/em>, <strong>773<\/strong>, L35, (2013).<<\/li>\n<li><span style=\"text-decoration: underline;\">Y.Fukazawa<\/span>(49\u756a\u76ee), T.Mizuno(101\u756a\u76ee), <span style=\"text-decoration: underline;\">H.Takahashi<\/span>(139\u756a\u76ee), \u5168158\u4eba; \u201cConstraints on the  Galactic Population of TeV Pulsar Wind Nebulae Using Fermi Large Area Telescope Observations\u201d, Fermi LAT Collaboration, <em>ApJ<\/em>, <strong>773<\/strong>, 77, (2013).<\/li>\n<li><span style=\"text-decoration: underline;\">Y.Fukazawa<\/span>(51\u756a\u76ee), T.Mizuno(100\u756a\u76ee), <span style=\"text-decoration: underline;\">H.Takahashi<\/span>(136\u756a\u76ee), \u5168156\u4eba; \u201cThe Fermi All-sky Variability Analysis: A List of Flaring Gamma-Ray Sources and the Search for Transients in Our Galaxy\u201d, Fermi LAT Collaboration, <em>ApJ<\/em>, <strong>771<\/strong>, 57, (2013).<\/li>\n<li><span style=\"text-decoration: underline;\">Y.Fukazawa<\/span>(53\u756a\u76ee), T.Mizuno(102\u756a\u76ee), <span style=\"text-decoration: underline;\">H.Takahashi<\/span>(151\u756a\u76ee),\u5168175\u4eba; \u201cDetermination of the Point-spread Function for the Fermi Large Area Telescope from On-orbit Data and Limits on Pair Halos of Active Galactic Nuclei\u201d, Fermi LAT Collaboration, <em>ApJ<\/em>, <strong>765<\/strong>, 54, (2013).<\/li>\n<li><span style=\"text-decoration: underline;\">Y.Fukazawa<\/span>(55\u756a\u76ee), T.Mizuno(105\u756a\u76ee), <span style=\"text-decoration: underline;\">M.Ohno<\/span>(114\u756a\u76ee), <span style=\"text-decoration: underline;\">H.Takahashi<\/span>(146\u756a\u76ee),\u5168169\u4eba;   \u201cDetection of the Characteristic Pion-Decay Signature in Supernova Remnants\u201d, Fermi LAT Collaboration,<em> Science<\/em>, <strong>339<\/strong>, 807-811, (2013).<\/li>\n<li><span style=\"text-decoration: underline;\">Y.Fukazawa<\/span>(42\u756a\u76ee), T.Mizuno(82\u756a\u76ee), <span style=\"text-decoration: underline;\">M.Ohno<\/span>(93\u756a\u76ee), <span style=\"text-decoration: underline;\">H.Takahashi<\/span>(119\u756a\u76ee),\u5168162\u4eba; \u201cMultiwavelength Observations of GRB 110731A: GeV Emission from Onset to Afterglow\u201d, Fermi LAT Collaboration, <em>ApJ<\/em>, <strong>763<\/strong>, 71, (2013).<\/li>\n<li>T.Yoshida, T.Mizuno<em> et al.<\/em>; \u201cTwo Power-Law Stats of the Ultraluminous X-ray Source IC 342 X-1\u201d, <em>PASJ<\/em>, <strong>65<\/strong>, 48 (2013).<\/li>\n<li>B. Acharya, T. Mizuno<em> et al<\/em>.; \u201cIntroducting the CTA concept\u201d, <em>Astroparticle Physics<\/em> <strong>43<\/strong>, 3 (2013).<\/li>\n<li><span style=\"text-decoration: underline;\">M.Ohno<\/span>, K.Goto, Y.Hanabata, <span style=\"text-decoration: underline;\">H.Takahashi<\/span>, <span style=\"text-decoration: underline;\">Y.Fukazawa<\/span>, M.Yoshino, T.Saito, T.Nakamori, J.Kataoka, M.Sasano, S.Torii, H.Uchiyama, K.Nakazawa, S.Watanabe, M.Kokubun, M.Ohta, T.Sato, T.Takahashi, H.Tajima; \u201cDevelopment of signal processing system of avalanche photo diode  for space observations by Astro-H\u201d, <em>NIMA<\/em>,<strong> 699<\/strong>, 112-115 (2013).<\/li>\n<li>T.Saito, T.Nakamori, M.Yoshino, H.Mizoma, J.Kataoka, K.Kawakami, Y.Yatsu, <span style=\"text-decoration: underline;\">M.Ohno<\/span>, K.Goto,  Y.Hanabata, <span style=\"text-decoration: underline;\">H.Takahashi<\/span>, <span style=\"text-decoration: underline;\">Y.Fukazawa<\/span>, M.Sasano, S.Torii, H.Uchiyama, K.Nakazawa, K.Makishima, S.Watanabe, M.Kokubun, T.Takahashi, K.Mori, <em>et al.<\/em>; \u201cDevelopment of high performance Avalanche Photodiodes and dedicated analog system for HXI\/SGD detectors onboard the Astro-H mission\u201d, <em>NIMA<\/em>, <strong>699<\/strong>, 230-234 (2013).<\/li>\n<li>K.Hayashi, I.C.Park, K.D.Otsu, I.Ueno, S.Nishino, M.Matsuoka, H.Yasuda, <span style=\"text-decoration: underline;\">Y.Fukazawa<\/span>, T.Ohsugi,  T.Mizuno, <span style=\"text-decoration: underline;\">H.Takahashi<\/span>, <span style=\"text-decoration: underline;\">M.Ohno<\/span>, S.Endo, T.Tanaka, H.Tajima, M.Kokubun, S.Watanabe, T.Takahashi, K.Nakazawa, Y.Uchihori, H.Kitamura, <em>et al.<\/em>; \u201cRadiation effects on the silicon semiconductor detectors for the ASTRO-H mission\u201d, <em>NIMA<\/em>, <strong>699<\/strong>, 225-229 (2013).<\/li>\n<li>S.Ishikawa, S.Krucker, <span style=\"text-decoration: underline;\">M.Ohno,<\/span> R.Lin; \u201cSuzaku\/WAM and RHESSI Observations of Non-thermal Electrons in Solar Microflares\u201d, <em>ApJ<\/em>, <strong>765<\/strong>, 2, 1-6 (2013).<\/li>\n<li>S.Masuda, M.Shimoo, T.Kawate, S.Ishikawa, <span style=\"text-decoration: underline;\">M.Ohno<\/span>; \u201cExtremely Microwave-Rich Solar Flare  Observed with Nobeyama Radioheliograph\u201d, <em>PASJ<\/em>, <strong>65<\/strong>, S1, 1-6 (2013).<\/li>\n<li>K.Watanabe, T.Shimizu, S.Masuda, K.Ichimoto, <span style=\"text-decoration: underline;\">M.Ohno<\/span>; \u201cEmission Height and Temperature Distribution of White-light Emission Observed by Hinode\/SOT from the 2012 January 27 X-class Solar Flare\u201d, <em>ApJ<\/em>, <strong>776<\/strong>, 123, 1-9 (2013).<\/li>\n<li>K.Hurley, <span style=\"text-decoration: underline;\">Y.Fukazawa<\/span>(20\u756a\u76ee), <span style=\"text-decoration: underline;\">M.Ohno<\/span>(26\u756a\u76ee), \u4ed637\u540d\uff1b\u201cThe Interplanetary Network Supplement to the Fermi GBM Catalog of Cosmic Gamma-Ray Bursts\u201d, <em>ApJS<\/em>, <strong>207<\/strong>, 39, 1-8 (2013).<\/li>\n<li>V.D.Pal\u2019shin, <span style=\"text-decoration: underline;\">M.Ohno<\/span>(35\u756a\u76ee), <span style=\"text-decoration: underline;\">Y.Fukazawa<\/span>(36\u756a\u76ee), \u4ed671\u540d\uff1b\u201cInterplanetary Network Localizations of Konus Short Gamma-Ray Bursts\u201d, <em>ApJS<\/em>, <strong>207<\/strong>, 38, 1-14 (2013).<\/li>\n<li>K.Hurley, <span style=\"text-decoration: underline;\">M.Ohno<\/span>(23\u756a\u76ee),\u4ed640\u540d; \u201cThe Interplanetary Network\u201d, <em>EAS Publications Series<\/em>, <strong>61<\/strong>, 459-464 (2013).<\/li>\n<li>H.Odaka, D.Khangulyan, Y.T.Tanaka, S.Watanabe, T.Takahashi, K.Makishima; \u201cShort-term Variability of X-Rays from Accreting Neutron Star Vela X-1. I. Suzaku Observations\u201d, <em>Astrophysical Journal<\/em>,<strong>767<\/strong>, 70-86 (2013).<\/li>\n<li>Y.T.Tanaka, <span style=\"text-decoration: underline;\">Y.Fukazawa<\/span> (\uff19\u756a\u76ee),<em> et al.<\/em>; \u201cFermi Large Area Telescope Detection of Two Very- high-energy (<em>E<\/em>>100 GeV) Gamma-Ray Photons from the z = 1.1 Blazar PKS 0426-380\u201d, <em>ApJ<\/em>, <strong>777<\/strong>, L18 (2013).<\/li>\n<li>R.Itoh, Y.T.Tanaka (\uff12\u756a\u76ee), <span style=\"text-decoration: underline;\">Y.Fukazawa<\/span> (\uff13\u756a\u76ee), K.S.Kawabata (\uff14\u756a\u76ee), M.Uemura (\uff19\u756a\u76ee), M.Yoshida(11\u756a\u76ee)<em> et al.<\/em>; \u201cMinute-scale Rapid Variability of the Optical Polarization in the Narrow-line Seyfert 1 Galaxy PMN J0948+0022\u201d, <em>ApJ<\/em>, <strong>775<\/strong>, L26 (2013).<\/li>\n<li>T.Kouzu, <span style=\"text-decoration: underline;\">Y.Fukazawa<\/span>(\uff18\u756a\u76ee) <em>et al.<\/em>; \u201cSpectral Variation of Hard X-Ray Emission from the Crab Nebula with the Suzaku Hard X-Ray Detector\u201d,<em> PASJ<\/em>, <strong>65<\/strong>, 74 (2013).<\/li>\n<li>K.Takaki, K.S.Kawabata(\uff12\u756a\u76ee), <span style=\"text-decoration: underline;\">Y.Fukazawa<\/span>(\uff17\u756a\u76ee), M.Uemura(13\u756a\u76ee), M.Yoshida(13\u756a\u76ee)  <em>et al<\/em>.; \u201cA Luminous and Fast-expanding Type Ib Supernova SN 2012au\u201d, <em>ApJ<\/em>, <strong>772<\/strong>, L17 (2013).<\/li>\n<li>R.Itoh, <span style=\"text-decoration: underline;\">Y.Fukazawa<\/span>(\uff12\u756a\u76ee), Y.Tanaka(\uff13\u756a\u76ee), K.S.Kawabata(11\u756a\u76ee), M.Uemura(32\u756a\u76ee), M.Yoshida(38\u756a\u76ee) <em>et al<\/em>.; \u201cDense Optical and Near-infrared Monitoring of CTA 102 during High State in 2012 with OISTER: Detection of Intra-night Orphan Polarized Flux Flare\u201d, <em>ApJ<\/em>, <strong>768<\/strong>, L24 (2013).<\/li>\n<li>R.Itoh, <span style=\"text-decoration: underline;\">Y.Fukazawa<\/span>(\uff12\u756a\u76ee) <em>et al.<\/em>; \u201cA Study of the Long-Term Spectral Variations of 3C 66A Observed with the Fermi and Kanata Telescope\u201d, <em>PASJ<\/em>, <strong>65<\/strong>, 18 (2013).<\/li>\n<li>Y.Hanabata, <span style=\"text-decoration: underline;\">Y.Fukazawa<\/span>(\uff15\u756a\u76ee) <em>et al.<\/em>; \u201cX-Ray Observations of the W 51 Complex with Suzaku\u201d,  <em>PASJ<\/em>, <strong>65<\/strong>, 42 (2013).<\/li>\n<li>K.Sakimoto, M.Uemura(\uff12\u756a\u76ee), K.S.Kawabata(\uff14\u756a\u76ee), <span style=\"text-decoration: underline;\">Y.Fukazawa<\/span>(\uff15\u756a\u76ee), M.Yoshida(\uff19\u756a\u76ee) <em>et al.<\/em>; \u201cPhotopolarimetric Monitoring of the Blazar BL Lac in the Optical and Near-Infrared Bands: Decay of the Long-Lived Component\u201d, <em>PASJ<\/em>, <strong>65<\/strong>, 35 (2013).<\/li>\n<li>S.Yamazaki, <span style=\"text-decoration: underline;\">Y.Fukazawa<\/span>(\uff12\u756a\u76ee),<span style=\"text-decoration: underline;\"> H.Takahashi(<\/span>\uff16\u756a\u76ee), K.S.Kawabata(\uff18\u756a\u76ee), M.Yoshida(\uff19\u756a\u76ee), M.Uemura(10\u756a\u76ee) <em>et al.<\/em>; \u201cX-Ray and Optical Monitoring of a Gamma-Ray-Emitting Radio Galaxy, NGC 1275\u201d, <em>PASJ<\/em>,<strong> 65<\/strong>, 30 (2013).<\/li>\n<li>K.Ichikawa, <span style=\"text-decoration: underline;\">Y.Fukazawa<\/span>(\uff18\u756a\u76ee) <em>et al.<\/em>; \u201cSuzaku Observations of the Outskirts of A1835: Deviation from Hydrostatic Equilibrium\u201d, <em>ApJ<\/em>, <strong>766<\/strong>, 90 (2013).<\/li>\n<li>B.Rani, <span style=\"text-decoration: underline;\">Y.Fukazawa<\/span>(12\u756a\u76ee) <em>et al.<\/em>; \u201cRadio to gamma-ray variability study of blazar S5 0716+714\u201d, <em>A&amp;A<\/em>, <strong>552<\/strong>, A11 (2013).<\/li>\n<li>L.Stawarz, Y.T.Tanaka(\uff12\u756a\u76ee), <span style=\"text-decoration: underline;\">Y.Fukazawa<\/span>(\uff17\u756a\u76ee) <em>et al.<\/em>; \u201cGiant Lobes of Centaurus A Radio Galaxy Observed with the Suzaku X-Ray Satellite\u201d, <em>ApJ<\/em>, <strong>766<\/strong>, 48 (2013).<\/li>\n<li>M.Yamanaka, K.Maeda, M.Kawabata, M.Tanaka, K.Takaki, I.Ueno, K.Masumoto, K.S.Kawabata, R.Itoh, Y.Moritani, H.Akitaya, A.Arai, S.Honda, K.Nishiyama, F.Kabashima, K.Matsumoto, D.Nogami, M.Yoshida; \u201cEarly-phase Photometry and Spectroscopy of Transitional Type Ia SN 2012ht: Direct Constraint on the Rise Time\u201d, <em>ApJ Letters<\/em>, <strong>782<\/strong>, article id. L35 (1-6) (2014).<\/li>\n<li>H.Gaur, A.C.Gupta, P.J.Wiita, M.Uemura, R.Itoh, M.Sasada; \u201cAnti-correlated Optical Flux and Polarization Variability in BL Lac\u201d, <em>ApJ Letters<\/em>, <strong>781<\/strong>, article id. L4 (1-5) (2014).<\/li>\n<li>PACS-CS Collaboration: Y.Namekawa, S.Aoki, <span style=\"text-decoration: underline;\">K.-I.Ishikawa<\/span>, N.Ishizuka, K.Kanaya, Y.Kuramashi,<span style=\"text-decoration: underline;\"> M.Okawa<\/span>, Y.Taniguchi, A.Ukawa, N.Ukita, T.Yoshie, \u201cCharmed baryons at the physical point in 2+1 flavor lattice QCD,\u201d <em>Phys. Rev.<\/em> D<strong>87<\/strong> (2013) 094512.<\/li>\n<li>A.Gonzalez-Arroyo and <span style=\"text-decoration: underline;\">M.Okawa<\/span>, \u201cTwisted space-time reduced model of large N QCD with two  adjoint Wilson fermions\u201d, <em>Phys. Rev.<\/em> D<strong>88<\/strong> (2013) 014514.<\/li>\n<li>M.Garcia Perez, A.Gonzalez-Arroyo and M.Okawa, \u201cSpatial volume dependence for 2+1  dimensional SU(N) Yang-Mills theory\u201d, <em>JHEP<\/em> <strong>1309<\/strong> (2013) 003.<\/li>\n<li>M.Hayakawa, <span style=\"text-decoration: underline;\">K.-I.Ishikawa<\/span>, S.Takeda, N.Yamada, \u201cRunning coupling constant and mass anomalous dimension of six-flavor SU(2) gauge theory\u201d, <em>Phys. Rev.<\/em> D<strong> 88<\/strong> (2013) 094504.<\/li>\n<li>M.Hayakawa, <span style=\"text-decoration: underline;\">K.-I.Ishikawa<\/span>, S.Takeda, M.Tomii, N.Yamada,\u201cLattice study on quantum-mechanical    dynamics of two-color QCD with six light flavors\u201d, <em>Phys. Rev<\/em>. D <strong>88<\/strong> (2013) 094506.<\/li>\n<li><span style=\"text-decoration: underline;\">K.-I.Ishikawa<\/span>, Y.Iwasaki, Yu Nakayama, T.Yoshie, \u201cConformal theories with an IR cutoff\u201d, <em>Phys. Rev. <\/em>D <strong>87<\/strong> (2013) 071503.<\/li>\n<li>R.Kawasaki, <span style=\"text-decoration: underline;\">T.Morozumi,<\/span> and H.Umeeda, \u201cQuark sector CP violation of the universal seesaw    model\u201d, <em>Phys.Rev.<\/em> D<strong>88<\/strong> (2013) 033019.<\/li>\n<li>K.Tamai and <span style=\"text-decoration: underline;\">T.Morozumi,<\/span>\u201cCharged Higgs and neutral Higgs pair production of the weak gauge    boson fusion process in electron-positron collisions\u201d, <em>PTEP<\/em> 093B02 (2013), Errtam-ibid.2014 (2014) 4, 049201.<\/li>\n<li><span style=\"text-decoration: underline;\">K.-I.Ishikawa<\/span>, D.Kimura, <span style=\"text-decoration: underline;\">K.Shigaki<\/span>, A.Tsuji, \u201cA numerical evaluation of vacuum polarization tensor in constant external magnetic fields\u201d, <em>Int. J. Mod. Phys.<\/em> A <strong>28<\/strong> (2013) 1350100.<\/li>\n<li>J. Kov\u00e1\u0159, O. Kop\u00e1\u010dek, V. Karas and <span style=\"text-decoration: underline;\">Y. Kojima<\/span>,\u201cRegular and chaotic orbits near a massive magnetic dipole\u201d, <em>Class. Quantum Grav.<\/em> <strong>30<\/strong> (2013) 025010. (23 pages).<\/li>\n<li>S.Iso, <span style=\"text-decoration: underline;\">K<\/span><span style=\"text-decoration: underline;\">.<\/span><span style=\"text-decoration: underline;\">Yamamoto<\/span>, S.Zhang, \u201cOn the Cancellation Mechanism of Radiation from the Unruh Detector\u201d, <em>Progress of Theoretical and Experimental Physics<\/em> (2013) 063B01-1-16.<\/li>\n<li>C.Hikage, <span style=\"text-decoration: underline;\">K<\/span><span style=\"text-decoration: underline;\">.<\/span><span style=\"text-decoration: underline;\">Yamamoto<\/span>, \u201cImpact of satellite galaxies in measuring the redshift-space distortions\u201d, <em>Journal of Cosmology and Astroparticle Physics<\/em>, <strong>08<\/strong> (2013) 019-1-29.<\/li>\n<li>T.Sato, G.Huetsi, G.Nakamura, <span style=\"text-decoration: underline;\">K<\/span><span style=\"text-decoration: underline;\">.<\/span><span style=\"text-decoration: underline;\">Yamamoto<\/span>, \u201cWindow effect in the power spectrum analysis of a galaxy redshift survey\u201d, <em>International Journal of Astronomy and Astrophysics<\/em>, <strong>3<\/strong> (2013) 243-256.<\/li>\n<li>B.Abelev, <span style=\"text-decoration: underline;\">K.Shigaki<\/span>, <span style=\"text-decoration: underline;\">T.Sugitate<\/span>, <em>et al.<\/em>, \u201cK0s and Lambda production in Pb-Pb collisions at \u221as<sub>NN<\/sub> =  2.76 TeV\u201d, <em>Phys. Rev. Lett. <\/em><strong>111<\/strong>, 222301, 2013.<\/li>\n<li>B.Abelev, <span style=\"text-decoration: underline;\">K.Shigaki<\/span>, <span style=\"text-decoration: underline;\">T.Sugitate<\/span>, <em>et al.<\/em>, \u201cLong-range angular correlations of pi, K and p in p-Pb collisions at \u221as<sub>NN<\/sub> = 5.02 TeV\u201d, <em>Phys. Lett. <\/em><strong>B726<\/strong>, 164-177, 2013.<\/li>\n<li>B.Abelev, <span style=\"text-decoration: underline;\">K.Shigaki<\/span>, <span style=\"text-decoration: underline;\">T.Sugitate<\/span>, <em>et al.<\/em>, \u201cMultiplicity dependence of two-particle azimuthal  correlations in pp collisions at the LHC\u201d, <em>JHEP<\/em><strong> 1309<\/strong>, 049, 2013.<\/li>\n<li>B.Abelev, <span style=\"text-decoration: underline;\">K.Shigaki<\/span>, <span style=\"text-decoration: underline;\">T.Sugitate<\/span>, <em>et al.<\/em>, \u201cMultiplicity dependence of the average transverse  momentum in pp, p-Pb, and Pb-Pb collisions at the LHC\u201d, <em>Phys. Lett. <\/em><strong>B727<\/strong>, 371-380, 2013.<\/li>\n<li>B.Abelev, <span style=\"text-decoration: underline;\">K.Shigaki<\/span>, <span style=\"text-decoration: underline;\">T.Sugitate<\/span>, <em>et al.<\/em>, \u201cEnergy dependence of the transverse momentum   distributions of charged particles in pp collisions measured by ALICE\u201d, <em>Euro. Phys. J. <\/em><strong>C73<\/strong>, 2662, 2013.<\/li>\n<li>B.Abelev, <span style=\"text-decoration: underline;\">K.Shigaki<\/span>, <span style=\"text-decoration: underline;\">T.Sugitate<\/span>, <em>et al.<\/em>, \u201cDirected flow of charged particles at midrapidity relative to the spectator plane in Pb-Pb collisions at \u221as<sub>NN<\/sub> = 2.76 TeV\u201d, <em>Phys. Rev. Lett. <\/em><strong>111<\/strong>, 232302, 2013.<\/li>\n<li>E.Abbas, <span style=\"text-decoration: underline;\">K.Shigaki<\/span>, <span style=\"text-decoration: underline;\">T.Sugitate<\/span>, <em>et al.<\/em>, \u201cPerformance of the ALICE VZERO system\u201d, <em>JINST <\/em><strong>8<\/strong>, P10016, 2013.<\/li>\n<li>B.Abelev, <span style=\"text-decoration: underline;\">K.Shigaki<\/span>, <span style=\"text-decoration: underline;\">T.Sugitate<\/span>, <em>et al.<\/em>, \u201cD meson elliptic flow in non-central Pb-Pb collisions at \u221as<sub>NN<\/sub> = 2.76 TeV\u201d, <em>Phys. Rev. Lett. <\/em><strong>111<\/strong>, 102301, 2013.<\/li>\n<li>E.Abbas, <span style=\"text-decoration: underline;\">K.Shigaki<\/span>, <span style=\"text-decoration: underline;\">T.Sugitate<\/span>, <em>et al.<\/em>, \u201cMid-rapidity anti-baryon to baryon ratios in pp collisions at \u221as = 0.9, 2.76 and 7 TeV measured by ALICE\u201d, <em>Euro. Phys. J. <\/em><strong>C73<\/strong>, 2496, 2013.<\/li>\n<li>E.Abbas, <span style=\"text-decoration: underline;\">K.Shigaki<\/span>, <span style=\"text-decoration: underline;\">T.Sugitate<\/span>, <em>et al.<\/em>, \u201cCharmonium and e+e\u2212 pair photoproduction at mid-rapidity in ultra-peripheral Pb-Pb collisions at \u221as<sub>NN<\/sub> = 2.76 TeV\u201d, <em>Euro. Phys. J. <\/em><strong>C73<\/strong>, 2617, 2013.<\/li>\n<li>E.Abbas, <span style=\"text-decoration: underline;\">K.Shigaki<\/span>, <span style=\"text-decoration: underline;\">T.Sugitate<\/span>, <em>et al.<\/em>, \u201cCentrality dependence of the pseudorapidity density distribution for charged particles in Pb-Pb collisions at\u3000\u221as<sub>NN<\/sub> = 2.76 TeV\u201d, <em>Phys. Lett. <\/em><strong>B726<\/strong>, 610-622, 2013.<\/li>\n<li>E.Abbas, <span style=\"text-decoration: underline;\">K.Shigaki<\/span>, <span style=\"text-decoration: underline;\">T.Sugitate<\/span>, <em>et al.<\/em>, \u201cJ\/psi elliptic flow in Pb-Pb collisions at \u221as<sub>NN<\/sub> = 2.76 TeV\u201d,  <em>Phys. Rev. Lett. <\/em><strong>111<\/strong>, 162301, 2013.<\/li>\n<li>B.Abelev, <span style=\"text-decoration: underline;\">K.Shigaki<\/span>, <span style=\"text-decoration: underline;\">T.Sugitate<\/span>, <em>et al.<\/em>, \u201cCentrality dependence of pi, K, p production in Pb-Pbcollisions at \u221as<sub>NN<\/sub> = 2.76 TeV\u201d, <em>Phys. Rev. C <\/em><strong>88<\/strong>, 044910, 2013.<\/li>\n<li>B.Abelev, <span style=\"text-decoration: underline;\">K.Shigaki<\/span>, <span style=\"text-decoration: underline;\">T.Sugitate<\/span>, <em>et al.<\/em>, \u201cCentrality determination of Pb-Pb collisions at \u221as<sub>NN<\/sub> = 2.76\u3000TeV with ALICE\u201d, <em>Phys. Rev. C <\/em><strong>88<\/strong>, 044909, 2013.<\/li>\n<li>B.Abelev, <span style=\"text-decoration: underline;\">K.Shigaki<\/span>, <span style=\"text-decoration: underline;\">T.Sugitate<\/span>, <em>et al.<\/em>, \u201cCharge correlations using the balance function in Pb-Pb collisions at \u221as<sub>NN<\/sub> = 2.76 TeV\u201d, <em>Phys. Lett. <\/em><strong>B723<\/strong>, 267-279, 2013.<\/li>\n<li>B.Abelev, <span style=\"text-decoration: underline;\">K.Shigaki<\/span>, <span style=\"text-decoration: underline;\">T.Sugitate<\/span>, <em>et al.<\/em>, \u201cMeasurement of the inclusive differential jet cross section in pp collisions at \u221as = 2.76 TeV\u201d, <em>Phys. Lett. <\/em><strong>B722<\/strong>, 262-272, 2013.<\/li>\n<li>B.Abelev, <span style=\"text-decoration: underline;\">K.Shigaki<\/span>, <span style=\"text-decoration: underline;\">T.Sugitate<\/span>, <em>et al.<\/em>, \u201cCharged kaon femtoscopic correlations in pp collisions  at \u221as = 7 TeV\u201d, <em>Phys. Rev. D <\/em><strong>87<\/strong>, 052016, 2013.<\/li>\n<li>B.Abelev, <span style=\"text-decoration: underline;\">K.Shigaki<\/span>, <span style=\"text-decoration: underline;\">T.Sugitate<\/span>, <em>et al.<\/em>, \u201cLong-range angular correlations on the near and away side in p-Pb collisions at \u00d6s<sub>NN<\/sub> = 5.02 TeV\u201d, <em>Phys. Lett. <\/em><strong>B719<\/strong>, 29-41, 2013.<\/li>\n<li>B.Abelev, <span style=\"text-decoration: underline;\">K.Shigaki<\/span>, <span style=\"text-decoration: underline;\">T.Sugitate<\/span>, <em>et al.<\/em>, \u201cTransverse momentum distribution and nuclear modification factor of charged particles in p-Pb collisions at \u221as<sub>NN<\/sub> = 5.02 TeV\u201d, <em>Phys. Rev. Lett. <\/em><strong>110<\/strong>, 082302, 2013.<\/li>\n<li>B.Abelev, <span style=\"text-decoration: underline;\">K.Shigaki<\/span>, <span style=\"text-decoration: underline;\">T.Sugitate<\/span>, <em>et al.<\/em>, \u201cPseudorapidity density of charged particles p-Pb collisions  at \u221as<sub>NN<\/sub> = 5.02 TeV\u201d, <em>Phys. Rev. Lett. <\/em><strong>110<\/strong>, 032301, 2013.<\/li>\n<li>B.Abelev, <span style=\"text-decoration: underline;\">K.Shigaki<\/span>, <span style=\"text-decoration: underline;\">T.Sugitate<\/span>, <em>et al.<\/em>, \u201cCoherent J\/psi photoproduction in ultra-peripheral Pb-Pb  collisions at \u221as<sub>NN<\/sub> = 2.76 TeV\u201d, <em>Phys. Lett. <\/em><strong>B718<\/strong>, 1273-1283, 2013.<\/li>\n<li>B.Abelev, <span style=\"text-decoration: underline;\">K.Shigaki<\/span>, <span style=\"text-decoration: underline;\">T.Sugitate<\/span>, <em>et al.<\/em>, \u201cMeasurement of inelastic, single- and double-diffraction cross sections in proton-proton collisions at the LHC with ALICE\u201d, <em>Euro. Phys. J. <\/em><strong>C73<\/strong>, 2456, 2013.<\/li>\n<li>B.Abelev, <span style=\"text-decoration: underline;\">K.Shigaki<\/span>, <span style=\"text-decoration: underline;\">T.Sugitate<\/span>, <em>et al.<\/em>, \u201cCentrality dependence of charged particle production at large transverse momentum in Pb-Pb collisions at \u221as<sub>NN<\/sub> = 2.76 TeV\u201d, <em>Phys. Lett. <\/em><strong>B720<\/strong>, 52-62, 2013.<\/li>\n<li>B.Abelev, <span style=\"text-decoration: underline;\">K.Shigaki<\/span>, <span style=\"text-decoration: underline;\">T.Sugitate<\/span>, <em>et al.<\/em>, \u201cMeasurement of electrons from beauty hadron decays  in pp collisions at \u221as = 7 TeV\u201d, <em>Phys. Lett. <\/em><strong>B721<\/strong>, 13-23, 2013.<\/li>\n<li>B.Abelev, <span style=\"text-decoration: underline;\">K.Shigaki<\/span>, <span style=\"text-decoration: underline;\">T.Sugitate<\/span>, <em>et al.<\/em>, \u201cNet-charge fluctuations in Pb-Pb collisions at \u221as<sub>NN<\/sub> = 2.76 TeV\u201d, <em>Phys. Rev. Lett. <\/em><strong>110<\/strong>, 152301, 2013.<\/li>\n<li>B.Abelev, <span style=\"text-decoration: underline;\">K.Shigaki<\/span>, <span style=\"text-decoration: underline;\">T.Sugitate<\/span>, <em>et al.<\/em>, \u201cCharge separation relative to the reaction plane in Pb-Pb collisions at \u00d6s<sub>NN<\/sub> = 2.76 TeV\u201d, <em>Phys. Rev. Lett. <\/em><strong>110<\/strong>, 012301, 2013.<\/li>\n<li>B.Abelev, <span style=\"text-decoration: underline;\">K.Shigaki<\/span>, <span style=\"text-decoration: underline;\">T.Sugitate<\/span>, <em>et al.<\/em>, \u201cAnisotropic flow of charged hadrons, pions and (anti-)protons measured at high transverse momentum in Pb-Pb collisions at \u221as<sub>NN<\/sub> = 2.76 TeV\u201d, <em>Phys. Lett. <\/em><strong>B719<\/strong>, 18-28, 2013.<\/li>\n<li>A.Adare, <span style=\"text-decoration: underline;\">K.Homma<\/span>, <span style=\"text-decoration: underline;\">K.Shigaki<\/span>, <span style=\"text-decoration: underline;\">T.Sugitate<\/span>, <em>et al.<\/em>, \u201cAzimuthal anisotropy of pi0 and eta mesons  in Au+Au collisions at \u221as<sub>NN<\/sub> = 200 GeV\u201d, <em>Phys. Rev. C <\/em><strong>88<\/strong>, 064910, 2013.<\/li>\n<li>A.Adare, <span style=\"text-decoration: underline;\">K.Homma<\/span>, <span style=\"text-decoration: underline;\">K.Shigaki<\/span>, <span style=\"text-decoration: underline;\">T.Sugitate<\/span>, <em>et al.<\/em>, \u201cNuclear modification of psi\u2019, chic, and J\/psi\u3000  production in d+Au collisions at \u221as<sub>NN<\/sub> = 200 GeV\u201d, <em>Phys. Rev. Lett. <\/em><strong>111<\/strong>, 202301, 2013.<\/li>\n<li>A.Adare, <span style=\"text-decoration: underline;\">K.Homma<\/span>, <span style=\"text-decoration: underline;\">K.Shigaki<\/span>, <span style=\"text-decoration: underline;\">T.Sugitate<\/span>, <em>et al.<\/em>, \u201cSpectra and ratios of identified particles in Au+Au and d+Au collisions at \u221as<sub>NN<\/sub> = 200 GeV\u201d, <em>Phys. Rev. C <\/em><strong>88<\/strong>, 024906, 2013.<\/li>\n<li>A.Adare, <span style=\"text-decoration: underline;\">K.Homma<\/span>, <span style=\"text-decoration: underline;\">K.Shigaki<\/span>, <span style=\"text-decoration: underline;\">T.Sugitate<\/span>, <em>et al.<\/em>, \u201cQuadrupole anisotropy in dihadron azimuthal correlations in central d+Au collisions at \u221as<sub>NN<\/sub> = 200 GeV\u201d, <em>Phys. Rev. Lett. <\/em><strong>111<\/strong>, 212301, 2013.<\/li>\n<li>A.Adare, <span style=\"text-decoration: underline;\">K.Homma<\/span>, <span style=\"text-decoration: underline;\">K.Shigaki<\/span>, <span style=\"text-decoration: underline;\">T.Sugitate<\/span>, <em>et al.<\/em>, \u201cMedium modification of jet fragmentation     in Au+Au collisions at \u221as<sub>NN<\/sub> = 200 GeV measured in direct photon-hadron correlations\u201d, <em>Phys. Rev. Lett. <\/em><strong>111<\/strong>, 212301, 2013.<\/li>\n<li>A.Adare, <span style=\"text-decoration: underline;\">K.Homma<\/span>, <span style=\"text-decoration: underline;\">K.Shigaki<\/span>, <span style=\"text-decoration: underline;\">T.Sugitate<\/span>, <em>et al.<\/em>, \u201cUpsilon(1S+2S+3S) production in d+Au and p+p collisions at \u221as<sub>NN<\/sub> = 200 GeV and cold-nuclear matter effects\u201d, <em>Phys. Rev. C <\/em><strong>87<\/strong>, 044909, 2013.<\/li>\n<li>A.Adare, <span style=\"text-decoration: underline;\">K.Homma<\/span>, <span style=\"text-decoration: underline;\">K.Shigaki<\/span>, <span style=\"text-decoration: underline;\">T.Sugitate<\/span>, <em>et al.<\/em>, \u201cInclusive cross section and single transverse  spin asymmetry for very forward neutron production in polarized p+p collisions at \u221as = 200 GeV\u201d, <em>Phys. Rev. D <\/em><strong>88<\/strong>, 032006, 2013.<\/li>\n<li>A.Adare, <span style=\"text-decoration: underline;\">K.Homma<\/span>, <span style=\"text-decoration: underline;\">K.Shigaki<\/span>, <span style=\"text-decoration: underline;\">T.Sugitate<\/span>, <em>et al.<\/em>, \u201cDouble spin asymmetry of electrons from heavy flavor decays in p+p collisions at \u221as = 200 GeV\u201d, <em>Phys. Rev. D <\/em><strong>87<\/strong>, 012011, 2013.<\/li>\n<li>A.Adare, <span style=\"text-decoration: underline;\">K.Homma<\/span>, <span style=\"text-decoration: underline;\">K.Shigaki<\/span>, <span style=\"text-decoration: underline;\">T.Sugitate<\/span>, <em>et al.<\/em>, \u201cNeutral pion production with respect to centrality and reaction plane in Au+Au collisions at \u221as<sub>NN<\/sub> = 200 GeV\u201d, <em>Phys. Rev. C <\/em><strong>87<\/strong>, 034911, 2013.<<\/li>\n<li>A.Adare, <span style=\"text-decoration: underline;\">K.Homma<\/span>, <span style=\"text-decoration: underline;\">K.Shigaki<\/span>, <span style=\"text-decoration: underline;\">T.Sugitate<\/span>, <em>et al.<\/em>, \u201cDirect photon production in d+Au collisions at \u221as<sub>NN<\/sub> = 200 GeV\u201d, <em>Phys. Rev. C <\/em><strong>87<\/strong>, 054907, 2013.<\/li>\n<li>A.Adare, <span style=\"text-decoration: underline;\">K.Homma<\/span>, <span style=\"text-decoration: underline;\">K.Shigaki<\/span>, <span style=\"text-decoration: underline;\">T.Sugitate<\/span>, <em>et al.<\/em>, \u201cTransverse-momentum dependence of the J\/psi nuclear modification in d+Au collisions at \u221as<sub>NN<\/sub> = 200 GeV\u201d, <em>Phys. Rev. C <\/em><strong>87<\/strong>, 034904, 2013.<\/li>\n<li>Y.Nakamiya, <span style=\"text-decoration: underline;\">K.Homma<\/span>, \u201cMeasurability of f, w, and r mesons via di-electron decays in high-temperature states produced in heavy-ion collisions\u201d, <em>Progress of Theoretical Experimental Physics <\/em>(2013) <strong>11<\/strong>, 113H01.<\/li>\n<\/ul>\n\n<p><a id=\"presentations_H25\"><\/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>Y.Tanaka: \u201cELF and VLF observations of ionospheric disturbances caused by extra-terrestrial origin\u201d,   AGU meeting of the Americas (2013\/5\/14-17, Cancun, Mexico)<\/li>\n<li><span style=\"text-decoration: underline;\">Y.Fukazawa<\/span>: \u201cAstro-H, and future CAST mission\u201d, Understanding Relativistic Jets by Polarimetry     and Synergetic Study from Radio to TeV (Hiroshima University, Mar. 24-26, 2014)<\/li>\n<li><span style=\"text-decoration: underline;\">H.Takahashi<\/span>:\u201cLiCAF and BGO Phoswich Detectors for Simultaneous Measurements of Atmospheric Neutrons and Gamma-Rays\u201d, IEEE NSS\/MIC (2014\/10\/31, \u30bd\u30a6\u30eb, \u97d3\u56fd)<\/li>\n<li><span style=\"text-decoration: underline;\">H.Takahashi<\/span>:\u201cSuzaku Observation of the Symbiotic X-ray Binary IGR J16194-2810\u201d, Suzaku-MAXI 2014 (2014\/02\/19, \u611b\u5a9b\u5927\u5b66)<\/li>\n<li>T.Kawano: \u201cSuzaku-WAM soft gamma-ray all-sky monitor by the earth occultation technique\u201d, Suzaku-MAXI 2014 (2014\/02\/19, \u611b\u5a9b\u5927\u5b66)<\/li>\n<li>T.Tanabe: \u201cX-Ray investigation of the gamma-ray excess \u201cCygnus Cocoon\u201d by Suzaku\u201d, Suzaku-MAXI 2014 (2014\/02\/19, \u611b\u5a9b\u5927\u5b66) <\/li>\n<li>I.Edahiro: \u201cStudy of Fe-<em>K<\/em> Line Resonance Scattering in the Intracluster Medium with Monte-Carlo Simulation and Suzaku Data\u201d Suzaku-MAXI 2014 (2014\/02\/19, \u611b\u5a9b\u5927\u5b66)<\/li>\n<li>H.Shirakawa: \u201cStudy of the X-ray emission mechanism of a narrow-line radio-loud Seyfert 1 galaxy 1H0323+342 with Suzaku observations\u201d, Suzaku-MAXI 2014 (2014\/02\/19, \u611b\u5a9b\u5927\u5b66)<\/li>\n<li>T.Nakaoka: \u201cDevelopment of a Detector for High-Energy Astrophysical Objects Using a Conbination of Plastic Scintillator and MPPC\u201d, Suzaku-MAXI 2014 (2014\/02\/19, \u611b\u5a9b\u5927\u5b66) <\/li>\n<li><span style=\"text-decoration: underline;\">M.Ohno<\/span>: \u201cFuture Astro-H Observations of Gamma-ray Bursts\u201d, Huntsville GRB Symposium 2013,  (2013\/04\/14~04\/20, Nashville, USA)<\/li>\n<li><span style=\"text-decoration: underline;\">M.Ohno<\/span>: \u201cUpdate on MAXI-Fermi GRBs\u201d, Fermi-LAT Collaboration Meeting, (2013\/08\/26~08\/30, Stockholm, Sweden) <\/li>\n<li>Y.Tanaka: \u201cFermi Large Area Telescope detection of Two Very-high-energy Photons from the z=1.1 blazar PKS 0426- 380\u201d, Texas Symposium 2013 (2013\/12\/10~12\/13, Dallas, USA)<\/li>\n<li>R.Itoh: \u201cMinute-to-Hour Scale Rapid Variability of the Optical Polarization in the Relativistic Jets\u201d, Texas Symposium 2013 (2013\/12\/10~12\/13, Dallas, USA) <\/li>\n<li><span style=\"text-decoration: underline;\">Y.Fukazawa<\/span>: \u201cAstro-H, and future CAST mission\u201d, Understanding Relativistic Jets by Polarimetry and Synergetic Study from Radio to TeV, (Hiroshima University, Mar. 24-26, 2014).<\/li>\n<li>R.Itoh: \u201cStudy of Relativistic Jets with Optical Polarimetry and Multi-Wavelength Observation\u201d \u201cAstro-H, and future CAST mission\u201d, Understanding Relativistic Jets by Polarimetry and Synergetic Study from Radio to TeV, (Hiroshima University, Mar. 24-26, 2014).<\/li>\n<li><span style=\"text-decoration: underline;\">Y.Fukazawa<\/span>: \u201c1LAC FR\u2010I Radio Galaxies with Suzaku and Fermi 52month\u201d, Fermi-LAT Collaboration Meeting, (2013\/08\/26~08\/30, Stockholm, Sweden)<\/li>\n<li>Y.Tanaka: \u201cSub-TeV candidates inferred from hard spectra and possible VHE events during flaring states\u201d, Fermi-LAT Collaboration Meeting, (2013\/08\/26~08\/30, Stockholm, Sweden)<\/li>\n<li>R.Itoh: \u201cCTA 102 with Fermi and OISTER\u201d, Fermi-LAT Collaboration Meeting, (2013\/08\/26~ 08\/30, Stockholm, Sweden)<\/li>\n<li>T.Hayashi: \u201c14Status of the Third Quadrant Analysis with P7\u201d, Fermi-LAT Collaboration Meeting,  (2013\/08\/26~08\/30, Stockholm, Sweden)<\/li>\n<li>T.Mizuno: \u201cStatus of the Third Quadrant Analysis with P7 with P7\u201d, Fermi-LAT Collaboration  Meeting, (2014\/02\/17-21, SLAC, Stanford University)<\/li>\n<li>Y.Tanaka: \u201c5-year Pass 8 data analysis of Cen A lobe\u201d, Fermi-LAT Collaboration Meeting, (2014\/02\/17-21, SLAC, Stanford University)<\/li>\n<li>R.Itoh: \u201cShort term variability of CTA 102 in Pass 8 data\u201d, Fermi-LAT Collaboration Meeting,  (2014\/02\/17-21, SLAC, Stanford University) <\/li>\n<li>J.Katsuta: Update on G25.0+0.0 region; gamma-rays from a young massive star forming region?\u201d, Fermi-LAT Collaboration Meeting,( 2014\/02\/17-21, SLAC, Stanford University)<\/li>\n<li>K.Takaki: \u201cA Luminosu and Fast-Expanding Type Ib Supernova SN 2012au\u201d, Supernovae and Gamma-ray Bursts 2013, (2013\u5e7410\u670828\u65e5-11\u67081\u65e5, \u4eac\u90fd\u5927\u5b66) <\/li>\n<li>K.Takaki: \u201cPolarization observations of 5 GRB afterglows\u201d, Astronomical Polarimetry 2014: Polarisation as a tool to study the Solar System and beyon, (2014\u5e745\u670826-30\u65e5, MINATEC, France)<\/li>\n<li>K.Kawabata: \u201cPotential of TMT polarimetry\u201d, TMT Science and Instrumentation Workshop: Astronomy in the TMT Era, (2014\/10\/16-17, Asahi Seimei Ohtemachi Building, Tokyo)<\/li>\n<li>M.Garcia-Perez, A.Gonzalez-Arroyo, L.Keegan and <span style=\"text-decoration: underline;\">M.Okawa<\/span>, \u201cMass anomalous dimension from large N twisted volume reduction\u201d, PoS LATTICE2013 (2013) 098.<\/li>\n<li>A.Gonzalez-Arroyo and <span style=\"text-decoration: underline;\">M.Okawa<\/span>, \u201cTwisted reduction in large N QCD with adjoint Wilson fermions\u201d, PoS LATTICE2013 (2013) 099.<\/li>\n<li>M.Garcia-Perez, A.Gonzalez-Arroyo and <span style=\"text-decoration: underline;\">M.Okawa<\/span>, \u201cPerturbative analysis of twisted volume reduced theories\u201d, PoS LATTICE2013 (2013) 342.<\/li>\n<li><span style=\"text-decoration: underline;\">K.-I.Ishikawa<\/span>, \u201cTesting reweighting method for truncated Overlap fermions\u201d, 31<sup>st<\/sup> International Symposium on Lattice Field Theory LATTICE2013, (29 July-3 Aug.2013, Mainz, Germany) PoS (LATTICE 2013) 026.<\/li>\n<li><span style=\"text-decoration: underline;\">K.Yamamoto<\/span>, G.Huetsi, T.Kanemaru, A.Terukina, C.Hikage, \u201cHalo approach and testing gravity with redshift-space distortinos\u201d, PAPC-YITP collaboration : Mini-Workshop on Gravitation and Cosmology \uff082014\u5e74\uff12\u6708\uff15-\uff16\u65e5 YITP, Kyoto\uff09\uff08\u53c2\u52a0\u800560\u540d\uff09<\/li>\n<li>A.Terukina, <span style=\"text-decoration: underline;\">K<\/span><span style=\"text-decoration: underline;\">.<\/span><span style=\"text-decoration: underline;\">Yamamoto<\/span>, K.Koyama, D.Bacon, R.C.Nichol, L.Lombriser, \u201cHydrostatic equilibrium of gas distribution in Coma cluster and a test of chameleon gravity model\u201d, \uff08JGRG23, 2013\u5e7411\u6708\uff15-\uff18\u65e5, \u5f18\u524d\u5927\u5b66\uff09<\/li>\n<li>C.Hikage, <span style=\"text-decoration: underline;\">K<\/span><span style=\"text-decoration: underline;\">.<\/span><span style=\"text-decoration: underline;\">Yamamoto<\/span>: \u201cImpacts of satellite galaxies in measuring the cosmic growth rate\u201d,\uff08PASCOS2013, 2013\u5e7411\u670820-26\u65e5, Taipei, Taiwan\uff09<\/li>\n<li><span style=\"text-decoration: underline;\">T.Kato<\/span>, S.Ishiguro, H.Ohtani and K.Hagita, \u201cStudy of TOKI compression for plasma particle simulation\u201d, 23rd International Toki Conference (ITC-23) on Large-scale Simulation and Fusion Science (2013, 11\/18-21, Gifu)<\/li>\n<li><span style=\"text-decoration: underline;\">T.Sugitate<\/span>, \u201cRecent results in proton-lead collisions with ALICE at the LHC\u201d, APCTP 2013 LHC Physics Workshop at Korea (Seoul, Korea, 2013.8.6-8.8)<\/li>\n<li><span style=\"text-decoration: underline;\">T.Sugitate<\/span>, \u201cStatus of ALICE Tear-2 in Japan\u201d, Asia Forum 2013 for ALICE Tiers, (Daejeon, Korea, 2013.8.5)<\/li>\n<li><span style=\"text-decoration: underline;\">K.Homma<\/span>, \u201cLow energy stimulated photon-photon collider toward laboratory search for dark fields\u201d,   From Fundamental Physics to Societal Applications at the Embassy of France,(Tokyo, Japan, 2013.11.19)<\/li>\n<li><span style=\"text-decoration: underline;\">K.Homma<\/span>, \u201cProspect to search for sub-eV dark fields with high-intensity and high-energy lasers\u201d, 3<sup>rd<\/sup> IZEST meeting (Livermore, USA, 2013.07.17)<\/li>\n<li><span style=\"text-decoration: underline;\">K.Homma<\/span>, \u201cVacuum Quantum Optics \u2013 toward Search for sub-eV Dark Matter \/ Dark Energy  Candidates \u2013\u201d, 22nd International Laser Physics Workshop (Prague, Czeck Republic, 2013.07.15)<\/li>\n<li><span style=\"text-decoration: underline;\">K.Homma<\/span>, \u201cDark field search via photon-photon coupling at ELI-NP\u201d, Towards Technical Design Reports (TDR) of experiments with intense laser beams at ELI-NP, (Bucharest-Magurele, Romania, 2013.06.28)<\/li>\n<li><span style=\"text-decoration: underline;\">K.Homma<\/span>, \u201cRequired Laser System toward Laboratory Search for Low-mass Dark Matter and Dark     Energy Candidates\u201d, ICAN Conference (CERN, Geneva, Switzerland, 2013.06.27)<\/li>\n<li>\u6c34\u91ce\u6052\u53f2\uff1a\u201cDark Matter Search with Fermi Large Area Telescope\u201d, 2<sup>nd<\/sup> Workshop on Particle Physics and Dark Universe,\uff08\u6771\u4eac\u5927\u5b66, 2013\u5e74\uff14\u6708\uff14\u65e5\uff09<\/li>\n<li>\u6c34\u91ce\u6052\u53f2\uff1a\u201cRecent Results by Fermi-LAT and Future Prospects\u201d, \u9ad8\u5b87\u9023\u7814\u7a76\u4f1a\uff08\u91d1\u6ca2, 2013\u5e74\uff15\u6708\uff14\u65e5\uff09<\/li>\n<li><span style=\"text-decoration: underline;\">\u5927\u91ce\u96c5\u529f<\/span>\uff1a\u300c\u30d5\u30a7\u30eb\u30df\u885b\u661f\u3067\u898b\u305f\u30ac\u30f3\u30de\u7dda\u30d0\u30fc\u30b9\u30c8\u304b\u3089\u306e\u9ad8\u30a8\u30cd\u30eb\u30ae\u30fc\u653e\u5c04\u300d, \u7279\u5225\u63a8\u9032\u7814\u7a76\u4f1a\u30fb\u5b87\u5b99\u7dda\u7814\u7a76\u6240\u5171\u540c\u5229\u7528\u7814\u7a76\u4f1a\uff62\u9ad8\u30a8\u30cd\u30eb\u30ae\u30fc\u30ac\u30f3\u30de\u7dda\u3067\u307f\u308b\u6975\u9650\u5b87\u5b992013\uff63\uff082013\u5e74\uff19\u6708\uff13\uff5e\uff14\u65e5, \u6771\u4eac\u5927\u5b66\u67cf\u30ad\u30e3\u30f3\u30d1\u30b9\uff09<\/li>\n<li>\u7530\u4e2d\u5eb7\u4e4b\uff1a\u300c\u30d5\u30a7\u30eb\u30df\u885b\u661f\u3066\u3099\u89b3\u6e2c\u3057\u305f\u592a\u967d\uff0c\u30d5\u3099\u30ec\u30fc\u30b5\u3099\u30fc\u304b\u3089\u306eMeV\/GeV\u30ab\u3099\u30f3\u30de\u7dda\u653e\u5c04\u300d,\u7406\u8ad6\u5929\u6587\u5b66\u7814\u7a76\u4f1a\uff08\u6e6f\u6cb3\u539f\uff0c2013\u5e7410\u6708\uff09<\/li>\n<li><span style=\"text-decoration: underline;\">\u6df1\u6ca2\u6cf0\u53f8<\/span>\uff1a\u300c\u30d5\u30a7\u30eb\u30df\u885b\u661f\u306b\u3088\u308bAGN\u30b8\u30a7\u30c3\u30c8\u653e\u5c04\u306e\u89b3\u6e2c\u3068ALMA\u3068\u306e\u95a2\u9023\u300d, \u7814\u7a76\u4f1a\u300cALMA\u3067\u63a2\u308b\u30d6\u30e9\u30c3\u30af\u30db\u30fc\u30eb\u9ad8\u30a8\u30cd\u30eb\u30ae\u30fc\u73fe\u8c61\u300d,\uff082013\u5e74\uff19\u670825-26\u65e5\uff0c\u56fd\u7acb\u5929\u6587\u53f0\u4e09\u9df9\uff09<\/li>\n<li><span style=\"text-decoration: underline;\">\u6df1\u6ca2\u6cf0\u53f8<\/span>\uff1a\u300c\u30ac\u30f3\u30de\u7dda\u306b\u3088\u308b\u9280\u6cb3\u56e3\u306e\u89b3\u6e2c\u306e\u73fe\u72b6\u3068\u4eca\u5f8c\u300d, \u30ef\u30fc\u30af\u30b7\u30c3\u30d7\u300c\u9280\u6cb3\u56e3\u306e\u7269\u7406\u300d\uff082013\u5e7412\u670828\u65e5\uff0c\u6771\u4eac\u7406\u79d1\u5927\u5b66\uff09<\/li>\n<li><span style=\"text-decoration: underline;\">\u6df1\u6ca2\u6cf0\u53f8<\/span>\uff1a\u300cNGC1365 \u306eFe-K\u5438\u53ce\u7dda\u306e\u6642\u9593\u5909\u5316\u3068\u786c\uff38\u7dda\u89b3\u300d\u79cb\u5b63\u5929\u6587\u5b66\u4f1a\uff082013\u5e74\uff19\u670810-12\u65e5\uff0c\u6771\u5317\u5927\u5b66\uff09<\/li>\n<li><span style=\"text-decoration: underline;\">\u9ad8\u6a4b\u5f18\u5145<\/span>\uff1a\u300cPoGOLite \u6c17\u7403\u5b9f\u9a13\uff1a2013\u5e74\u306e\u30d1\u30b9\u30d5\u30a1\u30a4\u30f3\u30c0\u30fc\u30d5\u30e9\u30a4\u30c8\u300d\u79cb\u5b63\u5929\u6587\u5b66\u4f1a\uff082013\u5e74\uff19\u670810-12\u65e5\uff0c\u6771\u5317\u5927\u5b66\uff09<<\/li>\n<li><span style=\"text-decoration: underline;\">\u5927\u91ce\u96c5\u529f<\/span>\uff1a\u300c\u3059\u3056\u304f\u885b\u661f\u642d\u8f09\u5e83\u5e2f\u57df\u5168\u5929\u30e2\u30cb\u30bf\u306b\u3088\u308b\u592a\u967d\u30d5\u30ec\u30a2\u89b3\u6e2c\u300d\u79cb\u5b63\u5929\u6587\u5b66\u4f1a\uff082013\u5e74\uff19\u670810-12\u65e5\uff0c\u6771\u5317\u5927\u5b66\uff09<\/li>\n<li>\u79cb\u7530\u8c37\u6d0b\uff1a\u300c\u53ef\u8996\u8d64\u5916\u7dda\u540c\u6642\u30ab\u30e1\u30e9HONIR: \u5206\u5149\u6a5f\u80fd\u642d\u8f09\u3068\u8a66\u9a13\u89b3\u6e2c\u300d\u79cb\u5b63\u5929\u6587\u5b66\u4f1a\uff082013\u5e74\uff19\u670810-12\u65e5\uff0c\u6771\u5317\u5927\u5b66\uff09<\/li>\n<li>\u4f0a\u85e4\u4eae\u4ecb\uff1a\u300cNarrow-line Seyfert 1\u578b\u9280\u6cb3PMN J0948+0022\u306b\u304a\u3051\u308b\u5206\u30b9\u30b1\u30fc\u30eb\u3067\u306e\u53ef\u8996\u504f\u5149\u5909\u52d5\u89b3\u6e2c\u89b3\u6e2c\u300d\uff0c\u79cb\u5b63\u5929\u6587\u5b66\u4f1a\uff082013\u5e74\uff19\u670810-12\u65e5\uff0c\u6771\u5317\u5927\u5b66\uff09<\/li>\n<li>\u6d66\u91ce\u525b\u5fd7\uff1a\u300c\u30d6\u30ec\u30fc\u30b6\u30fcS5 0716+714 \u306e\u591a\u6ce2\u9577\u89b3\u6e2c\u306b\u3088\u308b\u6642\u9593\u5909\u52d5\u89e3\u6790\u300d\u79cb\u5b63\u5929\u6587\u5b66\u4f1a\uff082013\u5e74\uff19\u670810-12\u65e5\uff0c\u6771\u5317\u5927\u5b66\uff09<\/li>\n<li>\u6cb3\u91ce\u8cb4\u6587\uff1a\u300c\u5b87\u5b99\u786c\uff38\u7dda\u504f\u5149\u691c\u51fa\u5668PoGOLite\u6c17\u7403\u5b9f\u9a13\u306e\u5730\u4e0a\u8f03\u6b63\u8a66\u9a13\u300d\u79cb\u5b63\u5929\u6587\u5b66\u4f1a\uff082013\u5e74\uff19\u670810-12\u65e5\uff0c\u6771\u5317\u5927\u5b66\uff09<\/li>\n<li>\u9ad8\u6728\u52dd\u4fca\uff1a\u300c\u6975\u8d85\u65b0\u661f\u306b\u985e\u4f3c\u3057\u305f\u8fd1\u508dIb \u578b\u8d85\u65b0\u661fSN 2012au \u306e\u5f8c\u671f\u89b3\u6e2c\u300d\u79cb\u5b63\u5929\u6587\u5b66\u4f1a\uff082013\u5e74\uff19\u670810-12\u65e5\uff0c\u6771\u5317\u5927\u5b66\uff09<\/li>\n<li>\u5fb3\u7530\u4f38\u77e2\uff1a\u300cASTRO-H\u885b\u661f\u642d\u8f09\u578b\u30a2\u30af\u30c6\u30a3\u30d6\u30b7\u30fc\u30eb\u30c9\u7cfb\u306e\u53d7\u3051\u5165\u308c\u8a66\u9a13\u53ca\u3073\u52d5\u4f5c\u691c\u8a3c\u300d\u79cb\u5b63\u5929\u6587\u5b66\u4f1a\uff082013\u5e74\uff19\u670810-12\u65e5\uff0c\u6771\u5317\u5927\u5b66\uff09<\/li>\n<li>\u6cb3\u53e3\u8ce2\u81f3\uff1a\u300cRadio-loud Narrow-line Seyfert 1 Galaxies\u306e\u53ef\u8996\u504f\u5149\u89b3\u6e2c\u300d\u79cb\u5b63\u5929\u6587\u5b66\u4f1a\uff082013\u5e74\uff19\u670810-12\u65e5\uff0c\u6771\u5317\u5927\u5b66\uff09<\/li>\n<li>\u6797\u5b5d\u5178\uff1a\u300c\u30d5\u30a7\u30eb\u30df\u30fb\u30ac\u30f3\u30de\u7dda\u5b87\u5b99\u671b\u9060\u93e1\u306b\u3088\u308b\u9280\u6cb3\u9762\u30ac\u30f3\u30de\u7dda\u653e\u5c04(The 3rd glactic quadrant)\u306e\u89e3\u6790\u300d\uff0c\u79cb\u5b63\u5929\u6587\u5b66\u4f1a\uff082013\u5e74\uff19\u670810-12\u65e5\uff0c\u6771\u5317\u5927\u5b66\uff09><\/li>\n<li>\u53e4\u4e95\u4fca\u4e5f\uff1a\u300cASTRO-H\u642d\u8f09\u8edf\u30ac\u30f3\u30de\u7dda\u691c\u51fa\u5668\u30b3\u30f3\u30d7\u30c8\u30f3\u30ab\u30e1\u30e9\u30fb\u30a8\u30f3\u30b8\u30cb\u30a2\u30ea\u30f3\u30b0\u30e2\u30c7\u30eb\u306e\u6027\u80fd\u8a55\u4fa1\u300d\uff0c\u79cb\u5b63\u5929\u6587\u5b66\u4f1a\uff082013\u5e74\uff19\u670810-12\u65e5\uff0c\u6771\u5317\u5927\u5b66\uff09<\/li>\n<li><span style=\"text-decoration: underline;\">\u9ad8\u6a4b\u5f18\u5145<\/span>\uff1a\u300c\u786c\uff38\u7dda\u504f\u5149\u691c\u51fa\u5668PoGOLite\u6c17\u7403\u5b9f\u9a13 2013\u5e74\u30d1\u30b9\u30d5\u30a1\u30a4\u30f3\u30c0\u30fc\u30d5\u30e9\u30a4\u30c8\u300d\u79cb\u5b63\u7269\u7406\u5b66\u4f1a\uff082013\u5e74\uff19\u670820-23\u65e5\uff0c\u9ad8\u77e5\u5927\u5b66\uff09<\/li>\n<li><span style=\"text-decoration: underline;\">\u9ad8\u6a4b\u5f18\u5145<\/span>\uff1a\u300cPoGOLino\u6c17\u7403\u5b9f\u9a13\u3067\u8a08\u6e2c\u3057\u305f\u6c17\u7403\u9ad8\u5ea6\u3067\u306e\u4e2d\u6027\u5b50\u30d0\u30c3\u30af\u30b0\u30e9\u30a6\u30f3\u30c9\u300d\u6625\u5b63\u5929\u6587\u5b66\u4f1a\uff082014\u5e74\uff13\u670819-22\u65e5\uff0c\u56fd\u969b\u57fa\u7763\u6559\u5927\u5b66\uff09<\/li>\n<li>\u5927\u91ce\u96c5\u529f\uff1a\u300cASTRO-H\u885b\u661f\u642d\u8f09\u8edf\u30ac\u30f3\u30de\u7dda\u691c\u51fa\u5668(SGD)\u958b\u767a\u306e\u73fe\u72b6\u300d\u6625\u5b63\u5929\u6587\u5b66\u4f1a\uff082014\u5e74\uff13\u670819-22\u65e5\uff0c\u56fd\u969b\u57fa\u7763\u6559\u5927\u5b66\uff09<\/li>\n<li>\u4f0a\u85e4\u4eae\u4ecb\uff1a\u300c\u76f8\u5bfe\u8ad6\u30b8\u30a7\u30c3\u30c8\u306b\u304a\u3051\u308b\u53ef\u8996\u504f\u5149\u65b9\u4f4d\u89d2\u3068\u96fb\u6ce2\u30b8\u30a7\u30c3\u30c8\u4f4d\u7f6e\u89d2\u3068\u306e\u76f8\u95a2\u300d\u6625\u5b63\u5929\u6587\u5b66\u4f1a\uff082014\u5e74\uff13\u670819-22\u65e5\uff0c\u56fd\u969b\u57fa\u7763\u6559\u5927\u5b66\uff09<\/li>\n<li>\u9ad8\u6728\u52dd\u4fca\uff1a\u300c\u521d\u3081\u3066\u89aa\u661f\u304c\u76f4\u63a5\u540c\u5b9a\u3055\u308c\u305fIb\u578b\u8d85\u65b0\u661fiPTF13bvn\u306e\u521d\u671f\u89b3\u6e2c\u300d\u6625\u5b63\u5929\u6587\u5b66\u4f1a\uff082014\u5e74\uff13\u670819-22\u65e5\uff0c\u56fd\u969b\u57fa\u7763\u6559\u5927\u5b66\uff09<\/li>\n<li>\u7530\u9089\u5229\u660e\uff1a\u300c\u300c\u3059\u3056\u304f\u300d\u306b\u3088\u308b\u30ac\u30f3\u30de\u7dda\u8d85\u904eCygnus Cocoon\u306e\uff38\u7dda\u8abf\u67fb\u300d\u6625\u5b63\u5929\u6587\u5b66\u4f1a\uff082014\u5e74\uff13\u670819-22\u65e5\uff0c\u56fd\u969b\u57fa\u7763\u6559\u5927\u5b66\uff09<\/li>\n<li>\u5fb3\u7530\u4f38\u77e2\uff1a\u300cASTRO-H\u885b\u661f\u642d\u8f09\u786c\uff38\u7dda\u64ae\u50cf\u691c\u51fa\u5668\u306eEnd-to-End\u8a66\u9a13\u306b\u3088\u308b\u30a2\u30af\u30c6\u30a3\u30d6\u30b7\u30fc\u30eb\u30c9\u306e\u6a5f\u80fd\u691c\u8a3c\u6e2c\u300d\uff0c\u6625\u5b63\u5929\u6587\u5b66\u4f1a\uff082014\u5e74\uff13\u670819-22\u65e5\uff0c\u56fd\u969b\u57fa\u7763\u6559\u5927\u5b66\uff09<\/li>\n<li><span style=\"text-decoration: underline;\">\u9ad8\u6a4b\u5f18\u5145<\/span>\uff1a\u300cPoGOLino\u6c17\u7403\u5b9f\u9a13\u306b\u3088\u308b\u5927\u6c17\u4e2d\u6027\u5b50\u30d5\u30e9\u30c3\u30af\u30b9\u306e\u8a08\u6e2c\u300d\u6625\u5b63\u7269\u7406\u5b66\u4f1a\uff082014\u5e74\uff13\u670827-30\u65e5\uff0c\u6771\u6d77\u5927\u5b66\u6e58\u5357\u30ad\u30e3\u30f3\u30d1\u30b9\uff09<\/li>\n<li>\u5927\u91ce\u96c5\u529f\uff1a\u300cASTRO-H\u885b\u661f\u642d\u8f09\u786c\uff38\u7dda\u8edf\u30ac\u30f3\u30de\u7dda\u691c\u51fa\u5668\u306b\u304a\u3051\u308bBGO\u30a2\u30af\u30c6\u30a3\u30d6\u30b7\u30fc\u30eb\u30c9\u306e\u958b\u767a\u72b6\u6cc1\u300d\uff0c\u6625\u5b63\u7269\u7406\u5b66\u4f1a\uff082014\u5e74\uff13\u670827-30\u65e5\uff0c\u6771\u6d77\u5927\u5b66\u6e58\u5357\u30ad\u30e3\u30f3\u30d1\u30b9\uff09<\/li>\n<li>\u4e2d\u5ddd\u5d07\u4e4b\uff1a\u300c\u643a\u5e2f\u578b\u653e\u5c04\u7dda\u691c\u51fa\u5668\u306e\u958b\u767a\u306b\u3080\u3051\u305fMPPC\u306e\u500b\u6027\u6e2c\u5b9a\u300d\u6625\u5b63\u7269\u7406\u5b66\u4f1a\uff082014\u5e74\uff13\u670827-30\u65e5\uff0c\u6771\u6d77\u5927\u5b66\u6e58\u5357\u30ad\u30e3\u30f3\u30d1\u30b9\uff09<\/li>\n<li>\u4e2d\u6751\u7adc\uff1a\u300cASTRO-H\u642d\u8f09\u8edf\u30ac\u30f3\u30de\u7dda\u691c\u51fa\u5668\u4e3b\u691c\u51fa\u90e8\u72ed\u8996\u91ce\u591a\u5c64\u534a\u5c0e\u4f53\u30b3\u30f3\u30d7\u30c8\u30f3\u30ab\u30e1\u30e9\u96fb\u6c17\u8a66\u9a13\u9032\u6357\u5831\u544a\u300d\uff0c\u6625\u5b63\u7269\u7406\u5b66\u4f1a\uff082014\u5e74\uff13\u670827-30\u65e5\uff0c\u6771\u6d77\u5927\u5b66\u6e58\u5357\u30ad\u30e3\u30f3\u30d1\u30b9\uff09<\/li>\n<li>\u68ee\u5065\u5f70\uff1a\u300cKWFC\u3092\u7528\u3044\u305f\u8fd1\u508d\u8d85\u65b0\u661f\u306e\u63a2\u67fb\u300d, \u6728\u66fd\u30b7\u30e5\u30df\u30c3\u30c8\u30b7\u30f3\u30dd\u30b8\u30a6\u30e02013\u3000\uff082013\u5e74\uff17\u6708\uff19\u65e5-10\u65e5\uff0c\u6728\u66fd\u90e1\u6c11\u4f1a\u9928\uff09<\/li>\n<li>\u6cb3\u53e3\u8ce2\u81f3\uff1a\u300cRadio-loud Narrow-line Seyfert 1 Galaxies\u306e\u53ef\u8996\u504f\u5149\u89b3\u6e2c\u300d\u7b2c24\u56de\u5149\u8d64\u5916\u30e6\u30fc\u30b6\u30fc\u30ba\u30df\u30fc\u30c6\u30a3\u30f3\u30b0\uff082013\u5e74\uff18\u6708\uff11\u65e5-\uff13\u65e5\uff0c\u5009\u6577\u5e02\u7acb\u7f8e\u8853\u9928\uff09<\/li>\n<li>\u68ee\u5065\u5f70\uff1a\u300c\u6697\u3044IIP\u578b\u8d85\u65b0\u661f\u7206\u767a SN2013am\u306e\u53ef\u8996\u30fb\u8fd1\u8d64\u5916\u7dda\u3067\u306e\u89b3\u6e2c\u300d\u7b2c24\u56de\u5149\u8d64\u5916\u30e6\u30fc\u30b6\u30fc\u30ba\u30df\u30fc\u30c6\u30a3\u30f3\u30b0\uff082013\u5e74\uff18\u6708\uff11\u65e5-\uff13\u65e5\uff0c\u5009\u6577\u5e02\u7acb\u7f8e\u8853\u9928\uff09<\/li>\n<li>\u4f0a\u85e4\u4eae\u4ecb\uff1a\u300c\u5927\u5b66\u9593\u9023\u643a\u3092\u7528\u3044\u305f\u30d6\u30ec\u30fc\u30b6\u30fc\u5929\u4f53CTA102\u306e\u77ed\u671f\u6642\u9593\u5909\u52d5\u89b3\u6e2c\u300d\u7b2c24\u56de\u5149\u8d64\u5916\u30e6\u30fc\u30b6\u30fc\u30ba\u30df\u30fc\u30c6\u30a3\u30f3\u30b0\uff082013\u5e74\uff18\u6708\uff11\u65e5-\uff13\u65e5\uff0c\u5009\u6577\u5e02\u7acb\u7f8e\u8853\u9928\uff09<\/li>\n<li>\u6d66\u91ce\u525b\u5fd7\uff1a\u300c\u30d6\u30ec\u30fc\u30b6\u30fcS5 0716+714 \u306e\u591a\u6ce2\u9577\u89b3\u6e2c\u306b\u3088\u308b\u6642\u9593\u5909\u52d5\u89e3\u6790\u300d\u7b2c24\u56de\u5149\u8d64\u5916\u30e6\u30fc\u30b6\u30fc\u30ba\u30df\u30fc\u30c6\u30a3\u30f3\u30b0\uff082013\u5e74\uff18\u6708\uff11\u65e5-\uff13\u65e5\uff0c\u5009\u6577\u5e02\u7acb\u7f8e\u8853\u9928\uff09<\/li>\n<li>\u4e0a\u91ce\u4e00\u8aa0\uff1a\u300c\u6975\u3081\u3066\u660e\u308b\u3044IIn\u578b\u8d85\u65b0\u661f SN 2010jl \u306e\u53ef\u8996\u3068\u8fd1\u8d64\u5916\u306b\u3088\u308b\u5f8c\u671f\u89b3\u6e2c\u300d\u7b2c24\u56de\u5149\u8d64\u5916\u30e6\u30fc\u30b6\u30fc\u30ba\u30df\u30fc\u30c6\u30a3\u30f3\u30b0\uff082013\u5e74\uff18\u6708\uff11\u65e5-\uff13\u65e5\uff0c\u5009\u6577\u5e02\u7acb\u7f8e\u8853\u9928\uff09<\/li>\n<li>\u9ad8\u6728\u52dd\u4fca\uff1a\u300cGRB-SN\u3068\u95a2\u9023\u304c\u3042\u308bIb\u578b\u8d85\u65b0\u661f SN 2012au\u300d\u7b2c24\u56de\u5149\u8d64\u5916\u30e6\u30fc\u30b6\u30fc\u30ba\u30df\u30fc\u30c6\u30a3\u30f3\u30b0\uff082013\u5e74\uff18\u6708\uff11\u65e5-\uff13\u65e5\uff0c\u5009\u6577\u5e02\u7acb\u7f8e\u8853\u9928\uff09<\/li>\n<li>\u5b87\u4e95\u5d07\u7d18\uff1a\u300c\u304b\u306a\u305f\u671b\u9060\u93e1\u7528\u8d64\u5916\u7dda\u691c\u51fa\u5668\u306e\u8aad\u307f\u51fa\u3057\u30b7\u30b9\u30c6\u30e0\u306e\u958b\u767a\u300d\u7b2c24\u56de\u5149\u8d64\u5916\u30e6\u30fc\u30b6\u30fc\u30ba\u30df\u30fc\u30c6\u30a3\u30f3\u30b0\uff082013\u5e74\uff18\u6708\uff11\u65e5-\uff13\u65e5\uff0c\u5009\u6577\u5e02\u7acb\u7f8e\u8853\u9928\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\u691c\u51fa\u5668\u8aad\u307f\u51fa\u3057\u56de\u8def\u306e\u958b\u767a\u300d\u7b2c\uff13\u56de\u53ef\u8996\u8d64\u5916\u7dda\u89b3\u6e2c\u88c5\u7f6e\u6280\u8853\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d7\uff082013\u5e7412\u670817\u65e5-18\u65e5\uff0c\u4eac\u90fd\u5927\u5b66\uff09<\/li>\n<li>\u9ad8\u6728\u52dd\u4fca\uff1a\u300cIb\u578b\u8d85\u65b0\u661f SN2012au - GRB\u4ed8\u968f\u578b\u8d85\u65b0\u661f\u3068\u306e\u30ea\u30f3\u30af\u300d2013\u5e74\u5ea6\u5929\u6587\u30fb\u5929\u4f53\u7269\u7406\u82e5\u624b\u590f\u306e\u5b66\u6821\uff082013\u5e74\uff17\u670829\u65e5-\uff18\u6708\uff11\u65e5\uff0c\u5bae\u57ce\u8535\u738b\u30ed\u30a4\u30e4\u30eb\u30db\u30c6\u30eb\uff09<\/li>\n<li>\u9ad8\u6728\u52dd\u4fca\uff1a\u300c\u5916\u5c64\u3092\u5265\u304e\u53d6\u3089\u308c\u305f\u91cd\u529b\u5d29\u58ca\u578b\u8d85\u65b0\u661f\u306e\u591a\u30d0\u30f3\u30c9\u6e2c\u5149\u30fb\u5206\u5149\u89b3\u6e2c\u306b\u3088\u308b\u7206\u767a\u8a3a\u65ad\u300d\u7b2c3\u56de\u5927\u5b66\u9593\u9023\u643a\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d7\uff082013\u5e7412\u670810-11\u65e5\uff0c\u897f\u306f\u308a\u307e\u5929\u6587\u53f0\uff09<\/li>\n<li>\u4f0a\u85e4\u4eae\u4ecb\uff1a\u300c\u6d3b\u52d5\u9280\u6cb3\u6838\u306e\u77ed\u6642\u9593\u5909\u52d5\u89b3\u6e2c\u3068CTA102\u591a\u6ce2\u9577\u89b3\u6e2c\u300d\u7b2c\uff13\u56de\u5927\u5b66\u9593\u9023\u643a\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d7\uff082013\u5e7412\u670810-11\u65e5\uff0c\u897f\u306f\u308a\u307e\u5929\u6587\u53f0\uff09<\/li>\n<li><span style=\"text-decoration: underline;\">\u9ad8\u6a4b\u5f18\u5145<\/span>\uff1a\u300cPoGOLite\u6c17\u7403\u5b9f\u9a13 2013\u5e74\u306e\u30d1\u30b9\u30d5\u30a1\u30a4\u30f3\u30c0\u30fc\u30d5\u30e9\u30a4\u30c8\u306e\u72b6\u6cc1\u3068\u4eca\u5f8c\u300d\u5927\u6c17\u7403\u30b7\u30f3\u30dd\u30b8\u30a6\u30e0\uff082013\u5e7411\u670814\u65e5, \u5b87\u5b99\u822a\u7a7a\u7814\u7a76\u958b\u767a\u6a5f\u69cb\u30fb\u5b87\u5b99\u79d1\u5b66\u7814\u7a76\u6240\uff09<\/li>\n<li><span style=\"text-decoration: underline;\">\u9ad8\u6a4b\u5f18\u5145<\/span>\uff1a\u300c\u786c\uff38\u7dda\u504f\u5149\u691c\u51fa\u5668PoGOLite\u6c17\u7403\u5b9f\u9a13\uff1a2013\u5e74\u306e\u30d1\u30b9\u30d5\u30a1\u30a4\u30f3\u30c0\u30fc\u30d5\u30e9\u30a4\u30c8\u300d\u5b87\u5b99\u79d1\u5b66\u30b7\u30f3\u30dd\u30b8\u30a6\u30e0\uff082014\u5e74\uff11\u6708\uff19\u65e5-10\u65e5, \u5b87\u5b99\u822a\u7a7a\u7814\u7a76\u958b\u767a\u6a5f\u69cb\u30fb\u5b87\u5b99\u79d1\u5b66\u7814\u7a76\u6240\uff09<\/li>\n<li>\u4f0a\u85e4\u4eae\u4ecb\uff1a\u300c\u6d3b\u52d5\u9280\u6cb3\u6838\u30b8\u30a7\u30c3\u30c8\u306e\u8d64\u5916\u7dda\u30fb\u591a\u6ce2\u9577\u89b3\u6e2c\u300dMIMIZUKU science WS\uff082013\/5\/24, \u6771\u4eac\u5927\u5b66\u5929\u6587\u5b66\u6559\u80b2\u7814\u7a76\u30bb\u30f3\u30bf\u30fc\uff09<\/li>\n<li>\u679d\u5ee3\u80b2\u5b9f\uff1a\u300c\u9280\u6cb3\u56e3\u30d7\u30e9\u30ba\u30de\u3067\u306eFe-K\u30e9\u30a4\u30f3\u5171\u9cf4\u6563\u4e71\u306e\u30b7\u30df\u30e5\u30ec\u30fc\u30b7\u30e7\u30f3\u300d\u3000\uff38\u7dda\u9280\u6cb3\u56e3\u7814\u7a76\u4f1a\uff082013\u5e7412\u670827\u65e5, \u6771\u4eac\u7406\u79d1\u5927\u5b66\uff09<\/li>\n<li>\u6cb3\u91ce\u8cb4\u6587\uff1a\u300c\u5b87\u5b99\u786c\uff38\u7dda\u691c\u51fa\u5668PoGOLite\u6c17\u7403\u5b9f\u9a13\u306e\u5730\u4e0a\u8f03\u6b63\u8a66\u9a13\u300d\u5b87\u5b99\u7dda\u7814\u7a76\u6240\u5bfa\u6ca2\u7814\u30bb\u30df\u30ca\u30fc\uff082013\u5e74\uff15\u670817\u65e5\uff0c\u6771\u4eac\u5927\u5b66\u5b87\u5b99\u7dda\u7814\uff09<\/li>\n<li>\u6cb3\u91ce\u8cb4\u6587\uff1a\u201cPathfinder flight of Polarized Gamma-ray Observer (PoGOLite) in 2013\u201d,\u6771\u4eac\u5927\u5b66\u7406\u5b66\u7814\u7a76\u79d1\u7269\u7406\u79d1\u5b66\u5c02\u653b\u7267\u5cf6\u4e2d\u6fa4\u7814\u30bb\u30df\u30ca\u30fc\uff082013\u5e7412\u670818\u65e5\uff0c\u6771\u4eac\u5927\u5b66\u672c\u90f7\u30ad\u30e3\u30f3\u30d1\u30b9\uff09<\/li>\n<li>\u68ee\u8c37\u53cb\u7531\u5e0c\uff1a\u300c\u53ef\u8996\u8fd1\u8d64\u5916\u7dda\u540c\u6642\u30ab\u30e1\u30e9 HONIR\u958b\u767a\u306e\u9032\u6357\u72b6\u6cc1\u300d\u7b2c24\u56de\u5149\u8d64\u5916\u30e6\u30fc\u30b6\u30fc\u30ba\u30df\u30fc\u30c6\u30a3\u30f3\u30b0\uff082013\u5e74\uff18\u6708\uff11\u65e5-\uff13\u65e5\uff0c\u5009\u6577\u5e02\u7acb\u7f8e\u8853\u9928\uff09<\/li>\n<li>\u5409\u7530\u9053\u5229\uff1a\u300c\u5e83\u5cf6\u5927\u306e\u6d3b\u52d5\u5831\u544a\u300d\uff0c\u7b2c24\u56de\u5149\u8d64\u5916\u30e6\u30fc\u30b6\u30fc\u30ba\u30df\u30fc\u30c6\u30a3\u30f3\u30b0\uff082013\u5e74\uff18\u6708\uff11\u65e5-\uff13\u65e5\uff0c\u5009\u6577\u5e02\u7acb\u7f8e\u8853\u9928\uff09<\/li>\n<li>\u690d\u6751\u8aa0\uff1a\u300c\u304b\u306a\u305f\u671b\u9060\u93e1\u30fb\u89b3\u6e2c\u88c5\u7f6e\u4f7f\u7528\u72b6\u6cc1\u300d\uff0c \u7b2c24\u56de\u5149\u8d64\u5916\u30e6\u30fc\u30b6\u30fc\u30ba\u30df\u30fc\u30c6\u30a3\u30f3\u30b0\uff082013\u5e74\uff18\u6708\uff11\u65e5-\uff13\u65e5\uff0c\u5009\u6577\u5e02\u7acb\u7f8e\u8853\u9928\uff09<\/li>\n<li>\u79cb\u7530\u8c37\u6d0b\uff1a\u300c\u304b\u306a\u305f\u671b\u9060\u93e1\u306e\u88c5\u7f6e\u958b\u767a\u300d\uff0c \u7b2c24\u56de\u5149\u8d64\u5916\u30e6\u30fc\u30b6\u30fc\u30ba\u30df\u30fc\u30c6\u30a3\u30f3\u30b0\uff082013\u5e74\uff18\u6708\uff11\u65e5-\uff13\u65e5\uff0c\u5009\u6577\u5e02\u7acb\u7f8e\u8853\u9928\uff09<\/li>\n<li><span style=\"text-decoration: underline;\">\u5927\u5ddd\u6b63\u5178<\/span>, \u201cRecent progress in twisted space-time reduction in large N QCD\u201d, \u300c\u96e2\u6563\u7684\u624b\u6cd5\u306b\u3088\u308b\u5834\u3068\u6642\u7a7a\u306e\u30c0\u30a4\u30ca\u30df\u30af\u30b9\u300d\u7814\u7a76\u4f1a\uff089\u670827\u65e5\uff0d30\u65e5\uff0c\u9ad8\u30a8\u30cd\u30eb\u30ae\u30fc\u52a0\u901f\u5668\u7814\u7a76\u6a5f\u69cb\uff09<\/li>\n<li><span style=\"text-decoration: underline;\">\u4e21\u89d2\u5353\u4e5f<\/span>, \u5927\u517c\u82f1\u6717, \u6885\u679d\u5b8f\u4e4b\uff0c\u201cTesting T and CPT violation using B meson system \u2013 validity and limit of CP tagging \u2013\u201d\uff082014\u5e74\uff12\u670820\u65e5\uff0c\u7b2c13\u56de B\u30d5\u30a1\u30af\u30c8\u30ea\u30fc\u7269\u7406\u52c9\u5f37\u4f1a\uff0c\u540d\u53e4\u5c4b\u5927\u5b66\uff09\uff08\u4e00\u822c\u8b1b\u6f14\uff09<\/li>\n<li><span style=\"text-decoration: underline;\">\u77f3\u5ddd\u5065\u4e00<\/span>\uff0c\u6728\u6751\u5927\u81ea\uff0c<span style=\"text-decoration: underline;\">\u5fd7\u57a3\u8ce2\u592a<\/span>\uff0c\u8fbb\u4e9c\u7d17\u5b50\uff1a\u201c\u5f37\u78c1\u5834\u4e2d\u3067\u306e\u5149\u5b50\uff12\u70b9\u95a2\u6570\u306e\u30d5\u30a7\u30eb\u30df\u30aa\u30f3\uff11\u30eb\u30fc\u30d7\u8a08\u7b97\u306e\u6570\u5024\u89e3\u6790\u306b\u3064\u3044\u3066\u201d,\u65e5\u672c\u7269\u7406\u5b66\u4f1a\u30002013\u5e74\u79cb\u5b63\u5927\u4f1a\uff08\uff19\u670821\u65e5\uff0c\u9ad8\u77e5\u5927\u5b66\uff09<\/li>\n<li>T. Morozumi, \u201cTime reversal and CPT in Neutral B meson system: Review\u201d , \u7b2c12\u56de\uff22\u30d5\u30a1\u30af\u30c8\u30ea\u30fc\u7269\u7406\u52c9\u5f37\u4f1a\uff0810\u670828\u65e5\uff0c\u5927\u962a\u5927\u5b66\uff09<\/li>\n<li><span style=\"text-decoration: underline;\">\u52a0\u85e4\u6052\u5f66<\/span>\uff1a\u300c\u78c1\u6c17\u4e0d\u5b89\u5b9a\u306e\u975e\u7dda\u578b\u767a\u5c55\u306b\u4f34\u3046\u7121\u885d\u7a81\u885d\u6483\u6ce2\u300d, \u65e5\u672c\u7269\u7406\u5b66\u4f1a 2013\u5e74\u79cb\u5b63\u5927\u4f1a\uff082013\u5e74\uff19\u670827\u65e5\uff0c\u5fb3\u5cf6\u5927\u5b66\uff09<\/li>\n<li><span style=\"text-decoration: underline;\">\u5c0f\u5d8c\u5eb7\u53f2<\/span>\uff1a\u300c\u6bbb\u306b\u5c40\u5728\u3057\u305f\u78c1\u5834\u304c\u3042\u308b\u30de\u30b0\u30cd\u30bf\u30fc\u306e\u8ef8\u6027\u65b9\u5411\u632f\u52d5\u300d, \u65e5\u672c\u5929\u6587\u5b66\u4f1a\u79cb\u5b63\u5e74\u4f1a\uff08\uff19\u670810-12\u65e5\uff0c\u6771\u5317\u5927\u5b66\uff09<\/li>\n<li>\u7167\u559c\u540d\u6b69\uff0c<span style=\"text-decoration: underline;\">\u5c71\u672c\u4e00\u535a<\/span>\uff0c\u5c0f\u5c71\u548c\u54c9, D. Bacon, R.C.Nichol, L. Lombriser\uff1a \u300c\u9280\u6cb3\u56e3\u306e\u30ac\u30b9\u5206\u5e03\u89b3\u6e2c\u3092\u7528\u3044\u305f\u4fee\u6b63\u91cd\u529b\u6a21\u578b\u306e\u691c\u8a3c\u300d, \u65e5\u672c\u5929\u6587\u5b66\u4f1a\u79cb\u5b63\u5e74\u4f1a\uff08\uff19\u670810\u65e5\uff0c\u6771\u5317\u5927\u5b66\uff09<\/li>\n<li>\u5ca1\u30a2\u30ad\u30e9\uff0c\u6a3d\u5bb6\u7be4\u53f2\uff0c\u5c0f\u5c71\u548c\u54c9\uff0c\u5e73\u677e\u5c1a\u5fd7\uff0c\u897f\u9053\u5553\u535a\uff0c<span style=\"text-decoration: underline;\">\u5c71\u672c\u4e00\u535a<\/span>\uff1a \u300cSDSS LRG\u975e\u7b49\u65b9\u30af\u30e9\u30b9\u30bf\u30ea\u30f3\u30b0\u3092\u7528\u3044\u305ff(R)\u91cd\u529b\u7406\u8ad6\u306b\u5bfe\u3059\u308b\u5236\u9650\u300d, \u65e5\u672c\u5929\u6587\u5b66\u4f1a\u79cb\u5b63\u5e74\u4f1a\uff08\uff19\u670810\u65e5\uff0c\u6771\u5317\u5927\u5b66\uff09<\/li>\n<li>\u65e5\u5f71\u5343\u79cb\uff0c<span style=\"text-decoration: underline;\">\u5c71\u672c\u4e00\u535a<\/span>\uff1a\u300cImpacts of satellite galaxies in measuring the cosmic growth rate\u300d, \u65e5\u672c\u5929\u6587\u5b66\u4f1a\u79cb\u5b63\u5e74\u4f1a\uff08\uff19\u670810\u65e5\uff0c\u6771\u5317\u5927\u5b66\uff09<\/li>\n<li><span style=\"text-decoration: underline;\">\u52a0\u85e4\u6052\u5f66<\/span>\uff1a\u300cPIC\u30b7\u30df\u30e5\u30ec\u30fc\u30b7\u30e7\u30f3\u306b\u304a\u3051\u308b\u9ad8\u30a8\u30cd\u30eb\u30ae\u30fc\u7c92\u5b50\u306e\u30a8\u30cd\u30eb\u30ae\u30fc\u30ed\u30b9\u300d, \u65e5\u672c\u5929\u6587\u5b66\u4f1a 2013\u5e74\u79cb\u5b63\u5e74\u4f1a\uff08\uff19\u670812\u65e5\uff0c\u6771\u5317\u5927\u5b66\uff09<\/li>\n<li>\u5b85\u5d8c\u7950\u4e00\u90ce\uff0c\u7167\u559c\u540d\u6b69\uff0c<span style=\"text-decoration: underline;\">\u5c71\u672c\u4e00\u535a<\/span>\uff1a \u300c\u6700\u3082\u4e00\u822c\u7684\u306a\u30b9\u30ab\u30e9\u30fc\u30c6\u30f3\u30bd\u30eb\u7406\u8ad6\u306b\u304a\u3051\u308b\u5b87\u5b99\u8ad6\u7684\u5bc6\u5ea6\u63fa\u3089\u304e\u306e\u30d0\u30a4\u30b9\u30da\u30af\u30c8\u30eb\u300d,\u65e5\u672c\u7269\u7406\u5b66\u4f1a\u79cb\u5b63\u5e74\u4f1a\uff08\uff19\u670821\u65e5\uff0c\u9ad8\u77e5\u5927\u5b66\uff09<\/li>\n<li>\u65e5\u5f71\u5343\u79cb\uff0c<span style=\"text-decoration: underline;\">\u5c71\u672c\u4e00\u535a<\/span>\uff1a\u300cImpacts of satellite galaxies on the redshift-space distortions\u300d, \u65e5\u672c\u7269\u7406\u5b66\u4f1a\u79cb\u5b63\u5e74\u4f1a\uff08\uff19\u670821\u65e5\uff0c\u9ad8\u77e5\u5927\u5b66\uff09<\/li>\n<li>\u7167\u559c\u540d\u6b69\uff0c<span style=\"text-decoration: underline;\">\u5c71\u672c\u4e00\u535a<\/span>\uff0c\u5c0f\u5c71\u548c\u54c9, D. Bacon, R.C.Nichol, L Lombriser\uff1a \u300c\u9aea\u306e\u6bdb\u5ea7\u9280\u6cb3\u56e3\u306e\u591a\u6ce2\u9577\u89b3\u6e2c\u3092\u7528\u3044\u305f\u30ab\u30e1\u30ec\u30aa\u30f3\u91cd\u529b\u6a21\u578b\u306e\u691c\u8a3c\u300d, \u7b2c\uff12\u56de\u89b3\u6e2c\u7684\u5b87\u5b99\u8ad6\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d7\uff0812\u6708\uff15\u65e5\uff0c\u56fd\u7acb\u5929\u6587\u53f0\uff09<\/li>\n<li>\u5b85\u5d8c\u7950\u4e00\u90ce\uff0c\u7167\u559c\u540d\u6b69\uff0c<span style=\"text-decoration: underline;\">\u5c71\u672c\u4e00\u535a<\/span>\uff1a\u300c\u6700\u3082\u4e00\u822c\u7684\u306a\u30b9\u30ab\u30e9\u30fc\u30c6\u30f3\u30bd\u30eb\u7406\u8ad6\u306b\u304a\u3051\u308b\u5b87\u5b99\u8ad6\u7684\u5bc6\u5ea6\u63fa\u3089\u304e\u306e\u30d0\u30a4\u30b9\u30da\u30af\u30c8\u30eb\u300d, \u7b2c\uff12\u56de\u89b3\u6e2c\u7684\u5b87\u5b99\u8ad6\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d7\uff0812\u6708\uff15\u65e5\uff0c\u56fd\u7acb\u5929\u6587\u53f0\uff09<\/li>\n<li>\u65e5\u5f71\u5343\u79cb\uff0c<span style=\"text-decoration: underline;\">\u5c71\u672c\u4e00\u535a<\/span>\uff1a\u300cImpacts of satellite galaxies in measureing the comsmic growt rate\u300d, \u7b2c\uff12\u56de\u89b3\u6e2c\u7684\u5b87\u5b99\u8ad6\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d7\uff0812\u6708\uff15\u65e5\uff0c\u56fd\u7acb\u5929\u6587\u53f0\uff09<\/li>\n<li>\u5ca1\u30a2\u30ad\u30e9\uff0c\u6a3d\u5bb6\u7be4\u53f2\uff0c\u5c0f\u5c71\u548c\u54c9\uff0c\u5e73\u677e\u5c1a\u5fd7\uff0c\u897f\u9053\u5553\u535a\uff0c<span style=\"text-decoration: underline;\">\u5c71\u672c\u4e00\u535a<\/span>\uff1a\u300cCosmological Test of f(R) Gravity with Anisotropic Galaxy Cllustering\u300d, \u7b2c\uff12\u56de\u89b3\u6e2c\u7684\u5b87\u5b99\u8ad6\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d7\uff0812\u6708\uff15\u65e5\uff0c\u56fd\u7acb\u5929\u6587\u53f0\uff09<\/li>\n<li><span style=\"text-decoration: underline;\">\u5c0f\u5d8c\u5eb7\u53f2<\/span>\uff1a\u300c\u30de\u30b0\u30cd\u30bf\u30fc\u306e\u8ef8\u6027\u65b9\u5411\u632f\u52d5\u3068\u78c1\u6c17\u570f\u3068\u306e\u7d50\u5408\u300d, \u65e5\u672c\u5929\u6587\u5b66\u4f1a\u6625\u5b63\u5e74\u4f1a\uff082014\u5e74\uff13\u670819-22\u65e5\uff0c\u56fd\u969b\u57fa\u7763\u6559\u5927\u5b66\uff09<\/li>\n<li><span style=\"text-decoration: underline;\">\u52a0\u85e4\u6052\u5f66<\/span>\uff1a\u300c\u9ad8\u30de\u30c3\u30cf\u6570\u306e\u6e96\u5e73\u884c\u885d\u6483\u6ce2\u306b\u304a\u3051\u308b\u967d\u5b50\u3068\u96fb\u5b50\u306e\u52a0\u901f\u300d, \u65e5\u672c\u5929\u6587\u5b66\u4f1a 2014\u5e74\u6625\u5b63\u5e74\u4f1a\uff082014\u5e74\uff13\u670822\u65e5\uff0c\u56fd\u969b\u57fa\u7763\u6559\u5927\u5b66\uff09<\/li>\n<li>\u5b85\u5d8c\u7950\u4e00\u90ce\uff0c\u7167\u559c\u540d\u6b69\uff0c<span style=\"text-decoration: underline;\">\u5c71\u672c\u4e00\u535a<\/span>\uff1a \u300c\u6700\u3082\u4e00\u822c\u7684\u306a\u30b9\u30ab\u30e9\u30fc\u30c6\u30f3\u30bd\u30eb\u7406\u8ad6\u306b\u304a\u3051\u308b\u5b87\u5b99\u8ad6\u7684\u5bc6\u5ea6\u63fa\u3089\u304e\u306e\u6a19\u6e96\u6442\u52d5\u7406\u8ad6\u300d, \u65e5\u672c\u7269\u7406\u5b66\u4f1a\u6625\u5b63\u5e74\u4f1a\uff082014\u5e74\uff13\u670827\u65e5\uff0c\u6771\u6d77\u5927\u5b66\uff09<\/li>\n<li><span style=\"text-decoration: underline;\">\u5c71\u672c\u4e00\u535a<\/span>, G. Huetsi, \u91d1\u4e38\u9054\u90ce\uff0c\u7167\u559c\u540d\u6b69\uff0c\u65e5\u5f71\u5343\u79cb\uff1a \u300cSDSS III DR9 CMASS\u9280\u6cb3\u30b5\u30f3\u30d7\u30eb\u306e\u591a\u91cd\u6975\u30d1\u30ef\u30fc\u30b9\u30da\u30af\u30c8\u30eb\u3068\u30cf\u30ed\u30fc\u30a2\u30d7\u30ed\u30fc\u30c1\u300d, \u65e5\u672c\u7269\u7406\u5b66\u4f1a\u6625\u5b63\u5e74\u4f1a\uff082014\u5e74\uff13\u670828\u65e5\uff0c\u6771\u6d77\u5927\u5b66\uff09<\/li>\n<li><span style=\"text-decoration: underline;\">\u5fd7\u57a3\u8ce2\u592a<\/span>\uff1a\u300cPast\/Present\/Future of ALICE and (s)PHENIX and More for Heavy Ion Program \u3000\u3000at J-PARC\u300dJ-PARC \u91cd\u30a4\u30aa\u30f3\u52a0\u901f\u56fd\u969b\u7814\u7a76\u4f1a, \uff082014\u5e74\uff13\u670817-18\u65e5\uff0c\u65e5\u672c\u539f\u5b50\u529b\u7814\u7a76\u958b\u767a\u6a5f\u69cb\uff09<\/li>\n<li><span style=\"text-decoration: underline;\">\u5fd7\u57a3\u8ce2\u592a<\/span>\uff1a\u300cPhysics with Hard\/Heavy Probes at sPHENIX\/RHIC and Non-MIE Pre-Shower \u3000\u3000\u3000Detector\u300dPHENIX Workshop on Physics Prospects with Detector and Accelerator Upgrades, \uff082013\u5e74\uff17\u670829\u65e5-\uff18\u6708\uff12\u65e5\uff0c\u7406\u5316\u5b66\u7814\u7a76\u6240\uff09<\/li>\n<li><span style=\"text-decoration: underline;\">\u5fd7\u57a3\u8ce2\u592a<\/span>\uff1a\u300cSearch for Ultra-Intense U(1) Magnetic Field\u300dALICE \u5b9f\u9a13\u65e5\u4ecf\u7814\u7a76\u4f1a, \uff082014\u5e74\uff13\u6708\uff13-\uff17\u65e5\uff0c\u7b51\u6ce2\u5927\u5b66\uff09<\/li>\n<li><span style=\"text-decoration: underline;\">\u672c\u9593\u8b19\u8f14<\/span>\uff1a\u300c\u771f\u7a7a\u91cf\u5b50\u5149\u5b66\u3000-\u6697\u9ed2\u30a8\u30cd\u30eb\u30ae\u30fc\u6e90\u5019\u88dc\u306e\u5730\u4e0a\u63a2\u7d22\u3078\u5411\u3051\u3066-\u300d, \u30ec\u30fc\u30b6\u30fc\u5b66\u4f1a\u5b66\u8853\u8b1b\u6f14\u4f1a\u7b2c33\u56de\u5e74\u6b21\u5927\u4f1a\uff08\u59eb\u8def\u5546\u5de5\u4f1a\u8b70\u6240\uff0c2013\u5e74\uff11\u670828-30\u65e5\uff09<\/li>\n<li><span style=\"text-decoration: underline;\">\u4e09\u597d\u9686\u535a<\/span>\uff1a\u300c\u78c1\u6c17\u6d41\u4f53\u529b\u5b66\u65b9\u7a0b\u5f0f\u306b\u5bfe\u3059\u308b\u885d\u6483\u6ce2\u6355\u7372\u6cd5\u306e\u7814\u7a76\u300d, \u65e5\u672c\u7269\u7406\u5b66\u4f1a2013\u5e74\u79cb\u5b63\u5927\u4f1a\uff082013\u5e74\uff19\u670825-28\u65e5\uff0c\u5fb3\u5cf6\u5927\u5b66\uff09<\/li>\n<li><span style=\"text-decoration: underline;\">\u672c\u9593\u8b19\u8f14<\/span>\uff0c\u9577\u8c37\u90e8\u5b5d\uff0c\u4e45\u7c73\u4e00\u8f1d\uff0c\u5927\u8c37\u4e00\u4eba\uff0c\u6642\u7530\u8302\u6a39\uff0c\u6a4b\u7530\u660c\u6a39\uff0c\u962a\u90e8\u5468\u4e8c\uff1a\u300c\u771f\u7a7a\u91cf\u5b50\u5149\u5b66\u3000-\u6697\u9ed2\u30a8\u30cd\u30eb\u30ae\u30fc\u6e90\u5019\u88dc\u306e\u5730\u4e0a\u63a2\u7d22\u3078\u5411\u3051\u3066-\u300d\u65e5\u672c\u7269\u7406\u5b66\u4f1a\u7b2c68\u56de\u5e74\u6b21\u5927\u4f1a\uff08\u5e83\u5cf6\u5927\u5b66\uff0c2013\u5e74\uff13\u670828\u65e5\uff09<\/li>\n<\/ul>\n\n<p><a id=\"events_H25\"><\/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<ul>\n<li style=\"text-align: justify;\">1st CORE-U International Conference: Intense Fields and Extreme Universe [CORE-U \u4e3b\u50ac]<br \/>\u65e5\u6642(Date\/Time): 2016\u5e743\u67087-8\u65e5 (Mar. 7th-8th 2016)<br \/>\u5834\u6240(Venue): \u7406\u5b66\u90e8E203, \u5e83\u5cf6\u5927\u5b66 (E203, Faculty of Science, Hiroshima Univ.)<br \/>HP: <a href=\"http:\/\/conf1st.core-u.hiroshima-u.ac.jp\/\">http:\/\/conf1st.core-u.hiroshima-u.ac.jp\/<\/a><\/li>\n<li style=\"text-align: justify;\">Astroparticle View of Galaxy Clusters [CORE-U \u5171\u50ac]<br \/>\u65e5\u6642(Date\/Time): 2015\u5e743\u670824\u65e5-3\u670826\u65e5 (Mar. 24th-26th 2015)<br \/>\u5834\u6240(Venue): \u5e83\u5cf6\u5927\u5b66 \u7406\u5b66\u90e8 (Faculty of Science, Hiroshima Univ.)<br \/>HP: <a href=\"http:\/\/www-heaf.hepl.hiroshima-u.ac.jp\/cluster1503\/index.html\">http:\/\/www-heaf.hepl.hiroshima-u.ac.jp\/cluster1503\/index.html<\/a><\/li>\n<li style=\"text-align: justify;\">\u9ad8\u5b87\u9023\u3000\u7b2c14\u56de\u7814\u7a76\u4f1a\u300c\u4eca\u5f8c10\u5e74\u306e\u5b87\u5b99\u89b3\u6e2c\u300d[CORE-U \u5354\u8cdb]<br \/>\u65e5\u6642(Date\/Time): 2015\u5e743\u67089\u65e5-3\u670811\u65e5 (Mar. 9th-11th 2015)<br \/>\u5834\u6240(Venue): \u5e83\u5cf6\u5927\u5b66\u5b66\u58eb\u4f1a\u9928\u30ec\u30bb\u30d7\u30b7\u30e7\u30f3\u30db\u30fc\u30eb (Faculty Club, Hiroshima Univ.)<br \/>HP: <a href=\"http:\/\/www-heaf.hepl.hiroshima-u.ac.jp\/heapa-ws2014\/index.html\">http:\/\/www-heaf.hepl.hiroshima-u.ac.jp\/heapa-ws2014\/index.html<\/a><\/li>\n<li style=\"text-align: justify;\">\u7b2c\uff18\u56de \u30d6\u30e9\u30c3\u30af\u30db\u30fc\u30eb\u78c1\u6c17\u570f\u7814\u7a76\u4f1a [CORE-U \u5f8c\u63f4]<br \/>\u65e5\u6642(Date\/Time): 2015\u5e743\u67082\u65e5-3\u67085\u65e5 (Mar. 2nd-5th 2015)<br \/>\u5834\u6240(Venue): \u5e83\u5cf6\u5927\u5b66 (Hiroshima Univ.)<br \/>HP: <a title=\"http:\/\/www.phyas.aichi-edu.ac.jp\/~takahasi\/BHmag2015\/\" href=\"http:\/\/www.phyas.aichi-edu.ac.jp\/~takahasi\/BHmag2015\/\">http:\/\/www.phyas.aichi-edu.ac.jp\/~takahasi\/BHmag2015\/<\/a><\/li>\n<li style=\"text-align: justify;\">CORE-U Kickoff Symposium [CORE-U \u4e3b\u50ac]<br \/>\u65e5\u6642(Date\/Time): 2015\u5e741\u670821\u65e5 (Jan. 21st 2015)<br \/>\u5834\u6240(Venue): \u5e83\u5cf6\u5927\u5b66\u4e2d\u592e\u56f3\u66f8\u9928\u30e9\u30a4\u30d6\u30e9\u30ea\u30db\u30fc\u30eb (Library Hall,  Central Library, Hiroshima Univ.)<br \/>HP: <a title=\"http:\/\/core-u.hiroshima-u.ac.jp\/~events\/COREUKOS.html\" href=\"http:\/\/core-u.hiroshima-u.ac.jp\/~events\/COREUKOS.html\">http:\/\/core-u.hiroshima-u.ac.jp\/~events\/COREUKOS.html<\/a><\/li>\n<li style=\"text-align: justify;\">\u7b2c2\u56de\u6975\u9650\u5b87\u5b99\u7814\u7a76\u62e0\u70b9\u30bb\u30df\u30ca\u30fc\uff08The 2nd Core-U seminar\uff09<br \/>\u65e5\u6642(Date\/TIME) : 2014\u5e7410\u670830\u65e5 (Oct. 30th 2014)<br \/> \u5834\u6240(Venue): \u7406\u5b66\u90e8E203, \u5e83\u5cf6\u5927\u5b66 (E203, Faculty of Science, Hiroshima Univ.)<br \/> Poster: pdf<\/li>\n<li style=\"text-align: justify;\">Workshop on Synergy of HSC and Hiroshima CORE-U projects for Galaxy Clusters and Astronomical Transients<br \/> \u5171\u50ac(Cosponsor) :  Hyper Suprime-Cam (HSC) project of Subaru Telescope<br \/>\u65e5\u6642(Date\/TIME) :  2014\u5e748\u670816\u65e5 (Jul. 16th 2014)<br \/> \u5834\u6240(Venue): \u6587\u5b66\u90e8B204, \u5e83\u5cf6\u5927\u5b66 (B204, Faculty of Letters, Hiroshima Univ.)<br \/> HP:<a href=\"http:\/\/home.hiroshima-u.ac.jp\/hasc\/hsc-coreu2014\/\">http:\/\/home.hiroshima-u.ac.jp\/hasc\/hsc-coreu2014\/<\/a><\/li>\n<li style=\"text-align: justify;\">\u7b2c1\u56de\u5e83\u5cf6\u5927\u5b66\u6975\u9650\u5b87\u5b99\u7814\u7a76\u62e0\u70b9\u5171\u50ac\u30bb\u30df\u30ca\u30fc\uff08The 1st Core-U seminar (joint)\uff09<br \/> \u5171\u50ac(Cosponsor) : B\u30d5\u30a1\u30af\u30c8\u30ea\u30fc\u7269\u7406\u52c9\u5f37\u4f1a\u3000\u7b2c14\u56de\u30df\u30fc\u30c6\u30a3\u30f3\u30b0 (the 14th B factory physics study meeting<br \/>\u65e5\u6642(Date\/TIME) : 2014\u5e748\u670827\u65e5 (Aug. 27th 2014)<br \/> \u5834\u6240(Venue): \u7406\u5b66\u90e8E203, \u5e83\u5cf6\u5927\u5b66 (E203, Faculty of Science, Hiroshima Univ.)<\/li>\n<\/ul>\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-1073","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/core-u.hiroshima-u.ac.jp\/en\/wp-json\/wp\/v2\/pages\/1073","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=1073"}],"version-history":[{"count":1,"href":"https:\/\/core-u.hiroshima-u.ac.jp\/en\/wp-json\/wp\/v2\/pages\/1073\/revisions"}],"predecessor-version":[{"id":1074,"href":"https:\/\/core-u.hiroshima-u.ac.jp\/en\/wp-json\/wp\/v2\/pages\/1073\/revisions\/1074"}],"wp:attachment":[{"href":"https:\/\/core-u.hiroshima-u.ac.jp\/en\/wp-json\/wp\/v2\/media?parent=1073"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}