{"id":1079,"date":"2018-02-02T15:55:08","date_gmt":"2018-02-02T06:55:08","guid":{"rendered":"http:\/\/core-u.hiroshima-u.ac.jp\/?page_id=1079"},"modified":"2018-02-02T15:55:08","modified_gmt":"2018-02-02T06:55:08","slug":"1079-2","status":"publish","type":"page","link":"https:\/\/core-u.hiroshima-u.ac.jp\/en\/1079-2.html","title":{"rendered":""},"content":{"rendered":"<p style=\"text-align: center;\">[<a href=\"#publications_H28\">\u8ad6\u6587 Publications<\/a>] [<a href=\"#presentations_H28\">\u5b66\u4f1a\u30fb\u7814\u7a76\u4f1a\u767a\u8868 Presentations<\/a>] [<a href=\"#events_H28\">Core-U\u30a4\u30d9\u30f3\u30c8 Core-U Events<\/a>]<\/p>\n<p><a id=\"publications_H28\"><\/a><\/p>\n<h2>\u8ad6\u6587 Publications<\/h2>\n<ul style=\"list-style-type: disc;\">\n<li>Abdollahi, S., <span class=\"underline\">Fukazawa, Y.<\/span>(34\u756a\u76ee), <span class=\"underline\">Mizuno,T.<\/span>(62\u756a\u76ee), et al. \u8a0894\u540d, &ldquo;Search for Cosmic-Ray Electron and Positron Anisotropies with SevenYears of Fermi Large Area Telescope Data,&rdquo; 2017, PRL 118, 091103.<\/li>\n<li>Aharonian, F. A., <span class=\"underline\">Fukazawa, Y.<\/span>(33\u756a\u76ee), <span class=\"underline\">Kitaguchi, T.<\/span> (78\u756a\u76ee), <span class=\"underline\">Mizuno, T.<\/span> (113\u756a\u76ee), <span class=\"underline\">Ohno,M.<\/span> (134\u756a\u76ee), <span class=\"underline\">Takahashi, H.<\/span> (170\u756a\u76ee),<span class=\"underline\">Tanaka, Y.<\/span> (179\u756a\u76ee) et al. \u8a08216\u540d, &ldquo;Hitomi Constraints on the 3.5 keV Line in the Perseus GalaxyCluster,&rdquo; 2017,ApJL 837, 15.<\/li>\n<li>Ackermann,M., <span class=\"underline\">Fukazawa, Y.<\/span>(45\u756a\u76ee), <span class=\"underline\">Mizuno, T.<\/span>(80\u756a\u76ee), et al. (\u8a08126\u540d), &ldquo;Gamma-Ray Blazars within the First 2 Billion Years,&rdquo; ApJL 837, 5 (2017).<\/li>\n<li><span class=\"underline\">Ohno, M.<\/span>, <span class=\"underline\">Tanaka,Y.<\/span>(9\u756a\u76ee), <span class=\"underline\">Takahashi, H.<\/span>(10\u756a\u76ee),<span class=\"underline\">Mizuno, T.<\/span>(11\u756a\u76ee), <span class=\"underline\">Fukazawa, Y.<\/span>(12\u756a\u76ee), et al. \u8a0847\u540d, &ldquo;Development and verification of signal processing system ofavalanche photo diode for the active shield onboard ASTRO-H,&rdquo; 2016, NIMA 831, 410.<\/li>\n<li>Nakaoka, T.,<span class=\"underline\">Mizuno, T.<\/span>, <span class=\"underline\">Takahashi, H.<\/span>, <span class=\"underline\">Fukazawa,Y.<\/span>,, &ldquo;Study of a detector system for high-energy astrophysical objectsusing a combination of plastic scintillator and MPPC,&rdquo; 2016, NIM-A 831, 400.<\/li>\n<li>Ackermann, M., <span class=\"underline\">Fukazawa, Y.<\/span>(31\u756a\u76ee), <span class=\"underline\">Mizuno, T.<\/span> (58\u756a\u76ee), \u4ed686\u540d, &ldquo;Fermi-LAT Observations of High-energy Behind-the-limb SolarFlares,&rdquo; 2017, ApJ835, 219, 13pp.<\/li>\n<li>Racusin, J. L., <span class=\"underline\">Fukazawa, Y.<\/span> (71\u756a\u76ee),<span class=\"underline\">Mizuno, T.<\/span> (104\u756a\u76ee), \u4ed6140\u540d, &ldquo;Searching the Gamma-Ray Sky for Counterparts to Gravitational WaveSources: \/Fermi GBM and LAT Observations of LVT151012 and GW151226,&rdquo; 2017, ApJ 835,82, 13pp.<\/li>\n<li>Itoh, R., <span class=\"underline\">Fukazawa, Y.<\/span> (3\u756a\u76ee), <span class=\"underline\">Uemura,M.<\/span> (4\u756a\u76ee), <span class=\"underline\">Tanaka, Y. T.<\/span> (5\u756a\u76ee),<span class=\"underline\">Kawabata, K. S.<\/span> (6\u756a\u76ee), <span class=\"underline\">Akitaya, H.<\/span> (11\u756a\u76ee), <span class=\"underline\">Ohsugi,T.<\/span> (14\u756a\u76ee), <span class=\"underline\">Yoshida, M.<\/span> (21\u756a\u76ee),\u4ed613\u540d, &ldquo;Systematic Study of Gamma-ray-bright Blazars with OpticalPolarization and Gamma-Ray Variability,&rdquo; 2016, ApJ 833, 77, 17pp.<\/li>\n<li>Hitomi collaboration, <span class=\"underline\">Fukazawa,Y.<\/span> (33\u756a\u76ee), <span class=\"underline\">Kitaguchi, T.<\/span> (79\u756a\u76ee),<span class=\"underline\">Mizuno, T.<\/span> (114\u756a\u76ee), <span class=\"underline\">Ohno, M.<\/span> (135\u756a\u76ee), <span class=\"underline\">Takahashi,H.<\/span> (171\u756a\u76ee), <span class=\"underline\">Tanaka, Y.<\/span> (180\u756a\u76ee)\u4ed6212\u540d, &ldquo;Hitomi Constraints on the 3.5 keV Line in the Perseus GalaxyCluster,&rdquo; 2017, ApJ 837, L15, 9pp.<\/li>\n<li>Katsuta, J., <span class=\"underline\">Mizuno, T.<\/span> (7\u756a\u76ee), <span class=\"underline\">Fukazawa,Y.<\/span> (8\u756a\u76ee), <span class=\"underline\">Kitaguchi, T.<\/span> (12\u756a\u76ee),<span class=\"underline\">Ohno, M.<\/span> (13\u756a\u76ee), <span class=\"underline\">Takahashi, H.<\/span> (15\u756a\u76ee), \u4ed614\u540d, &ldquo;Study of the polarimetric performance of a Si\/CdTe semiconductorCompton camera for the Hitomi satellite,&rdquo; 2016, NIM-A, 840, 51-58.<\/li>\n<li>Katsuda, S.,<span class=\"underline\">Fukazawa, Y.<\/span> (5\u756a\u76ee), <span class=\"underline\">Kawabata, K. S.<\/span> (6\u756a\u76ee), <span class=\"underline\">Ohno,M.<\/span> (7\u756a\u76ee), \u4ed66\u540d, &ldquo;Two Distinct-absorption X-Ray Components from Type IIn Supernovae:Evidence for Asphericity in the Circumstellar Medium,&rdquo; 2016. ApJ 832, 194, 12pp.<\/li>\n<li>Noda, H., <span class=\"underline\">Uemura, M.<\/span> (15\u756a\u76ee), <span class=\"underline\">Kawabata,K. S.<\/span> (16\u756a\u76ee), <span class=\"underline\">Yoshida, M.<\/span> (17\u756a\u76ee),<span class=\"underline\">Fukazawa, Y.<\/span> (25\u756a\u76ee), \u4ed621\u540d, &ldquo;X-Ray and Optical Correlation of Type I Seyfert NGC 3516 Studiedwith Suzaku and Japanese Ground-based Telescopes,&rdquo; 2016, ApJ 828,78, 15pp.<\/li>\n<li><span class=\"underline\">Tanaka, Y. T.<\/span>, <span class=\"underline\">Fukazawa,Y.<\/span> (12\u756a\u76ee), \u4ed619\u540d, &ldquo;A significant hardening and rising shape detected in the MeV\/GeV\u03bdF\u03bd spectrum from the recently discovered very-high-energy blazar S40954+65 during the bright optical flare in 2015 February,&rdquo; 2016. PASJ 68, 51, 10pp.<\/li>\n<li>Mori, K., <span class=\"underline\">Fukazawa, Y.<\/span> (9\u756a\u76ee), \u4ed610\u540d, &ldquo;A broadband x-ray imaging spectroscopy with high-angularresolution: the FORCE mission,&rdquo; 2016, Proc. SPIE 9905,990510, 10pp.<\/li>\n<li>Didler, B.,<span class=\"underline\">Fukazawa, Y.<\/span> (51\u756a\u76ee), \u4ed689\u540d, &ldquo;The Athena X-ray Integral Field Unit (X-IFU),&rdquo; 2016, Proc.SPIE 9905, 99052F, 41pp.<\/li>\n<li>Watanabe, S.<span class=\"underline\">Fukazawa, Y.<\/span> (3\u756a\u76ee), <span class=\"underline\">Kitaguchi, T.<\/span> (12\u756a\u76ee), <span class=\"underline\">Mizuno,T.<\/span> (19\u756a\u76ee), <span class=\"underline\">Ohno, M.<\/span> (26\u756a\u76ee),<span class=\"underline\">Takahashi, H.<\/span> (32\u756a\u76ee), <span class=\"underline\">Tanaka, Y.<\/span> (35\u756a\u76ee), \u4ed628\u540d, &ldquo;The soft gamma-ray detector (SGD) onboard ASTRO-H,&rdquo; 2016, Proc. SPIE 9905,990513, 16pp.<\/li>\n<li>Nakazawa, K.,<span class=\"underline\">Fukazawa, Y.<\/span> (5\u756a\u76ee), <span class=\"underline\">Mizuno, T.<\/span> (15\u756a\u76ee), <span class=\"underline\">Ohno,M.<\/span> (21\u756a\u76ee), <span class=\"underline\">Takahashi, H.<\/span> (26\u756a\u76ee),\u4ed630\u540d, &ldquo;The hard x-ray imager (HXI) onboard ASTRO-H,&rdquo; 2016, Proc, SPIE 5509, 550911, 13pp.<\/li>\n<li>Takahashi, T.,<span class=\"underline\">Fukazawa, Y.<\/span> (48\u756a\u76ee), <span class=\"underline\">Kitaguchi, T.<\/span> (101\u756a\u76ee), <span class=\"underline\">Mizuno,T.<\/span> (140\u756a\u76ee), <span class=\"underline\">Ohno, M.<\/span> (170\u756a\u76ee),<span class=\"underline\">Takahashi, H.<\/span> (220\u756a\u76ee), <span class=\"underline\">Tanaka, Y. T.<\/span> (228\u756a\u76ee), \u4ed6262\u540d, &ldquo;The ASTRO-H (Hitomi) x-ray astronomy satellite,&rdquo; 2016, Proc. SPIE 5509,55090U, 17pp.<\/li>\n<li>Hitomi collaboration, <span class=\"underline\">Fukazawa,Y.<\/span> (34\u756a\u76ee), <span class=\"underline\">Kitaguchi, T.<\/span> (77\u756a\u76ee),<span class=\"underline\">Mizuno, T.<\/span> (112\u756a\u76ee), <span class=\"underline\">Ohno, M.<\/span> (133\u756a\u76ee), <span class=\"underline\">Takahashi,H.<\/span> (168\u756a\u76ee), <span class=\"underline\">Tanaka, Y. T.<\/span> (177\u756a\u76ee),\u4ed6210\u540d, &ldquo;The quiescent intracluster medium in the core of the Perseuscluster,&rdquo; 2016, Nature 535, 117-121.<\/li>\n<li>Ohmori, N., <span class=\"underline\">Ohno, M.<\/span> (3\u756a\u76ee), <span class=\"underline\">Fukazawa,Y.<\/span> (12\u756a\u76ee), \u4ed625\u540d, &ldquo;Suzaku Wide-band All-sky Monitor measurements of durationdistributions of gamma-ray bursts,&rdquo; 2016, PASJ 68, S30, 11pp.<\/li>\n<li>Terada, Y., <span class=\"underline\">Fukazawa, Y.<\/span> (3\u756a\u76ee),\u4ed610\u540d, &ldquo;Measurements of the Soft Gamma-Ray Emission from SN2014J withSuzaku,&rdquo; 2016, ApJ 823, 32, 10pp.<\/li>\n<li><span class=\"underline\">Tanaka, Y.T.<\/span>, <span class=\"underline\">Uemura, M.<\/span> (3\u756a\u76ee), <span class=\"underline\">Kawabata, K. S.<\/span> (7\u756a\u76ee), <span class=\"underline\">Fukazawa, Y.<\/span> (8\u756a\u76ee), <span class=\"underline\">Akitaya,H.<\/span> (18\u756a\u76ee), <span class=\"underline\">Yoshida, M.<\/span> (23\u756a\u76ee),\u4ed636\u540d, &ldquo;No Evidence of Intrinsic Optical\/Near-infrared Linear Polarizationfor V404 Cygni during Its Bright Outburst in 2015: Broadband Modeling andConstraint on Jet Parameters,&rdquo; 2016, ApJ 823, 35, 8pp.<\/li>\n<li>Chidiac, C., <span class=\"underline\">Fukazawa, Y.<\/span> (11\u756a\u76ee), <span class=\"underline\">Uemura,M.<\/span> (12\u756a\u76ee), \u4ed613\u540d, &ldquo;Exploring the nature of the broadband variability in the flatspectrum radio quasar 3C 273,&rdquo; 2016, A&amp;A 590, A61, 16pp.<\/li>\n<li>Kiehlmann, S., <span class=\"underline\">Akitaya, H.<\/span> (9\u756a\u76ee),<span class=\"underline\">Fukazawa, Y.<\/span> (19\u756a\u76ee), <span class=\"underline\">Kawabata, K. S.<\/span> (27\u756a\u76ee), <span class=\"underline\">Uemura, M.<\/span> (59\u756a\u76ee), <span class=\"underline\">Yoshida,M.<\/span> (62\u756a\u76ee), \u4ed658\u540d, &ldquo;Polarization angle swings in blazars: The case of 3C 279,&rdquo; 2016, A&amp;A 590, A10, 20pp.<\/li>\n<li><span class=\"underline\">Fukazawa, Y.<\/span>,<span class=\"underline\">Ohno, M.<\/span> (4\u756a\u76ee), \u4ed64\u540d, &ldquo;Fe-K Line Time Variability and Ni Abundance of Distant Reflectorsin Seyfert Galaxies,&rdquo; 2016, ApJ 821, 15,8pp.<\/li>\n<li>Abbott, T. D., <span class=\"underline\">Fukazawa, Y.<\/span> (1209\u756a\u76ee), <span class=\"underline\">Mizuno,T.<\/span> (1258\u756a\u76ee), <span class=\"underline\">Ohsugi, T.<\/span> (1264\u756a\u76ee),<span class=\"underline\">Kawabata, K. S.<\/span> (1386\u756a\u76ee), <span class=\"underline\">Yoshida, M.<\/span> (1392\u756a\u76ee), \u4ed61571\u540d, &ldquo;Supplement: Localization and Broadband Follow-up of theGravitational-wave Transient GW150914,&rdquo; 2016, ApJS 225, 8, 15pp.<\/li>\n<li>Abbott, T. D., <span class=\"underline\">Fukazawa,Y.<\/span> (1209\u756a\u76ee), <span class=\"underline\">Mizuno, T.<\/span> (1258\u756a\u76ee),<span class=\"underline\">Ohsugi, T.<\/span> (1264\u756a\u76ee), <span class=\"underline\">Kawabata, K. S.<\/span> (1386\u756a\u76ee), <span class=\"underline\">Yoshida, M.<\/span> (1392\u756a\u76ee), \u4ed61571\u540d, &ldquo;Localization and Broadband Follow-up of the Gravitational-waveTransient GW150914,&rdquo; 2016, ApJ 826, L13, 8pp.<\/li>\n<li>Ackermann, M., <span class=\"underline\">Fukazawa, Y.<\/span> (45\u756a\u76ee), <span class=\"underline\">Mizuno,T.<\/span> (81\u756a\u76ee), <span class=\"underline\">Ohno, M.<\/span> (83\u756a\u76ee),<span class=\"underline\">Ohsugi, T.<\/span> (89\u756a\u76ee), <span class=\"underline\">Takahashi, H.<\/span> (112\u756a\u76ee), \u4ed6116\u540d, &ldquo;Fermi Large Area Telescope Detection of Extended Gamma-RayEmission from the Radio Galaxy Fornax A,&rdquo; 2016, ApJ 826, 1, 9pp.<\/li>\n<li>Ackermann,M., <span class=\"underline\">Fukazawa, Y.<\/span> (40\u756a\u76ee), <span class=\"underline\">Mizuno, T.<\/span> (75\u756a\u76ee), <span class=\"underline\">Ohsugi,T.<\/span> (82\u756a\u76ee), \u4ed6105\u540d, &ldquo;Minute-timescale &gt;100 MeV \u03b3-Ray Variability during the GiantOutburst of Quasar 3C 279 Observed by Fermi-LAT in 2015 June,&rdquo; 2016, ApJ 824, L20, 8pp.<\/li>\n<li>Acero, F.,<span class=\"underline\">Fukazawa, Y.<\/span> (49\u756a\u76ee), <span class=\"underline\">Mizuno, T.<\/span> (104\u756a\u76ee), <span class=\"underline\">Ohsugi,T.<\/span> (113\u756a\u76ee), <span class=\"underline\">Takahashi, H.<\/span> (145\u756a\u76ee),\u4ed6156\u540d, &ldquo;The First Fermi LAT Supernova Remnant Catalog,&rdquo; 2016, ApJS 224, 8, 50pp.<\/li>\n<li>Ackermann, M.,<span class=\"underline\">Fukazawa, Y.<\/span> (60\u756a\u76ee), <span class=\"underline\">Mizuno, T.<\/span> (114\u756a\u76ee), <span class=\"underline\">Ohsugi,T.<\/span> (123\u756a\u76ee), \u4ed6163\u540d, &ldquo;Fermi-LAT Observations of the LIGO Event GW150914,&rdquo; 2016, ApJ 823, L2, 13pp.<\/li>\n<li>Ajello, M., <span class=\"underline\">Fukazawa, Y.<\/span>(37\u756a\u76ee), <span class=\"underline\">Mizuno, T.<\/span> (66\u756a\u76ee), <span class=\"underline\">Takahashi, H.<\/span> (93\u756a\u76ee), \u4ed699\u540d, &ldquo;Search for Spectral Irregularities due toPhoton-Axionlike-Particle Oscillations with the Fermi Large AreaTelescope,&rdquo; 2016, Physical Review Let.116,161101.<\/li>\n<li>Ackermann, M., <span class=\"underline\">Fukazawa, Y.<\/span> (47\u756a\u76ee), <span class=\"underline\">Mizuno,T.<\/span> (84\u756a\u76ee), <span class=\"underline\">Ohsugi, T.<\/span> (92\u756a\u76ee),<span class=\"underline\">Takahashi, H.<\/span> (122\u756a\u76ee), \u4ed6124\u540d, &ldquo;Resolving the Extragalactic \u03b3 -Ray Background above 50 GeV withthe Fermi Large Area Telescope,&rdquo; 2016,Physical Review Let. 116,151105.<\/li>\n<li><span class=\"underline\">Mizuno, T.<\/span>,Abdollahi, S., Fukui, Y., Hayashi, K., Okumura, A., Tajima, H., Yamamoto,H., &ldquo;Quantifying the Interstellar Medium and Cosmic Rays in the MBM 53,54, and 55 Molecular Clouds and the Pegasus Loop Using Fermi-LATGamma-ray Observations,&rdquo; 2016, ApJ 833, 278, 19pp.<\/li>\n<li>Hayashida, K.,<span class=\"underline\">Mizuno, T.<\/span>(9\u756a\u76ee), <span class=\"underline\">Takahashi, H.<\/span>(10\u756a\u76ee), et al. \u8a0816\u540d, &ldquo;Hard x-ray imaging polarimeter for PolariS,&rdquo; 2016, Proc. SPIE9905, 99051A, 10pp.<\/li>\n<li>M. Chauvin, <span class=\"underline\">H. Takahashi<\/span>(8\u756a\u76ee), \u8a089\u540d, &ldquo;Optimizing a balloon-borne polarimeter in the hard X-ray domain:From the PoGOLite Pathfinder to PoGO+,&rdquo; 2016, Astroparticle Physics,Volume 82, p99-107.<\/li>\n<li>Arimoto M., <span class=\"underline\">Ohno M.<\/span> (3\u756a\u76ee), \u8a088\u540d, &ldquo;High-energy Non-thermal and Thermal Emission from GRB 141207A,&rdquo; 2016, TheAstrophysical Journal, 2016, ApJ 833, 139, 13pp.<\/li>\n<li>Ukwatta, T. N., <span class=\"underline\">Ohno,M.<\/span> (17\u756a\u76ee), \u4ed623\u540d, &ldquo;Investigation of Primordial Black Hole Bursts Using InterplanetaryNetwork Gamma-ray Bursts,&rdquo; 2016, ApJ 826, 98, 14pp.<\/li>\n<li>Acero, F., <span class=\"underline\">Mizuno, T.<\/span> (89\u756a\u76ee), <span class=\"underline\">Ohsugi, T.<\/span> (93\u756a\u76ee), <span class=\"underline\">Takahashi,H.<\/span> (121\u756a\u76ee), \u8a08134\u540d, &ldquo;Development of the Model of Galactic Interstellar Emission forStandard Point-source Analysis of Fermi Large Area Telescope Data,&rdquo; 2016, The Astrophysical Journal SupplementSeries, 223, 26.<\/li>\n<li>Goto,T., <span class=\"underline\">Utsumi, Y.<\/span> (3\u756a\u76ee), \u8a0835\u540d, &ldquo;Hyper Suprime-Camera Survey of the Akari NEP Wide Field,&rdquo; 2017,Publication of Korean Astronomical Society, 32, 225.<\/li>\n<li>Oh, Daehyeon, H., <span class=\"underline\">Miyama, S.<\/span>(35\u756a\u76ee), \u8a0851\u540d, &ldquo;Near-infrared imaging polarimetry of LkCa 15: A possible warpedinner disk,&rdquo; 2016, Publications of the Astronomical Society of Japan, 68,L3.<\/li>\n<li>Ackermann, M., <span class=\"underline\">Mizuno, T.<\/span>(77\u756a\u76ee), <span class=\"underline\">Takahashi,H.<\/span> (102\u756a\u76ee), \u8a08116\u540d, &ldquo;Measurement of the high-energy gamma-ray emission from the Moonwith the Fermi Large Area Telescope,&rdquo; 2016, Physical Review D, 93, 082001.<\/li>\n<li>McHardy,I. M., <span class=\"underline\">Uemura, M.<\/span> (15\u756a\u76ee), \u8a0815\u540d, &ldquo;The origin of UV-optical variability in AGN and test of discmodels, XMM-Newton and ground-based observations of NGC 4395,&rdquo; 2016,Astronomische Nachrichten, 337, 500.<\/li>\n<li>Ackermann,M., <span class=\"underline\">Mizuno, T.<\/span>(72\u756a\u76ee), <span class=\"underline\">Ohno, M.<\/span>(78\u756a\u76ee), <span class=\"underline\">Ohsugi,T.<\/span>(79\u756a\u76ee), <span class=\"underline\">Takahashi, H.<\/span>(102\u756a\u76ee),\u8a08112\u540d, &ldquo;Fermi LAT Stacking Analysis of Swift Localized GRBs,&rdquo; 2016, The Astrophysical Journal, 822, 68.<\/li>\n<li>Akiyama, K., <span class=\"underline\">Tanaka, Y.T.<\/span> (3\u756a\u76ee), \u8a086\u540d, &ldquo;EVN Observations of HESS J1943+213: Evidence for an Extreme TeVBL Lac Object,&rdquo; 2016, The Astrophysical Journal, 823, L26.<\/li>\n<li>Ryu, T., <span class=\"underline\">Miyama,S.<\/span> (44\u756a\u76ee), <span class=\"underline\">Yoshida, M.<\/span> (62\u756a\u76ee),\u8a0865\u540d, &ldquo;High-contrast Imaging of Intermediate-mass Giants with Long-termRadial Velocity Trends,&rdquo; 2016, The Astrophysical Journal, 825, 127, 13pp.<\/li>\n<li>Tanaka, M., <span class=\"underline\">Utsumi, Y.<\/span> (14\u756a\u76ee), \u8a0814\u540d, &ldquo;A Spectroscopically Confirmed Double Source Plane Lens System inthe Hyper Suprime-Cam Subaru Strategic Program,&rdquo; 2016, The AstrophysicalJournal, 826, L19, 6pp.<\/li>\n<li>Morokuma, T.,<span class=\"underline\">Utsumi, Y.<\/span>(6\u756a\u76ee), <span class=\"underline\">Kawabata, K. S.<\/span> (11\u756a\u76ee), <span class=\"underline\">Uemura, M.<\/span> (22\u756a\u76ee), <span class=\"underline\">Yoshida,M.<\/span> (25\u756a\u76ee), \u8a0825\u540d, &ldquo;J-GEM follow-up observations to search for an optical counterpartof the first gravitational wave source GW150914,&rdquo; 2016, Publications of the Astronomical Society ofJapan, 68, L9, 6pp.<\/li>\n<li>Asensio-Torres, R., <span class=\"underline\">Miyama, S.<\/span>(33\u756a\u76ee), \u8a0852\u540d, &ldquo;Polarimetry and flux distribution in the debris disk around HD32297,&rdquo; 2016, Astronomy and Astrophysics, 593, A73.<\/li>\n<li>Inoue, Y.i and<span class=\"underline\">Tanaka, Y. T.<\/span>,, &ldquo;Baryon Loading Efficiency and Particle Acceleration Efficiency ofRelativistic Jets: Cases for Low Luminosity BL Lacs,&rdquo; 2016, The AstrophysicalJournal, 828, 13, 10pp.<\/li>\n<li>Matsuoka, Y., <span class=\"underline\">Utsumi, Y.<\/span> (39\u756a\u76ee), \u8a0846\u540d, &ldquo;Subaru High-z Exploration of Low-luminosity Quasars (SHELLQs).Discovery of 15 Quasars and Bright Galaxies at 5.7&lt;z&lt;6.9,&rdquo; 2016, The Astrophysical Journal, 828, 26, 14pp.<\/li>\n<li><span class=\"underline\">Uemura, M.<\/span>, \u8a088\u540d, &ldquo;TimeTubes: Visualization of Polarization Variations in Blazars,&rdquo; 2016, Galaxies, 4, 23.<\/li>\n<li>Inoue, Y., <span class=\"underline\">Tanaka, Y. T.<\/span>, and Isobe, N.,, &ldquo;Binary black hole merger rates inferred from luminosity functionof ultra-luminous X-ray sources,&rdquo; 2016, Monthly Notices ofthe Royal Astronomical Society, 461, 4329.<\/li>\n<li>Yamanaka, M., <span class=\"underline\">Kawabata, K.S.<\/span> (5\u756a\u76ee), <span class=\"underline\">Akitaya, H.<\/span> (10\u756a\u76ee),<span class=\"underline\">Uemura, M.<\/span> (22\u756a\u76ee), <span class=\"underline\">Yoshida, M.<\/span> (23\u756a\u76ee), \u8a0837\u540d, &ldquo;OISTER optical and near-infrared observations of thesuper-Chandrasekhar supernova candidate SN 2012dn: Dust emission from thecircumstellar shell,&rdquo; 2016, Publications of theAstronomical Society of Japan, 68, 68, 24pp.<\/li>\n<li>Mizuki, T., <span class=\"underline\">Miyama, S.<\/span>(32\u756a\u76ee), \u8a0851\u540d, &ldquo;High-contrast imaging of &amp;epsilon; Eridani with ground-basedinstruments,&rdquo; 2016, Astronomy and Astrophysics, 595, A79, 8pp.<\/li>\n<li>Bhatta, G., <span class=\"underline\">Akitaya, H.<\/span>(5\u756a\u76ee),<span class=\"underline\">Kawabata, K. S.<\/span> (22\u756a\u76ee), <span class=\"underline\">Yoshida, M.<\/span> (45\u756a\u76ee), \u8a0846\u540d, &ldquo;Multifrequency Photo-polarimetric WEBT Observation Campaign on theBlazar S5 0716+714: Source Microvariability and Search for CharacteristicTimescales,&rdquo; 2016, The AstrophysicalJournal, 831, 92 , 17pp.<\/li>\n<li>Herczeg, G.J., <span class=\"underline\">Kawabata, K. S.<\/span> (26\u756a\u76ee), \u8a0830\u540d, &ldquo;The Eruption of the Candidate Young Star ASASSN-15QI,&rdquo; 2016,The Astrophysical Journal, 831, 133, 22p.<\/li>\n<li>Oh, Daehyeon, <span class=\"underline\">Miyama,S.<\/span> (33\u756a\u76ee), \u8a0851\u540d, &ldquo;Resolved Near-infrared Image of the Inner Cavity in the GM AurTransitional Disk,&rdquo; 2016, The Astrophysical Journal, 831, L7 , 6pp.<\/li>\n<li>Hefminiak, K. G.,<span class=\"underline\">Miyama, S.<\/span> (32\u756a\u76ee), \u8a0852\u540d, &ldquo;SEEDS Direct Imaging of the RV-detected Companion to V450Andromedae, and Characterization of the System,&rdquo; 2016, TheAstrophysical Journal, 832, 33 , 13pp.<\/li>\n<li>Ishiguro, M.,<span class=\"underline\">Akitaya, H.<\/span>(8\u756a\u76ee), <span class=\"underline\">Kawabata, K. S.<\/span> (9\u756a\u76ee), <span class=\"underline\">Yoshida, M.<\/span> (12\u756a\u76ee), \u8a0824\u540d, &ldquo;2014-2015 Multiple Outbursts of 15P\/Finlay,&rdquo; 2016, The AstronomicalJournal, 152, 169, 14pp.<\/li>\n<li>Akiyama, E., <span class=\"underline\">Miyama,S.<\/span> (43\u756a\u76ee), \u8a0861\u540d, &ldquo;Spiral Structure and Differential Dust Size Distribution in theLKH&amp;alpha; 330 Disk,&rdquo; 2016, The Astronomical Journal, 152, 222, 7pp.<\/li>\n<li>Chan, J. H. H., <span class=\"underline\">Utsumi, Y.<\/span>(15\u756a\u76ee), \u8a0816\u540d, &ldquo;Galaxy-scale Gravitational Lens Candidates from the HyperSuprime-Cam Imaging Survey and the Galaxy And Mass Assembly SpectroscopicSurvey,&rdquo; 2016, The Astrophysical Journal, 832, 135 , 9pp.<\/li>\n<li><span class=\"underline\">Utsumi, Y.<\/span>, \u8a0817\u540d, &ldquo;A Weak Lensing View of the Downsizing of Star-forming Galaxies,&rdquo; 2016, The AstrophysicalJournal, 833, 156 , 14pp.<\/li>\n<li>Kooistra, R., <span class=\"underline\">Miyama, S.<\/span> (33\u756a\u76ee), \u8a0859\u540d, &ldquo;Radial decoupling of small and large dust grains in thetransitional disk RX J1615.3-3255,&rdquo; 2017, Astronomy andAstrophysics, 597, A132 , 8pp.<\/li>\n<li>Yang, Y., <span class=\"underline\">Miyama, S.<\/span> (36\u756a\u76ee), \u8a0854\u540d, &ldquo;Near-infrared Imaging Polarimetry of Inner Region of GG Tau ADisk,&rdquo; 2017, The Astronomical Journal, 153, 7, 9pp.<\/li>\n<li>Garcia, E. V.,<span class=\"underline\">Miyama, S.<\/span> (35\u756a\u76ee), \u8a0855\u540d, &ldquo;SCExAO and GPI Y JHBand Photometry and Integral Field Spectroscopyof the Young Brown Dwarf Companion to HD 1160,&rdquo; 2017, TheAstrophysical Journal, 834, 162 , 14pp.<\/li>\n<li>Gupta, A. C., <span class=\"underline\">Uemura,M.<\/span> (9\u756a\u76ee), \u8a0834\u540d, &ldquo;Multiband optical variability of the blazar OJ 287 during itsoutbursts in 2015-2016,&rdquo; 2017, Monthly Notices of the Royal AstronomicalSociety, 465, 4423--4433.<\/li>\n<li><span class=\"underline\">Y. Kojima<\/span>, &ldquo;Axisymmetric force-freemagnetosphere in the exterior of a neutron star,&rdquo; <em>Mon. Not.Roy. Astron. Soc.<\/em> 468, (2017) 2011.<\/li>\n<li>S. Iso, N. Oshita, R. Tatsukawa, <span class=\"underline\">K.Yamamoto<\/span>, &ldquo;Quantumadiation produced by the entanglement ofquantum fields,&rdquo; Physical Review D 95 023512 (2017).<\/li>\n<li><span class=\"underline\">K. Yamamoto<\/span>, Y. Nan, C. Hikage, &ldquo;Ananalytic halo approach to the bispectrum of galaxies in redshiftspace,&rdquo; Physical Review D 95 043528 (2017).<\/li>\n<li>R. Kimura, T. Tanaka, <span class=\"underline\">K. Yamamoto<\/span>,T. Yamashita, &ldquo;Constraint on ghost-free bigravity fromgravitational Cherenkov radiation,&rdquo; Physical Review D 94 064059(2016).<\/li>\n<li>Y. Ueno, <span class=\"underline\">K. Yamamoto<\/span>, &ldquo;Constraintson alpha-attractor inflation and reheating,&rdquo; Physical Review D 93083524 (2016).<\/li>\n<li>Ziparo, Felicia, Smith, Graham P., <span class=\"underline\">Okabe,Nobuhiro<\/span>, Haines, Chris P., Pereira, Maria J., Egami, Eiichi, &ldquo;LoCuSS: exploring the selection of faint blue background galaxiesfor cluster weak-lensing,&rdquo; Monthly Notices of the RoyalAstronomical Society, Volume 463 (2016) Issue 4, p.4004-4018.<\/li>\n<li>Jaff\u00e9,Yara L., Verheijen, MarcA.W., Haines, ChrisP., Yoon, Hyein,Cybulski, Ryan, Montero-Casta\u00f1o, Mar\u00eda, Smith, Rory, Chung, Aeree,Deshev, BorisZ., Fern\u00e1ndez, Ximena, van Gorkom, Jacqueline,Poggianti, Bianca M.;, Yun, Min S., Finoguenov, Alexis, Smith,Graham P., <span class=\"underline\">Okabe, Nobuhiro<\/span>, &ldquo;BUDHIES- III: the fate of H I and the quenching of galaxies in evolvingenvironments,&rdquo; Monthly Notices of the Royal Astronomical Society,Volume 461 (2016) Issue 2, p.1202-1221.<\/li>\n<li>Sasaki, Toru, Matsushita, Kyoko, Sato, Kosuke, <span class=\"underline\">Okabe, Nobuhiro<\/span>, &ldquo;X-ray observations of asubhalo associated with the NGC 4839 group infalling toward theComa cluster,&rdquo; Publications of the Astronomical Society of Japan,Volume 68 (2016) Issue 5, id.85 pp.<\/li>\n<li><span class=\"underline\">N. Okabe<\/span> and Graham P. Smith, &ldquo;LoCuSS: Weak-lensing mass calibration of galaxy clusters,&rdquo; MonthlyNotices of the Royal Astronomical Society, Volume 461 (2016) Issue4, p.3794-3821.<\/li>\n<li>Pierre, M. et al. (<span class=\"underline\">N. Okabe<\/span> 103th of111 authours), &ldquo;The XXL survey: first results and future,&rdquo; Astronomische Nachrichten, vol. 338 (2017) issue 2-3, pp. 334-341.<\/li>\n<li>J.Adam, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;W and Z boson productionin p-Pb collisions at \u221as<sub>NN<\/sub> = 5.02 TeV,&rdquo; <em>JHEP<\/em><strong>1702<\/strong>, 077, 2017.<\/li>\n<li>J.Adam, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Determination of theevent collision time with the ALICE detector at the LHC,&rdquo; <em>Euro.Phys. J. Plus<\/em> <strong>132<\/strong>, 99, 2017.<\/li>\n<li>J.Adam, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Jet-like correlationswith neutral pion triggers in pp and central Pb\u2013Pb collisions at 2.76TeV,&rdquo; <em>Phys. Lett.<\/em> <strong>B763<\/strong>, 238-250, 2016.<\/li>\n<li>J.Adam, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;J\/\u03c8 suppression atforward rapidity in Pb-Pb collisions at \u221as<sub>NN<\/sub> = 5.02 TeV,&rdquo; <em>Phys. Lett.<\/em> <strong>B766<\/strong>, 212-224, 2017.<\/li>\n<li>J.Adam, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Higher harmonic flowcoefficients of identified hadrons in Pb-Pb collisions at \u221as<sub>NN<\/sub>= 2.76 TeV,&rdquo; <em>JHEP<\/em> <strong>1609<\/strong>, 164, 2016.<\/li>\n<li>J.Adam, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Elliptic flow ofelectrons from heavy-flavour hadron decays at mid-rapidity in Pb-Pbcollisions at \u221as<sub>NN<\/sub> = 2.76 TeV,&rdquo; <em>JHEP<\/em><strong>1609<\/strong>, 028, 2016.<\/li>\n<li>J.Adam, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;D meson production inp-Pb collisions at \u221as<sub>NN<\/sub> = 5.02 TeV and in pp collisions at \u221as= 7 TeV,&rdquo; <em>Phys. Rev. C<\/em> <strong>94<\/strong>, 054908, 2016.<\/li>\n<li>J.Adam, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Pseudorapiditydependence of the anisotropic flow of charged particles in Pb-Pbcollisions at \u221as<sub>NN<\/sub> = 2.76 TeV,&rdquo; <em>Phys. Lett.<\/em><strong>B762<\/strong>, 376-388, 2016.<\/li>\n<li>J.Adam, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Correlatedevent-by-event fluctuations of flow harmonics in Pb-Pb collisions at\u221as<sub>NN<\/sub> = 2.76 TeV,&rdquo; <em>Phys. Rev. Lett.<\/em><strong>117<\/strong>, 182301, 2016.<\/li>\n<li>J.Adam, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Measurement oftransverse energy at midrapidity in Pb-Pb collisions at \u221as<sub>NN<\/sub> =2.76 TeV,&rdquo; <em>Phys. Rev. C<\/em> <strong>94<\/strong>, 034903, 2016.<\/li>\n<li>J.Adam, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Centrality dependence ofcharged jet production in p\u2013Pb collisions at \u221as<sub>NN<\/sub> = 5.02 TeV,&rdquo; <em>Euro. Phys. J.<\/em> <strong>C76<\/strong>, 271, 2016.<\/li>\n<li>J.Adam, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Centrality dependence of\u03c8(2S) suppression in p-Pb collisions at \u221as<sub>NN<\/sub> = 5.02 TeV,&rdquo; <em>JHEP<\/em> <strong>1606<\/strong>, 050, 2016.<\/li>\n<li>J.Adam, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Measurement of D mesonproduction versus multiplicity in p-Pb collisions at \u221as<sub>NN<\/sub> =5.02 TeV,&rdquo; <em>JHEP<\/em> <strong>1608<\/strong>, 078, 2016.<\/li>\n<li>J.Adam, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Particle identificationin ALICE: a Bayesian approach,&rdquo; <em>Euro. Phys. J. Plus<\/em><strong>131<\/strong>, 168, 2016.<\/li>\n<li>J.Adam, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Anisotropic flow ofcharged particles in Pb-Pb collisions at \u221as<sub>NN<\/sub> = 5.02 TeV,&rdquo; <em>Phys. Rev. Lett.<\/em> <strong>116<\/strong>, 132302, 2016.<\/li>\n<li>J.Adam, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Production ofK<sup>*<\/sup>(892)<sup>0<\/sup> and \u03d5(1020) in p\u2013Pb collisions at\u221as<sub>NN<\/sub> = 5.02 TeV,&rdquo; <em>Euro. Phys. J.<\/em><strong>C76<\/strong>, 245, 2016.<\/li>\n<li>J.Adam, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Multiplicity dependenceof charged pion, kaon, and (anti)proton production at large transversemomentum in p-Pb collisions at \u221as<sub>NN<\/sub> = 5.02 TeV,&rdquo; <em>Phys.Lett.<\/em> <strong>B760<\/strong>, 720-735, 2016.<\/li>\n<li>J.Adam, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Multipion Bose-Einsteincorrelations in pp, p-Pb, and Pb-Pb collisions at energies available atthe CERN Large Hadron Collider,&rdquo; <em>Phys. Rev. C<\/em><strong>93<\/strong>, 054908, 2016.<\/li>\n<li>J.Adam, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Multi-strange baryonproduction in p-Pb collisions at \u221as<sub>NN<\/sub> = 5.02 TeV,&rdquo; <em>Phys.Lett.<\/em> <strong>B758<\/strong>, 389-401, 2016.<\/li>\n<li>J.Adam, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Centrality dependence ofthe charged-particle multiplicity density at midrapidity in Pb-Pbcollisions at \u221as<sub>NN<\/sub> = 5.02 TeV,&rdquo; <em>Phys. Rev. Lett.<\/em><strong>116<\/strong>, 222302, 2016.<\/li>\n<li>J.Adam, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Charge-dependent flowand the search for the chiral magnetic wave in Pb-Pb collisions at\u221as<sub>NN<\/sub> = 2.76 TeV,&rdquo; <em>Phys. Rev. C<\/em> <strong>93<\/strong>,044903, 2016.<\/li>\n<li>J.Adam, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Measurement of an excessin the yield of J\/\u03c8 at very low pT in Pb-Pb collisions at \u221as<sub>NN<\/sub>= 2.76 TeV,&rdquo; <em>Phys. Rev. Lett.<\/em> <strong>116<\/strong>, 222301,2016.<\/li>\n<li>J.Adam, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Inclusive quarkoniumproduction at forward rapidity in pp collisions at \u221as = 8 TeV,&rdquo; <em>Euro.Phys. J.<\/em> <strong>C76<\/strong>, 184, 2016.<\/li>\n<li>J.Adam, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Charged-particlemultiplicities in proton\u2013proton collisions at \u221as = 0.9 to 8 TeV,&rdquo; <em>Euro. Phys. J.<\/em> <strong>C77<\/strong>, 33, 2017.<\/li>\n<li>J.Adam, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;\u03d5 meson production atforward rapidity in p-Pb collisions at \u221as<sub>NN<\/sub> = 5.02 TeV and inpp collisions at \u221as = 2.76 TeV,&rdquo; <em>Phys. Lett.<\/em><strong>B768<\/strong>, 203-217, 2017.<\/li>\n<li>J.Adam, <span class=\"underline\">K.Shigaki<\/span>, <span class=\"underline\">T.Sugitate<\/span>, <em>et al.<\/em>, &ldquo;Differential studies ofinclusive J\/\u03c8 and \u03c8(2S) production at forward rapidity in Pb-Pbcollisions at \u221as<sub>NN<\/sub> = 2.76 TeV,&rdquo; <em>JHEP<\/em><strong>1605<\/strong>, 179, 2016.<\/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 the relative yields of \u03c8(2S) to \u03c8(1S)mesons produced at forward and backward rapidity in p+p, p+Al, p+Au, and<sup>3<\/sup>He+Au collisions at \u221as<sub>NN<\/sub> =200 GeV,&rdquo; <em>Phys.Rev.<\/em> C<strong>95<\/strong>, 034904, 2017.<\/li>\n<li>C.Aidala, <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 long-range angular correlations andazimuthal anisotropies in high-multiplicity p+Au collisions at\u221as<sub>NN<\/sub> =200 GeV,&rdquo; <em>Phys. Rev.<\/em> C<strong>95<\/strong>,034910, 2017.<\/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;Measurements of double-helicity asymmetries ininclusive J\/\u03c8 production in longitudinally polarized p+p collisios at \u221as=510 GeV,&rdquo; <em>Phys. Rev.<\/em> D<strong>94<\/strong>, 112008, 2016.<\/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;Measurements of directed, elliptic, and triangular flowin Cu+Au collisions at \u221as<sub>NN<\/sub> =200 GeV,&rdquo; <em>Phys. Rev.<\/em>C<strong>94<\/strong>, 054910, 2016.<\/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;Azimuthally anisotropic emission of low-momentum directphotons in Au+Au collisions at \u221as<sub>NN<\/sub> =200 GeV,&rdquo; <em>Phys.Rev.<\/em> C<strong>94<\/strong>, 064901, 2016.<\/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 the higher-order anisotropic flowcoefficients for identified hadrons in Au+Au collisions at\u221as<sub>NN<\/sub> =200 GeV,&rdquo; <em>Phys. Rev.<\/em> C<strong>93<\/strong>,051902, 2016.<\/li>\n<li>Y.Akiba (ed.), S.Esumi (ed.), K.Fukushima (ed.), H.Hamagaki (ed.),T.Hatsuda (ed.), T.Hirano (ed.), and <span class=\"underline\">K.Shigaki<\/span> (ed.), &ldquo;Proceedings, 25th InternationalConference on Ultra-Relativistic Nucleus-Nucleus Collisions (Quark Matter2015) : Kobe, Japan, September 27-October 3, 2015,&rdquo; <em>Nucl. Phys.<\/em><strong>A956<\/strong>, 1-974, 2016.<\/li>\n<li>H.Sako, <span class=\"underline\">K.Shigaki<\/span>, <em>et al.<\/em>, &ldquo;Studies of high density baryon matter with high intensity heavy-ionbeams at J-PARC,&rdquo; <em>Nucl. Phys.<\/em> <strong>A956<\/strong>, 850-853,2016.<\/li>\n<li><span class=\"underline\">K. Homma<\/span>, <em>et al.<\/em>, &ldquo;CombinedLaser Gamma Experiments at ELI-NP,&rdquo; <em>Romanian Reports in Physics,Supplement,<\/em> 68, S233-S274, 2016.<\/li>\n<li>T. Minoshima, <span class=\"underline\">T. Miyoshi<\/span>, and S.Imada, &ldquo;Boosting magnetic reconnection by viscous and thermalconduction,&rdquo; <em>Phys. Plasmas<\/em> <strong>23<\/strong>, 072122, 2016.<\/li>\n<li><span class=\"underline\">\u672c\u9593\u8b19\u8f14<\/span>, &ldquo;\u8d85\u9ad8\u5f37\u5ea6\u30ec\u30fc\u30b6\u30fc\u5834\u3092\u7528\u3044\u305f\u5b87\u5b99\u6697\u9ed2\u5834\u306e\u63a2\u7d22,&rdquo; OPTRONICS (2016) No.7 35-39.<\/li>\n<li><span class=\"underline\">K.-I. Ishikawa<\/span>, Y. Iwasaki, YuNakayama, T. Yoshie, &ldquo;Non-trivial Center Dominance in High TemperatureQCD,&rdquo; Mod.Phys.Lett. A31 (2016) no.25, 1650150.<\/li>\n<li><span class=\"underline\">T. Morozumi<\/span>, K. I. Nagao, A. S.Adam, and H. Takata, &ldquo;Creation and Evolution of Particle Number Asymmetryin an expanding universe,&rdquo; Russian Physics Journal Vol.59, No. 11, March2017, p1852-p1856(Russian Original, Izv.Vuz.Fiz.59(2016) no.11,108-111).<\/li>\n<li>H. Okane and <span class=\"underline\">T. Morozumi<\/span>, &ldquo;Constraint on Seesaw Model Parameters with Electroweak VacuumStability,&rdquo; Russian Physics Journal, Vol. 59, No. 11, March, 2017,p1857-p1863 (Russian Original,Izv.Vuz.Fiz.59(2016) no.11,112-116).<\/li>\n<\/ul>\n\n<p><a id=\"presentations_H28\"><\/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\">Fukazawa, Y.<\/span>, &ldquo;Recent Fermi resultsof extragalactic objects and TeV gamma-rays&rdquo; , &ldquo;The extremeUniverse viewed in very-high-energy gamma-rays 2016&rdquo;, December15-16, 2016, University of Tokyo, Chiba, Japan.<\/li>\n<li><span class=\"underline\">Ohno, M.<\/span>, &ldquo;Studying GW sources withFermi Gamma-ray Space Telescope&rdquo;, GW Astro BiMonthlly Meeting, Feb.4, 2017, Tokyo Inst. of Tech.<\/li>\n<li><span class=\"underline\">Ohno, M.<\/span>, &ldquo;Investigation of physicalcondition of hot plasma in the clusters of galaxies&rdquo;, BunClubcolloquium, Nov. 18, 2016, Institute of Astronomy University ofCambridge, UK.<\/li>\n<li><span class=\"underline\">Ohno, M.<\/span>, &ldquo;Resonant scattering as aprobe of physical condition of hot plasma in the cluster ofgalaxies&rdquo;, KIPAC Tea Talk colloquium, Mar. 17, 2016, KavliInstitute for Particle Astrophysics and Cosmology, StanfordUniversity\/SLAC National Accelerator Laboratory, USA.<\/li>\n<li><span class=\"underline\">Takahashi, H.<\/span>, &ldquo;Overview of spectralchange in NS-LMXB&rdquo;, 7 years of MAXII: monitoring X-ray Transients,5-7 Dec. 2016, RIKEN, Japan.<\/li>\n<li><span class=\"underline\">Mizuno, T.<\/span>, &ldquo;Study of the ISM andCRs of the MBM 53,54,55 Clouds and the Pegasus Loop&rdquo;, InterstellarHydrogen Workshop 2016, Sep. 27-28, 2016, Nagoya University, Japan,20\u540d.<\/li>\n<li><span class=\"underline\">Yoshida, M.<\/span>, &ldquo;J-GEM: an EM Follow-upNetwork in Japan&rdquo;, Gravitational Wave Astrophysics in the EventRate Regime, Dec. 5-6, 2016, RESCUE\/University of Tokyo.<\/li>\n<li>Okada, C., &ldquo;Hard X-ray study of low mass X-ray binary Sco X-1 withSuzaku&rdquo;, 7 years of MAXI, RIKEN, Japan, Dec. 5-7, 2016, \u7d04150\u540d.<\/li>\n<li>Shiki, K., &ldquo;Kanata optical monitoring of radio galaxy NGC 1275&rdquo;, 7years of MAXI, RIKEN, Japan, Dec. 5-7, 2016, \u7d04150\u540d.<\/li>\n<li>Uchida, N., &ldquo;Development of an in-orbit radiation environmentmonitor CUBES onboard a small satellite MIST&rdquo;, 7 years of MAXI,RIKEN, Japan, Dec. 5-7, 2016, \u7d04150\u540d.<\/li>\n<li>Tanaka, K., &ldquo;Location of Gamma-ray Bursts with BGO Active Shield ofthe Soft Gamma-ray Detector and Hard X-ray Imager onboard Hitomi&rdquo;,7 years of MAXI, RIKEN, Japan, Dec. 5-7, 2016, \u7d04150\u540d.<\/li>\n<li>Toda, K., &ldquo;Revisiting the cosmological evolution of X-ray selectedblazars with the Swift\/BAT 70 month all sky survey data&rdquo;, 7 yearsof MAXI, RIKEN, Japan, Dec. 5-7, 2016, \u7d04150\u540d.<\/li>\n<li><span class=\"underline\">Fukazawa, Y.<\/span>, &ldquo;In-flight Performanceof the Soft Gamma-ray Detector (SGD) onboard Hitomi&rdquo;, 7 years ofMAXI, RIKEN, Japan, Dec. 5-7, 2016, \u7d04150\u540d.<\/li>\n<li><span class=\"underline\">Ohno, M.<\/span>, &ldquo;Development and in-orbitperformance of all-sky monitoring function of BGO active shield ofthe soft gamma-ray detector onboard Hitomi&rdquo;, 7 years of MAXI,RIKEN, Japan, Dec. 5-7, 2016, \u7d04150\u540d.<\/li>\n<li><span class=\"underline\">Ohno, M.<\/span>, &ldquo;Suzaku Wide-band All-skyMonitor view of soft gamma-ray transient&rdquo;, 7 years of MAXI, RIKEN,Japan, Dec. 5-7, 2016, \u7d04150\u540d.<\/li>\n<li><span class=\"underline\">Takahashi, H.<\/span>, &ldquo;PoGOLite, PoGO+ andSPHiNX&rdquo;, 2nd CORE-U International Conference: Cosmic Polarimetryfrom Micro to Macro Scales, Feb. 17-18, 2017, Hiroshima University,50\u540d.<\/li>\n<li>Miyaoka, K., &ldquo;X-ray mass measurement of massive galaxy clusters inthe HSC SSP survey region&rdquo;, The 6th Subaru InternationalConference, Nov. 28 - Dec. 2, 2016, Hiroshima, \u7d04200\u540d.<\/li>\n<li>Kawabata, M., &ldquo;Long-term Optical\/NIR Observations of Type IaxSupernova SN 2014dt&rdquo;, The Supernovae Through the Ages Conference,Hanga Roa, Easter Island, Chili, Aug. 9-13, 2016, 150\u540d.<\/li>\n<li>Nakaoka, T., &ldquo;Extended UV-NIR observations of Type IIP supernova2014cx from two days after the explosion&rdquo;, The Supernovae Throughthe Ages Conference, Hanga Roa, \uff25aster Island, Chili, Aug. 9-13,2016, 150\u540d.<\/li>\n<li>Kawabata, M., &ldquo;Long-term Optical\/NIR Observations of type Iaxsupernova SN 2014dt&rdquo;, Transient Universe in the Big Survey Era:Understanding the Nature of Astrophysical Explosive Phenomena,Kyoto University, Jan. 23-24, 2017, 70\u540d.<\/li>\n<li>Nakaoka, T., &ldquo;Optical-NIR observation of Low-Luminosity Type IIPSupernova 2016bkv&rdquo;, Transient Universe in the Big Survey Era:Understanding the Nature of Astrophysical Explosive Phenomena,Kyoto University, Jan. 23-24, 2017, 70\u540d.<\/li>\n<li>Kawahara, N., &ldquo;Kanata follow-up of SNe Ib\/c&rdquo;, Transient Universe inthe Big Survey Era: Understanding the Nature of AstrophysicalExplosive Phenomena, Kyoto University, Jan. 23-24, 2017, 70\u540d.<\/li>\n<li><span class=\"underline\">Yoshida, M.<\/span>, &ldquo;Summary of the A02sub-project&rdquo;, New development in astrophysics throughmultimessenger observations of gravitational wave sources, Dec. 26,2016, YITP, Kyoto University, 70\u540d.<\/li>\n<li><span class=\"underline\">Kawabata, K. S.<\/span> , &ldquo;OpticalPolarimetric Survey Project, SGMAP, and GW&rdquo;, New development inastrophysics through multimessenger observations of gravitationalwave sources, Dec. 26, 2016, YITP, Kyoto University, 70\u540d.<\/li>\n<li><span class=\"underline\">Tanaka, Y.<\/span> , &ldquo;No Evidence ofIntrinsic Optical\/Near-Infrared Linear Polarization or V404 CygniDuring its Bright Outburst in 2015: Broadband Modeling andConstraint on Jet Parameters&rdquo;, 2nd CORE-U International Conference:Cosmic Polarimetry from Micro to Macro Scales, Feb. 17-18, 2017,Hiroshima University, 50\u540d.<\/li>\n<li><span class=\"underline\">Kawabata, K. S.<\/span> , &ldquo;Future Project ofOptical Polarimetry in Northern Hemisphere, SGMAP&rdquo;, 2nd CORE-UInternational Conference: Cosmic Polarimetry from Micro to MacroScales, Feb. 17-18, 2017, Hiroshima University, 50\u540d.<\/li>\n<li><span class=\"underline\">Takahashi, H.<\/span>, &ldquo;PoGOLite, PoGO+ andSPHiNX&rdquo;, 2nd CORE-U International Conference: Cosmic Polarimetryfrom Micro to Macro Scales, Feb. 17-18, 2017, Hiroshima University,50\u540d.<\/li>\n<li><span class=\"underline\">Uemura, M.<\/span>, &ldquo;High-DimensionalData-Driven Approach to Type Ia Supernovae&rdquo;, The Supernovae Throughthe Ages Conference, Easter Island (Chili), Aug. 8-13, 2016, 150\u540d.<\/li>\n<li><span class=\"underline\">Uemura, M.<\/span>, &ldquo;TimeTybes:Visualization of polarization in blazars&rdquo;, Blazars through SharpMulti-Wavelength Eyes, May 31 - June 3, 2016, Malaga, Spain.<\/li>\n<li><span class=\"underline\">Yoshida, M.<\/span>, &ldquo;Japaneseelectromagnetic follow-up network for gravitational wave sources,J-GEM&rdquo;, The 2nd International Meeting on KAGRA, Nov. 10-12, 2016,Normal University, Beijing.<\/li>\n<li><span class=\"underline\">K. Yamamoto<\/span>\uff1a\u300cQuantum radiationproduced by the entanglement of quantum fields\u300d, Sendai Workshop onQuantum Information Physics,\u6771\u5317\u5927\u5b66\u7406\u5b66\u7814\u7a76\u79d1, \u5e73\u621029\u5e74\uff13\u670813\u65e5, \u7814\u7a76\u8005\uff0830\u540d\uff09.<\/li>\n<li><span class=\"underline\">Y. Kojima<\/span>: &ldquo;Damping of MagnetarOscillations induced by Giant Flares&rdquo;, (The 4th DTAsymposium:Compact stars and gravitational waveastronomy,\u5e73\u621028\u5e74\uff15\u670813-14\u65e5, \u56fd\u7acb\u5929\u6587\u53f0\uff09\uff08\u53c2\u52a0\u800530\u540d\uff09.<\/li>\n<li><span class=\"underline\">K. Yamamoto<\/span>\uff1a\u300cExploring topics on theborder of accelerating universe\u300d,\u65b0\u5b66\u8853\u9818\u57df(\u306a\u305c\u5b87\u5b99\u306f\u52a0\u901f\u3059\u308b\u306e\u304b?\u2014\u5fb9\u5e95\u7684\u7a76\u660e\u3068\u5c06\u6765\u3078\u306e\u6311\u6226-)KEK, \u5e73\u621029\u5e74\uff13\u6708\uff19\u65e5,\u7814\u7a76\u8005\uff08117\u540d\uff09.<\/li>\n<li><span class=\"underline\">Y. Kojima<\/span>: &ldquo;Force-free magneticstructure in the exterior of relativistic stars&rdquo;, (JGRG26,\u5e73\u621028\u5e7410\u670824 -28\u65e5, \u5927\u962a\u5e02\u7acb\u5927\u5b66)\uff08\u53c2\u52a0\u8005150\u540d\uff09.<\/li>\n<li><span class=\"underline\">Y. Kojima<\/span>: &ldquo;Building up energybefore magnetar bursts&rdquo;, (\u65b0\u5b66\u8853\u9818\u57df\uff08\u91cd\u529b\u6ce2\u5929\u4f53\uff09\u30b7\u30f3\u30dd\u30b8\u30a6\u30e0, \u5e73\u621028\u5e7412\u670826 -28\u65e5,\u4eac\u90fd\u5927\u5b66)\uff08\u53c2\u52a0\u8005150\u540d\uff09.<\/li>\n<li><span class=\"underline\">K. Yamamoto<\/span>:\u300cQuantum radiation fromUnruh-De Witt detector\u300dJGRG26,\u5e73\u621028\u5e7410\u670828\u65e5, \u5927\u962a\u5e02\u7acb\u5927\u5b66.<\/li>\n<li><span class=\"underline\">K. Yamamoto<\/span>: \u300cHalo approach to powerspectrum and bispectrum of galaxies in redshift space \u300d(posterpresentation) The 6<sup>th<\/sup> Subaru International conference inHiroshima, Panoramas of the Evolving Cosmology, Internationalconference center Hiroshima, \u5e73\u621028\u5e7411\u670828\u65e5-12\u6708\uff12\u65e5.<\/li>\n<li><span class=\"underline\">N. Okabe<\/span>: &ldquo;Joint X-ray andSubaru\/HSC Weak-lensing Analysis of Very Nearby Galaxy Clusters&rdquo;Hot spots in the XMM sky: Cosmology from X-ray to Radio, MykonosIsland, Greece, June,15-18, 2016.<\/li>\n<li><span class=\"underline\">N. Okabe<\/span>: &ldquo;NECSUS : Subaru\/HSCWeak-lensing Analysis of Very Nearby Galaxy Clusters&rdquo;, Panoramas ofthe Evolving Cosmos, the 6th Subaru International conference, Nov28- Dec 2, 2016, International Conference Center Hiroshima.<\/li>\n<li><span class=\"underline\">T.Sugitate<\/span>, &ldquo;Japan Status Report&rdquo;,2nd Asia Tier Center Forum, Suranaree University of Technology,(Nakhon Ratchasima, Thailand, 2016.11.30-12.2).<\/li>\n<li><span class=\"underline\">K.Shigaki<\/span>, &ldquo;Dreams in the LHC HeavyIon Programme&rdquo;, 71<sup>st<\/sup> Fujihara Seminar &ldquo;Interplay betweenHadronic, Nuclear and Atomic Physics&rdquo; (Shimoda, Japan, 2016.7.6-8).<\/li>\n<li><span class=\"underline\">K. Homma<\/span>, &ldquo;Potential to search forDark Matter with multi-wavelengths light sources&rdquo;, Extreme LightScientific and Socio-Economic Outlook (Paris, France, 2016.11.30).<\/li>\n<li><span class=\"underline\">K. Homma<\/span>, <em>et al.<\/em>,&ldquo;Extracting phase retardation of GeV photons to probe vacuumbirefringence in high-intensity laser fields&rdquo;, 25th ANNUALINTERNATIONAL LASER PHYSICS WORKSHOP (Yerevan, Armenia, 2016.7.13).<\/li>\n<li><span class=\"underline\">K. Homma<\/span>, <em>et al.<\/em>, &ldquo;Searchfor dark components in the Universe with high-intensity lasers&rdquo;,Energy, Material &amp; Nanotechnology meeting on Laser MatterInteractions (Singapore, 2016.5.12).<\/li>\n<li><span class=\"underline\">T. Sugitate<\/span>, &ldquo;Status of ALICE-Japanand Tiers&rdquo;, ALICE Calo Meeting in Moscow, National Research Center&ldquo;Kurchatov Institute&rdquo; (Moscow, Russia, 2016.9.12-9.13).<\/li>\n<li><span class=\"underline\">K. Homma<\/span>, &ldquo;Prospects of directsearch for dilation\/axion fields with extreme high-intensitylasers&rdquo;, Why dose the Universe accelerate - Exhaustive study andthe challenge for the future (Tsukuba, Japan, 2017.3.8).<\/li>\n<li><span class=\"underline\">K. Homma<\/span>, &ldquo;Probing pseudoNambu-Goldstone bosons via multi-wavelengths four-wave mixing&rdquo;,Axion Dark Matter 2016 (Stockholm, Sweden, 2016.12.7).<\/li>\n<li><span class=\"underline\">K.Shigaki<\/span> for the ALICECollaboration, &ldquo;Detector Control System of the new Muon ForwardTracker at ALICE&rdquo; (poster), Quark Matter 2017 (Chicago, U.S.A.,2017.2.6-11).<\/li>\n<li><span class=\"underline\">T. Miyoshi<\/span>, T. Minoshima, and Y.Matsumoto, &ldquo;Weighted Compact Nonlinear Scheme for MultidimensionalMagnetohydrodynamics&rdquo;, 18th International Congress on PlasmaPhyscis (ICPP2016), Kaohsiung Exhibition Center, (Kaohsiung,Taiwan, 2016.6.27-7.1).<\/li>\n<li>T. Minoshima, <span class=\"underline\">T. Miyoshi<\/span>, and S.Imada, &ldquo;Boosting Magnetic Reconnection by Viscosity and ThermalConduction&rdquo;, 18th International Congress on Plasma Physcis(ICPP2016), Kaohsiung Exhibition Center, (Kaohsiung, Taiwan,2016.6.27-7.1).<\/li>\n<li><span class=\"underline\">T. Miyoshi<\/span>, &ldquo;A Hint from PlasmaPhysics for Quark-Gluon Plasma Physics&rdquo;, ALICE Calo Meeting, NRCKurchatov Institute, (Moscow, Russia, 2016.9.12-9.13).<\/li>\n<li>T. Shibayama, K. Kusano, <span class=\"underline\">T. Miyoshi<\/span>,and G. Vekstein &ldquo;MHD 2D Fast Reconnection Theory Beyond PlasmoidChain Reconnection&rdquo;, The US-Japan Workshop and School on MagneticReconnection (MR2017), Himegin Hall, (Matsuyama, Japan,2017.3.19-3.23).<\/li>\n<li>M. Garcia Perez, A. Gonzalez-Arroyo, <span class=\"underline\">M.Okawa<\/span>, &ldquo;Meson masses and decay constants at large N&rdquo;, PoSLATTICE2016 (2016) 319.<\/li>\n<li>M. Garcia Perez, A. Gonzalez-Arroyo, <span class=\"underline\">M.Okawa<\/span>, &ldquo;Volume reduction through perturbative Wilson loops&rdquo;, PoSLATTICE2016 (2016) 329.<\/li>\n<li>M. Garcia Perez, A. Gonzalez-Arroyo, <span class=\"underline\">M.Okawa<\/span>, &ldquo;`t Hooft model on the Lattice&rdquo;, PoS LATTICE2016 (2016)337.<\/li>\n<li>Takeshi Yamazaki, <span class=\"underline\">Ken-IchiIshikawa<\/span>, Yoshinobu Kuramashi, Akira Ukawa, for PACSCollaboration, &ldquo;Systematic study of operator dependence in nucleuscalculation at large quark mass&rdquo;, PoS LATTICE2016 (2017) 108.<\/li>\n<li>Taisuke Boku, <span class=\"underline\">Ken-Ichi Ishikawa<\/span>,Yoshinobu Kuramashi, Lawrence Meadows, Michael D`Mello, Maurice Troute,Ravi Vemuri, &ldquo;A performance evaluation of CCS QCD Benchmark on the COMA(Intel(R) Xeon PhiTM, KNC) system&rdquo;, PoS(LATTICE2016)261.<\/li>\n<li><span class=\"underline\">Ken-Ichi Ishikawa<\/span>, Issaku Kanamori,Yuko Murakami, Ayaka Nakamura, <span class=\"underline\">MasanoriOkawa<\/span>, Ryoichiro Ueno, &ldquo;Numerical determination of the \u039b-parameterin SU(3) gauge theory from the twisted gradient flow coupling&rdquo;,PoS(LATTICE2016) 185.<\/li>\n<li><span class=\"underline\">Takuya Morozumi<\/span>, &ldquo;Particle numberasymmetry induced with CP violating interaction&rdquo;, Quntum Field Theoryand Gravity 2016, Aug.2016, Tomsk, Russia.<\/li>\n<li><span class=\"underline\">Takuya Morozumi<\/span>, &ldquo;The creation ofthe particle number asymmetry in the universe&rdquo;, the 4 th Internatinalworkshop on Dark Matter,Dark Energy and Matter andanti-Matter Asymmetry 30<sup>th<\/sup> Dec.2016 NTHU, Hsinchu ,Taiwan.<\/li>\n<li>Hideaki Okane, <span class=\"underline\">Takuya Morozumi<\/span>,&ldquo;The Effect of Neutrino on the Meta-Stability of Electroweak Vacuum&rdquo;;December 29-31th 2016; 4th International Workshop on Dark Matter, DarkEnergy and Matter Antimatter Asymmetry; NTHU, Hsinchu.<\/li>\n<li>Apriadi Salim Adam, <span class=\"underline\">T. Morozumi<\/span>, K.I. Nagao and H. Takata, &ldquo;The creation of particle number asymmetry ofuniverse with arbitrary scale factor using perturbation method&rdquo;, KEK-PH2017, February 14-17th 2017 at KEK Tsukuba.<\/li>\n<li>T. Inagaki, S. D. Odintsov, and H. Sakamoto, &ldquo;Analysis of CMBfluctuations for gauged Nambu-Jona-Lasinio model&rdquo;, SCD2016, Aug. 2016,Tomsk, Russia.<\/li>\n<li>T. Inagaki, S. D. Odintsov, and H. Sakamoto, &ldquo;Inflation in GaugedNambu-Jona-Lasinio model&rdquo;, Quantum Field Theory and Gravity (QFTG2016),Aug. 2016, Tomsk, Russia.<\/li>\n<li>T. Inagaki, S. D. Odintsov, and H. Sakamoto, &ldquo;Attractor Structureof Gauged Nambu-Jona-Lasinio Model&rdquo;, The 3rd KMI InternationalSymposium on &ldquo;Quest for the Origin of Particles and the Universe&rdquo;, Jan.2017, Nagoya, Japan.<\/li>\n<li><span class=\"underline\">\u6df1\u6ca2\u6cf0\u53f8<\/span>\uff1a\u300c\uff38\u7dda\u89b3\u6e2c\u88c5\u7f6e\u958b\u767a\u3068\u5927\u5b66\u9662\u751f\u300d,\u53ef\u8996\u8d64\u5916\u7dda\u89b3\u6e2c\u88c5\u7f6e\u6280\u8853\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d7,2016\u5e7411\u670824-25\u65e5,\u56fd\u7acb\u5929\u6587\u53f0\u4e09\u9df9.<\/li>\n<li><span class=\"underline\">\u6df1\u6ca2\u6cf0\u53f8<\/span>\uff1a\u300c\uff38\u7dda\u30ac\u30f3\u30de\u7dda\u89b3\u6e2c\u3068\u89b3\u6e2c\u7684\u5b87\u5b99\u300d,\u7b2c\uff15\u56de\u89b3\u6e2c\u7684\u5b87\u5b99\u8ad6\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d7,11\u670824-26\u65e5,\u5e83\u5cf6\u5927\u5b66.<\/li>\n<li><span class=\"underline\">\u5409\u7530\u9053\u5229<\/span>\uff1a\u300c\u91cd\u529b\u6ce2\u306e\u5149\u5b66\u5bfe\u5fdc\u5929\u4f53\u63a2\u67fb\u30cd\u30c3\u30c8\u30ef\u30fc\u30afJ-GEM\u300d.<\/li>\n<li><span class=\"underline\">\u7530\u4e2d\u5eb7\u4e4b<\/span>\uff1a\u300c\u30d5\u30a7\u30eb\u30df\u885b\u661f\u306e\u73fe\u72b6\u3068IceCube\u30cb\u30e5\u30fc\u30c8\u30ea\u30ce\u30a4\u30d9\u30f3\u30c8\u306e\u53ef\u8996\u8fd1\u8d64\u5916\u7dda\u30d5\u30a9\u30ed\u30fc\u30a2\u30c3\u30d7\u89b3\u6e2c\u300d.<\/li>\n<li><span class=\"underline\">\u9ad8\u6a4b\u5f18\u5145<\/span>\uff1a\u300c\u8cea\u91cf\u964d\u7740\u7387\u306e\u9ad8\u3044\u4f4e\u8cea\u91cf\uff38\u7dda\u9023\u661f\u300d,MAXI\u30c1\u30fc\u30e0\u7406\u7814\u30bb\u30df\u30ca\u30fc,2016\u5e74\uff18\u670829-30\u65e5,\u7406\u7814.<\/li>\n<li><span class=\"underline\">\u7530\u4e2d\u5eb7\u4e4b<\/span>\uff1a\u300c\u30d5\u30a7\u30eb\u30df\u885b\u661f\u306b\u3088\u308bMeV\/GeV\u30ac\u30f3\u30de\u7dda\u89b3\u6e2c\u306e\u6210\u679c\u3068\u30d5\u30a7\u30eb\u30df\u304b\u3089\u306e\u671f\u5f85\u300d,\u7b2c\uff11\u56deMeV\u30ac\u30f3\u30de\u7dda\u5929\u6587\u5b66\u7814\u7a76\u4f1a,2017\u5e74\uff12\u670827-28\u65e5,\u4eac\u90fd\u5927\u5b66,50\u540d.<\/li>\n<li><span class=\"underline\">\u5ddd\u7aef\u5f18\u6cbb<\/span>:\u300c\u5e83\u5cf61.5m\u93e1\u306b\u3088\u308b\u53ef\u8996\u8fd1\u8d64\u5916\u89b3\u6e2c\u3067\u6311\u3093\u3060\u7a81\u767a\u5929\u4f53\u7814\u7a76\u3053\u306e10\u5e74\u3068\u4eca\u5f8c\u306e\u591a\u6ce2\u9577\u9023\u643a\u300d, \u8328\u57ce\u5927\u5b66\u91cd\u70b9\u7814\u7a76\u7814\u7a76\u4f1a\uff1a\u300c\u7a81\u767a\u30fb\u5909\u52d5\u5929\u4f53\u306e\u591a\u6ce2\u9577\u9023\u643a\u89b3\u6e2c\u300d, 2016\u5e74\uff13\u6708\uff16\uff5e\uff17\u65e5, \u8328\u57ce\u5927\u5b66, 40\u540d.<\/li>\n<li><span class=\"underline\">\u6df1\u6ca2\u6cf0\u53f8<\/span>\uff1a\u300c\uff38\u7dda\u5929\u6587\u885b\u661f\u300c\u3072\u3068\u307f(ASTRO-H)\u300d\u642d\u8f09\u8edf\u30ac\u30f3\u30de\u7dda\u691c\u51fa\u5668 (SGD)\u306e\u8ecc\u9053\u4e0a\u52d5\u4f5c\u300d,\u65e5\u672c\u5929\u6587\u5b66\u4f1a\u79cb\u306e\u5e74\u4f1a,2016\u5e74\uff19\u670814-16\u65e5,\u611b\u5a9b\u5927\u5b66\u57ce\u5317\u30ad\u30e3\u30f3\u30d1\u30b9.<\/li>\n<li><span class=\"underline\">\u690d\u6751 \u8aa0<\/span>\uff1a\u300c\u30d6\u30ec\u30fc\u30b6\u30fc\u3067\u89b3\u6e2c\u3055\u308c\u308b\u504f\u5149\u306e\u6642\u9593\u5909\u52d5\u306e\uff13\u6b21\u5143\u53ef\u8996\u5316\u300d,\u65e5\u672c\u5929\u6587\u5b66\u4f1a\u79cb\u306e\u5e74\u4f1a,2016\u5e74\uff19\u670814-16\u65e5,\u611b\u5a9b\u5927\u5b66\u57ce\u5317\u30ad\u30e3\u30f3\u30d1\u30b9.<\/li>\n<li><span class=\"underline\">\u6c34\u91ce\u6052\u53f2<\/span>\uff1a\u300c\u30d5\u30a7\u30eb\u30df\u885b\u661f LAT \u691c\u51fa\u5668\u306b\u3088\u308b MBM 53,54,55\u304a\u3088\u3073 Pegasus Loop \u9818\u57df\u306e\u89b3\u6e2c\u300d,\u65e5\u672c\u5929\u6587\u5b66\u4f1a\u79cb\u306e\u5e74\u4f1a,2016\u5e74\uff19\u670814-16\u65e5,\u611b\u5a9b\u5927\u5b66\u57ce\u5317\u30ad\u30e3\u30f3\u30d1\u30b9.<\/li>\n<li><span class=\"underline\">\u9ad8\u6a4b\u5f18\u5145<\/span>\uff1a\u300c\u786c\uff38\u7dda\u504f\u5149\u691c\u51fa\u5668 PoGOLite\u6c17\u7403\u5b9f\u9a13:2016\u5e74\u306e\u518d\u30d5\u30e9\u30a4\u30c8\u300d,\u65e5\u672c\u5929\u6587\u5b66\u4f1a\u79cb\u306e\u5e74\u4f1a,2016\u5e74\uff19\u670814-16\u65e5,\u611b\u5a9b\u5927\u5b66\u57ce\u5317\u30ad\u30e3\u30f3\u30d1\u30b9.<\/li>\n<li><span class=\"underline\">\u5927\u91ce\u96c5\u529f<\/span>\uff1a\u300c\u300c\u3072\u3068\u307f(ASTRO-H)\u300d\u642d\u8f09\u786c\uff38\u7dda\u8edf\u30ac\u30f3\u30de\u7dda\u691c\u51fa\u5668\u306b\u304a\u3051\u308b BGO\u30a2\u30af\u30c6\u30a3\u30d6\u30b7\u30fc\u30eb\u30c9\u306e\u8ecc\u9053\u4e0a\u6027\u80fd\u300d,\u65e5\u672c\u5929\u6587\u5b66\u4f1a\u79cb\u306e\u5e74\u4f1a,2016\u5e74\uff19\u670814-16\u65e5,\u611b\u5a9b\u5927\u5b66\u57ce\u5317\u30ad\u30e3\u30f3\u30d1\u30b9.<\/li>\n<li><span class=\"underline\">\u7530\u4e2d\u5eb7\u4e4b<\/span>\uff1a\u300cGeV - TeV \u30ac\u30f3\u30de\u7dda\u30c7\u30fc\u30bf\u306b\u3088\u308b HBL \u5929\u4f53\u306e\u5e73\u5747SED \u3068TeV \u30ac\u30f3\u30de\u7dda\u80cc\u666f\u653e\u5c04\u306e\u8d64\u65b9\u504f\u79fb\u5206\u5e03\u300d,\u65e5\u672c\u5929\u6587\u5b66\u4f1a\u79cb\u306e\u5e74\u4f1a,2016\u5e74\uff19\u670814-16\u65e5,\u611b\u5a9b\u5927\u5b66\u57ce\u5317\u30ad\u30e3\u30f3\u30d1\u30b9.<\/li>\n<li><span class=\"underline\">\u5185\u6d77\u6d0b\u8f14<\/span>\uff1a\u300c\u30c1\u30d9\u30c3\u30c8\u30ed\u30dc\u30c3\u30c8\u4e09\u8272\u64ae\u50cf\u30ab\u30e1\u30e9\uff08HinOTORI\uff09:\u8f38\u9001\u3068\u5efa\u8a2d\u300d,\u65e5\u672c\u5929\u6587\u5b66\u4f1a\u79cb\u306e\u5e74\u4f1a,2016\u5e74\uff19\u670814-16\u65e5,\u611b\u5a9b\u5927\u5b66\u57ce\u5317\u30ad\u30e3\u30f3\u30d1\u30b9.<\/li>\n<li>\u4e2d\u5ca1\u7adc\u4e5f\uff1a\u300cIIP \u578b\u8d85\u65b0\u661f SN 2016X\u306e\u65e9\u671f\u89b3\u6e2c\u306b\u57fa\u3065\u304f\u7206\u767a\u76f4\u5f8c\u306e\u5149\u7403\u306e\u9032\u5316\u300d,\u65e5\u672c\u5929\u6587\u5b66\u4f1a\u79cb\u306e\u5e74\u4f1a,2016\u5e74\uff19\u670814-16\u65e5,\u611b\u5a9b\u5927\u5b66\u57ce\u5317\u30ad\u30e3\u30f3\u30d1\u30b9.<\/li>\n<li>\u5927\u6a4b\u793c\u6075\uff1a\u300c\u786c\uff38\u7dda\u504f\u5149\u691c\u51fa\u5668 PoGOLite \u306e\u8aad\u307f\u51fa\u3057\u56de\u8def\u306e\u6539\u826f(\uff12)\u300d,\u65e5\u672c\u5929\u6587\u5b66\u4f1a\u79cb\u306e\u5e74\u4f1a,2016\u5e74\uff19\u670814-16\u65e5,\u611b\u5a9b\u5927\u5b66\u57ce\u5317\u30ad\u30e3\u30f3\u30d1\u30b9.<\/li>\n<li>\u5ca1\u7530\u5343\u7a42\uff1a\u300c\u300c\u3059\u3056\u304f\u300d\u885b\u661f\u306b\u3088\u308b\u4f4e\u8cea\u91cf\uff38\u7dda\u9023\u661f Sco X-1 \u306e\u786c\uff38\u7dda\u653e\u5c04\u306e\u89b3\u6e2c(2)\u300d,\u65e5\u672c\u5929\u6587\u5b66\u4f1a\u79cb\u306e\u5e74\u4f1a,2016\u5e74\uff19\u670814-16\u65e5,\u611b\u5a9b\u5927\u5b66\u57ce\u5317\u30ad\u30e3\u30f3\u30d1\u30b9.<\/li>\n<li>\u5bfa\u524d\u62d3\u4eba\uff1a\u300cGeant4\u3092\u7528\u3044\u305f\u6955\u5186\u9280\u6cb3\u4e2d\u5fc3\u306b\u304a\u3051\u308b\u5171\u9cf4\u6563\u4e71\u306e\u5f71\u97ff\u306e\u8a55\u4fa1\u300d,\u65e5\u672c\u5929\u6587\u5b66\u4f1a\u79cb\u306e\u5e74\u4f1a,2016\u5e74\uff19\u670814-16\u65e5,\u611b\u5a9b\u5927\u5b66\u57ce\u5317\u30ad\u30e3\u30f3\u30d1\u30b9.<\/li>\n<li>\u5ee3\u5730 \u8ac4\uff1a\u300c\u9ad8\u8f1d\u5ea6\u8d64\u8272\u65b0\u661f M31 LRN 2015\u306e\u7206\u767a\u524d\u5929\u4f53\u306e\u89b3\u6e2c\u7684\u7814\u7a76\u300d,\u65e5\u672c\u5929\u6587\u5b66\u4f1a\u79cb\u306e\u5e74\u4f1a,2016\u5e74\uff19\u670814-16\u65e5,\u611b\u5a9b\u5927\u5b66\u57ce\u5317\u30ad\u30e3\u30f3\u30d1\u30b9.<\/li>\n<li>\u6238\u7530\u7693\u967d\uff1a\uff62Swift\u885b\u661f\u306e\u786c\uff38\u7dda\u30b5\u30fc\u30d9\u30a4\u30c7\u30fc\u30bf\u306b\u57fa\u3065\u304f\u30d6\u30ec\u30fc\u30b6\u30fc\u306elogN-logS\u5206\u5e03\u306e\u69cb\u7bc9\u300d,\u65e5\u672c\u5929\u6587\u5b66\u4f1a\u79cb\u306e\u5e74\u4f1a,2016\u5e74\uff19\u670814-16\u65e5,\u611b\u5a9b\u5927\u5b66\u57ce\u5317\u30ad\u30e3\u30f3\u30d1\u30b9.<\/li>\n<li>\u7530\u4e2d\u6643\u53f8\uff1a\u300c\uff62\u3072\u3068\u307f(ASTRO-H)\u300d\u642d\u8f09SGD\u306eBGO\u30b7\u30fc\u30eb\u30c9\u3092\u7528\u3044\u305f\u30ac\u30f3\u30de\u7dda\u30d0\u30fc\u30b9\u30c8\u4f4d\u7f6e\u6c7a\u5b9a\u80fd\u529b\u306e\u8a55\u4fa1\u300d,\u65e5\u672c\u5929\u6587\u5b66\u4f1a\u79cb\u306e\u5e74\u4f1a,2016\u5e74\uff19\u670814-16\u65e5,\u611b\u5a9b\u5927\u5b66\u57ce\u5317\u30ad\u30e3\u30f3\u30d1\u30b9.<\/li>\n<li>\u5bae\u5ca1\u656c\u592a\uff1a\u300cSubaru\/HSC\u30b5\u30fc\u30d9\u30a4\u9818\u57df\u306b\u3042\u308b\u91cd\u91cf\u7d1a\u9280\u6cb3\u56e3\u306e\uff38\u7dda\u89b3\u6e2c\u306b\u3088\u308b\u8cea\u91cf\u63a8\u5b9a\u300d,\u65e5\u672c\u5929\u6587\u5b66\u4f1a\u79cb\u306e\u5e74\u4f1a,2016\u5e74\uff19\u670814-16\u65e5,\u611b\u5a9b\u5927\u5b66\u57ce\u5317\u30ad\u30e3\u30f3\u30d1\u30b9.<\/li>\n<li>\u7530\u4e2d\u614e\u4e4b\uff1a\u300c\u5e83\u304c\u3063\u305f TeV \u30ac\u30f3\u30de\u7dda\u6e90 VER J2019+368\u306e\uff38\u7dda\u89b3\u6e2c\u300d,\u65e5\u672c\u5929\u6587\u5b66\u4f1a\u79cb\u306e\u5e74\u4f1a,2016\u5e74\uff19\u670814-16\u65e5,\u611b\u5a9b\u5927\u5b66\u57ce\u5317\u30ad\u30e3\u30f3\u30d1\u30b9.<\/li>\n<li>\u68ee \u88d5\u6a39\uff1a\u300cHONIR\u7528\u65b0\u691c\u51fa\u5668\u8aad\u307f\u51fa\u3057\u30b7\u30b9\u30c6\u30e0\u306e\u30ce\u30a4\u30ba\u6539\u5584\u306b\u5411\u3051\u305f\u7814\u7a76\u300d,\u65e5\u672c\u5929\u6587\u5b66\u4f1a\u79cb\u306e\u5e74\u4f1a,2016\u5e74\uff19\u670814-16\u65e5,\u611b\u5a9b\u5927\u5b66\u57ce\u5317\u30ad\u30e3\u30f3\u30d1\u30b9.<\/li>\n<li><span class=\"underline\">\u6c34\u91ce\u6052\u53f2<\/span>\uff1a\uff62\u300c\u3059\u3056\u304f\u300d\u306b\u3088\u308b\u5e83\u304c\u3063\u305fTeV\u30ac\u30f3\u30de\u7dda\u653e\u5c04VERJ2019+368\u306e\uff38\u7dda\u89b3\u6e2c(\uff13)\u300d,\u7269\u7406\u5b66\u4f1a\u79cb\u5b63\u5927\u4f1a,2016\u5e74\uff19\u670821-24\u65e5,\u5bae\u5d0e\u5927\u5b66\u6728\u82b1\u30ad\u30e3\u30f3\u30d1\u30b9.<\/li>\n<li><span class=\"underline\">\u9ad8\u6a4b\u5f18\u5145<\/span>\uff1a\u300c\u786c\uff38\u7dda\u504f\u5149\u691c\u51fa\u5668PoGOLite\u6c17\u7403\u5b9f\u9a13\uff1a2016\u5e74\u306e\u518d\u30d5\u30e9\u30a4\u30c8\u300d,\u7269\u7406\u5b66\u4f1a\u79cb\u5b63\u5927\u4f1a,2016\u5e74\uff19\u670821-24\u65e5,\u5bae\u5d0e\u5927\u5b66\u6728\u82b1\u30ad\u30e3\u30f3\u30d1\u30b9.<\/li>\n<li><span class=\"underline\">\u5927\u91ce\u96c5\u529f<\/span>\uff1a\u300c\u300c\u3072\u3068\u307f(ASTRO-H)\u300d\u885b\u661f\u642d\u8f09\u786c\uff38\u7dda\u8edf\u30ac\u30f3\u30de\u7dda\u691c\u51fa\u5668BGO\u30a2\u30af\u30c6\u30a3\u30d6\u30b7\u30fc\u30eb\u30c9\u306e\u8ecc\u9053\u4e0a\u6027\u80fd\u300d,\u7269\u7406\u5b66\u4f1a\u79cb\u5b63\u5927\u4f1a,2016\u5e74\uff19\u670821-24\u65e5,\u5bae\u5d0e\u5927\u5b66\u6728\u82b1\u30ad\u30e3\u30f3\u30d1\u30b9.<\/li>\n<li><span class=\"underline\">\u5317\u53e3\u8cb4\u96c4<\/span>\uff1a\u300c\u5149\u96fb\u5b50\u8ffd\u8de1\u578b\uff38\u7dda\u504f\u5149\u8a08\u306e\u98db\u8de1\u753b\u50cf\u51e6\u7406\u306e\u958b\u767a\u300d,\u7269\u7406\u5b66\u4f1a\u79cb\u5b63\u5927\u4f1a,2016\u5e74\uff19\u670821-24\u65e5,\u5bae\u5d0e\u5927\u5b66\u6728\u82b1\u30ad\u30e3\u30f3\u30d1\u30b9.<\/li>\n<li>\u5185\u7530\u548c\u6d77\uff1a\u300c\u5c0f\u578b\u885b\u661fMIST\u642d\u8f09 \u8ecc\u9053\u653e\u5c04\u7dda\u30e2\u30cb\u30bf\u30fcCUBES\u306e\u691c\u51fa\u5668\u958b\u767a\u300d,\u7269\u7406\u5b66\u4f1a\u79cb\u5b63\u5927\u4f1a,2016\u5e74\uff19\u670821-24\u65e5,\u5bae\u5d0e\u5927\u5b66\u6728\u82b1\u30ad\u30e3\u30f3\u30d1\u30b9.<\/li>\n<li><span class=\"underline\">\u5ddd\u7aef\u5f18\u6cbb<\/span>\uff1a\u300c\u53ef\u8996\u504f\u5149\u30b5\u30fc\u30d9\u30a4\u8a08\u753b SGMAP:\u304b\u306a\u305f\u671b\u9060\u93e1\u3067\u306e\u5b9f\u65bd\u691c\u8a0e\u300d,\u5929\u6587\u5b66\u4f1a\u6625\u306e\u5e74\u4f1a,2017\u5e74\uff13\u670815-18\u65e5,\u4e5d\u5dde\u5927\u5b66\u4f0a\u90fd\u30ad\u30e3\u30f3\u30d1\u30b9.<\/li>\n<li><span class=\"underline\">\u690d\u6751 \u8aa0<\/span>\uff1a\u300c\u30d6\u30ec\u30fc\u30b6\u30fc PKS 1749+096\u306e\u53ef\u8996\u504f\u5149\u89b3\u6e2c\u304b\u3089\u63a2\u308b\u30b8\u30a7\u30c3\u30c8\u306e\u78c1\u5834\u69cb\u9020\u300d,\u5929\u6587\u5b66\u4f1a\u6625\u306e\u5e74\u4f1a,2017\u5e74\uff13\u670815-18\u65e5,\u4e5d\u5dde\u5927\u5b66\u4f0a\u90fd\u30ad\u30e3\u30f3\u30d1\u30b9.<\/li>\n<li><span class=\"underline\">\u7530\u4e2d\u5eb7\u4e4b<\/span>\uff1a\u300c\u30b8\u30a7\u30c3\u30c8\u3092\u4f34\u3046\u6f6e\u6c50\u7834\u58ca\u73fe\u8c61\u306b\u304a\u3051\u308b\u30ac\u30f3\u30de\u7dda\u653e\u5c04\u306e\u63a2\u7d22\u3068\u653e\u5c04\u6a5f\u69cb\u306e\u89e3\u660e\u6e2c\u300d,\u5929\u6587\u5b66\u4f1a\u6625\u306e\u5e74\u4f1a,2017\u5e74\uff13\u670815-18\u65e5,\u4e5d\u5dde\u5927\u5b66\u4f0a\u90fd\u30ad\u30e3\u30f3\u30d1\u30b9.<\/li>\n<li><span class=\"underline\">\u9ad8\u6a4b\u5f18\u5145<\/span>\uff1a\u300c\u5927\u578b\u4f4e\u6e29\u91cd\u529b\u6ce2\u671b\u9060\u93e1 KAGRA:\u5168\u4f53\u5831\u544a\u300d,\u5929\u6587\u5b66\u4f1a\u6625\u306e\u5e74\u4f1a,2017\u5e74\uff13\u670815-18\u65e5,\u4e5d\u5dde\u5927\u5b66\u4f0a\u90fd\u30ad\u30e3\u30f3\u30d1\u30b9.<\/li>\n<li><span class=\"underline\">\u5317\u53e3\u8cb4\u96c4<\/span>\uff1a\u300cPRAXyS\u885b\u661f\u306b\u642d\u8f09\u3059\u308b\u5149\u96fb\u5b50\u8ffd\u8de1\u578b\uff38\u7dda\u504f\u5149\u8a08\u306e\u504f\u5149\u89d2\u518d\u69cb\u6210\u6cd5\u300d,\u5929\u6587\u5b66\u4f1a\u6625\u306e\u5e74\u4f1a,2017\u5e74\uff13\u670815-18\u65e5,\u4e5d\u5dde\u5927\u5b66\u4f0a\u90fd\u30ad\u30e3\u30f3\u30d1\u30b9.<\/li>\n<li>\u4e2d\u5ca1\u7adc\u4e5f\uff1a\u300c\u4f4e\u5149\u5ea6 IIP \u306b\u5206\u985e\u3055\u308c\u308b\u8d85\u65b0\u661f SN 2016bkv\u306e\u65e9\u671f\u6e2c\u5149\u5206\u5149\u89b3\u6e2c\u300d,\u5929\u6587\u5b66\u4f1a\u6625\u306e\u5e74\u4f1a,2017\u5e74\uff13\u670815-18\u65e5,\u4e5d\u5dde\u5927\u5b66\u4f0a\u90fd\u30ad\u30e3\u30f3\u30d1\u30b9.<\/li>\n<li>\u5ddd\u7aef\u7f8e\u7a42\uff1a\u300cIax \u578b\u8d85\u65b0\u661f\u306e\u89b3\u6e2c\u7684\u7279\u5fb4\u3068\u7406\u8ad6\u30e2\u30c7\u30eb\u3068\u306e\u6bd4\u8f03\u300d,\u5929\u6587\u5b66\u4f1a\u6625\u306e\u5e74\u4f1a,2017\u5e74\uff13\u670815-18\u65e5,\u4e5d\u5dde\u5927\u5b66\u4f0a\u90fd\u30ad\u30e3\u30f3\u30d1\u30b9.<\/li>\n<li>\u5927\u6a4b\u793c\u6075\uff1a\u300c\u786c \uff38 \u7dda\u504f\u5149\u691c\u51fa\u5668 PoGOLite \u306e\u8aad\u307f\u51fa\u3057\u56de\u8def\u306e\u6539\u826f(\uff13)\u300d,\u5929\u6587\u5b66\u4f1a\u6625\u306e\u5e74\u4f1a,2017\u5e74\uff13\u670815-18\u65e5,\u4e5d\u5dde\u5927\u5b66\u4f0a\u90fd\u30ad\u30e3\u30f3\u30d1\u30b9.<\/li>\n<li>\u5fd7\u5c90\u5065\u6210\uff1a\u300c\u96fb\u6ce2\u9280\u6cb3 NGC 1275\u306e\uff38\u7dda\u3068\u53ef\u8996\u3067\u306e\u30e2\u30cb\u30bf\u30fc\u89b3\u6e2c\u300d,\u5929\u6587\u5b66\u4f1a\u6625\u306e\u5e74\u4f1a,2017\u5e74\uff13\u670815-18\u65e5,\u4e5d\u5dde\u5927\u5b66\u4f0a\u90fd\u30ad\u30e3\u30f3\u30d1\u30b9.<\/li>\n<li>\u5bae\u5ca1\u656c\u592a\uff1a\u300cSubaru\/HSC \u30b5\u30fc\u30d9\u30a4\u9818\u57df\u306b\u3042\u308b\u91cd\u91cf\u7d1a\u9280\u6cb3\u56e3\u306e\uff38\u7dda\u89b3\u6e2c\u306b\u3088\u308b\u8cea\u91cf\u63a8\u5b9aII\u300d,\u5929\u6587\u5b66\u4f1a\u6625\u306e\u5e74\u4f1a,2017\u5e74\uff13\u670815-18\u65e5,\u4e5d\u5dde\u5927\u5b66\u4f0a\u90fd\u30ad\u30e3\u30f3\u30d1\u30b9.<\/li>\n<li>\u68ee \u88d5\u6a39\uff1a\u300cHONIR\u7528\u65b0\u691c\u51fa\u5668\u8aad\u307f\u51fa\u3057\u30b7\u30b9\u30c6\u30e0\u306e\u30ce\u30a4\u30ba\u6539\u5584\u306b\u5411\u3051\u305f\u7814\u7a76\u300d,\u5929\u6587\u5b66\u4f1a\u6625\u306e\u5e74\u4f1a,2017\u5e74\uff13\u670815-18\u65e5,\u4e5d\u5dde\u5927\u5b66\u4f0a\u90fd\u30ad\u30e3\u30f3\u30d1\u30b9.<\/li>\n<li><span class=\"underline\">\u6df1\u6ca2\u6cf0\u53f8<\/span>\uff1a\uff62\u3072\u3068\u307f\u885b\u661f\u306b\u3088\u308bNGC1275\u306e\uff38\u7dda\u89b3\u6e2c\uff1a\u521d\u306e\u6d3b\u52d5\u9280\u6cb3\u6838Fe-K\u30e9\u30a4\u30f3\u7cbe\u5bc6\u5206\u5149\u300d,\u7269\u7406\u5b66\u4f1a\u6625\u5b63\u5927\u4f1a,2017\u5e74\uff13\u670817-20\u65e5,\u5927\u962a\u5927\u5b66\u8c4a\u4e2d\u30ad\u30e3\u30f3\u30d1\u30b9.<\/li>\n<li><span class=\"underline\">\u6c34\u91ce\u6052\u53f2<\/span>\uff1a\u300c\u30d5\u30a7\u30eb\u30df\u885b\u661f\u306b\u3088\u308bMBM 53-55\u5206\u5b50\u96f2\u30fbPegasusLoop\u9818\u57df\u306b\u304a\u3051\u308b\u661f\u9593\u30ac\u30b9\u3068\u5b87\u5b99\u7dda\u306e\u7814\u7a76\u300d,\u7269\u7406\u5b66\u4f1a\u6625\u5b63\u5927\u4f1a,2017\u5e74\uff13\u670817-20\u65e5,\u5927\u962a\u5927\u5b66\u8c4a\u4e2d\u30ad\u30e3\u30f3\u30d1\u30b9.<\/li>\n<li><span class=\"underline\">\u9ad8\u6a4b\u5f18\u5145<\/span>\uff1a\u300c\u786c\uff38\u7dda\u504f\u5149\u691c\u51fa\u5668PoGOLite\u6c17\u7403\u5b9f\u9a132016\u5e74\u30d5\u30e9\u30a4\u30c8\u300d,\u5927\u6c17\u7403\u30b7\u30f3\u30dd\u30b8\u30a6\u30e0 2016\u5e7411\u6708\uff12\u65e5,\u5b87\u5b99\u79d1\u5b66\u7814\u7a76\u6240.<\/li>\n<li><span class=\"underline\">\u9ad8\u6a4b\u5f18\u5145<\/span>\uff1a\u300c\u786c\uff38\u7dda\u504f\u5149\u691c\u51fa\u5668PoGO+\u6c17\u7403\u5b9f\u9a132016\u5e74\u30d5\u30e9\u30a4\u30c8\u300d,\u5b87\u5b99\u79d1\u5b66\u30b7\u30f3\u30dd\u30b8\u30a6\u30e0,2017\u5e74\uff11\u6708\uff15\u65e5,\u5b87\u5b99\u79d1\u5b66\u7814\u7a76\u6240.<\/li>\n<li>\u5b89\u90e8\u592a\u6674 : \u300c\u5927\u898f\u6a21\u30c7\u30fc\u30bf\u89e3\u6790\u306b\u5411\u3051\u305f\u5149\u5ea6\u66f2\u7dda\u304a\u3088\u3073AGB\u661f\u306eSED\u306e\u5206\u985e\u300d,\u9023\u661f\u7cfb\u30fb\u5909\u5149\u661f\u30fb\u4f4e\u6e29\u5ea6\u661f\u7814\u7a76\u4f1a 2016,2016\u5e7410\u670829\uff5e31\u65e5, \u6176\u5fdc\u5927\u5b66 \u65e5\u5409\u30ad\u30e3\u30f3\u30d1\u30b9, 50\u540d.<\/li>\n<li>\u5ee3\u5730 \u8ac4 : \u300c\u9ad8\u8f1d\u5ea6\u8d64\u8272\u65b0\u661f M31 LRN 2015 \u306e\u7206\u767a\u524d\u5929\u4f53\u306e\u89b3\u6e2c\u7684\u7814\u7a76\u300d, \u9023\u661f\u7cfb\u30fb\u5909\u5149\u661f\u30fb\u4f4e\u6e29\u5ea6\u661f\u7814\u7a76\u4f1a 2016,2016\u5e7410\u670829\uff5e31\u65e5, \u6176\u5fdc\u5927\u5b66 \u65e5\u5409\u30ad\u30e3\u30f3\u30d1\u30b9, 50\u540d.<\/li>\n<li>\u4e2d\u5ca1\u7adc\u4e5f: \u300c\u4f4e\u5149\u5ea6IIP\u306b\u5c5e\u3059\u308b\u8d85\u65b0\u661fSN2016bkv\u306e\u6e2c\u5149\u5206\u5149\u89b3\u6e2c\u306b\u57fa\u3065\u3044\u305f\u89e3\u6790\u300d, \u9023\u661f\u7cfb\u30fb\u5909\u5149\u661f\u30fb\u4f4e\u6e29\u5ea6\u661f\u7814\u7a76\u4f1a 2016,2016\u5e7410\u670829\uff5e31\u65e5, \u6176\u5fdc\u5927\u5b66 \u65e5\u5409\u30ad\u30e3\u30f3\u30d1\u30b9, 50\u540d.<\/li>\n<li>\u5ddd\u7aef\u7f8e\u7a42: \u300c\u7279\u7570\u306aIa\u578b\u8d85\u65b0\u661fSN 2014dt\u306e\u53ef\u8996\u30fb\u8fd1\u8d64\u5916\u7dda\u89b3\u6e2c\u300d, \u9023\u661f\u7cfb\u30fb\u5909\u5149\u661f\u30fb\u4f4e\u6e29\u5ea6\u661f\u7814\u7a76\u4f1a 2016,2016\u5e7410\u670829\uff5e31\u65e5, \u6176\u5fdc\u5927\u5b66\u65e5\u5409\u30ad\u30e3\u30f3\u30d1\u30b9, 50\u540d.<\/li>\n<li>\u6cb3\u539f\u76f4\u8cb4: \u300c\u5178\u578b\u7684\u306a\u53ef\u8996\u5149\u5ea6\u5909\u5316\u3092\u793a\u3057\u305fIb\u578b\u8d85\u65b0\u661fSN2016bau\u306e\u53ef\u8996\u8fd1\u8d64\u5916\u6e2c\u5149\u30fb\u53ef\u8996\u5206\u5149\u89b3\u6e2c\u300d,\u9023\u661f\u7cfb\u30fb\u5909\u5149\u661f\u30fb\u4f4e\u6e29\u5ea6\u661f\u7814\u7a76\u4f1a 2016, 2016\u5e7410\u670829\uff5e31\u65e5, \u6176\u5fdc\u5927\u5b66 \u65e5\u5409\u30ad\u30e3\u30f3\u30d1\u30b9, 50\u540d.<\/li>\n<li><span class=\"underline\">\u5409\u7530\u9053\u5229<\/span>: \u300c\u5e83\u5cf6\u5927\u5b66\u5b87\u5b99\u79d1\u5b66\u30bb\u30f3\u30bf\u30fc\u306e\u6d3b\u52d5\u5831\u544a\u300d,\u5149\u8d64\u5916\u30e6\u30fc\u30b6\u30fc\u30ba\u30df\u30fc\u30c6\u30a3\u30f3\u30b0, 2016\u5e74\uff19\u6708\uff17\uff5e\uff18\u65e5, \u56fd\u7acb\u5929\u6587\u53f0\u4e09\u9df9\u30ad\u30e3\u30f3\u30d1\u30b9, 70\u540d.<\/li>\n<li><span class=\"underline\">\u5ddd\u7aef\u5f18\u6cbb<\/span>: \u300c\u304b\u306a\u305f\u671b\u9060\u93e1\u30fb\u89b3\u6e2c\u88c5\u7f6e\u4f7f\u7528\u72b6\u6cc1\u300d,\u5149\u8d64\u5916\u30e6\u30fc\u30b6\u30fc\u30ba\u30df\u30fc\u30c6\u30a3\u30f3\u30b0, 2016\u5e74\uff19\u6708\uff17\uff5e\uff18\u65e5, \u56fd\u7acb\u5929\u6587\u53f0\u4e09\u9df9\u30ad\u30e3\u30f3\u30d1\u30b9, 70\u540d.<\/li>\n<li><span class=\"underline\">\u690d\u6751 \u8aa0<\/span>: \u300c\u88c5\u7f6e\u958b\u767a\u30fb\u30b9\u30c6\u30fc\u30bf\u30b9\u300d, \u5149\u8d64\u5916\u30e6\u30fc\u30b6\u30fc\u30ba\u30df\u30fc\u30c6\u30a3\u30f3\u30b0,2016\u5e74\uff19\u6708\uff17\uff5e\uff18\u65e5, \u56fd\u7acb\u5929\u6587\u53f0\u4e09\u9df9\u30ad\u30e3\u30f3\u30d1\u30b9, 70\u540d.<\/li>\n<li><span class=\"underline\">\u5ddd\u7aef\u5f18\u6cbb<\/span>: \u300c\u304b\u306a\u305f\u671b\u9060\u93e1\u30fb\u89b3\u6e2c\u88c5\u7f6e\u4f7f\u7528\u72b6\u6cc1\u300d,\u5149\u8d64\u5916\u30e6\u30fc\u30b6\u30fc\u30ba\u30df\u30fc\u30c6\u30a3\u30f3\u30b0, 2016\u5e74\uff19\u6708\uff17\uff5e\uff18\u65e5, \u56fd\u7acb\u5929\u6587\u53f0\u4e09\u9df9\u30ad\u30e3\u30f3\u30d1\u30b9, 70\u540d.<\/li>\n<li>\u4e2d\u5ca1\u7adc\u4e5f: \u300cIIP\u578b\u8d85\u65b0\u661fSN2016X\u306e\u65e9\u671f\u7d2b\u5916\u30fc\u8fd1\u8d64\u5916\u89b3\u6e2c\u306b\u57fa\u3065\u3044\u305f\u89e3\u6790\u300d,\u5149\u8d64\u5916\u30e6\u30fc\u30b6\u30fc\u30ba\u30df\u30fc\u30c6\u30a3\u30f3\u30b0,2016\u5e74\uff19\u6708\uff17\uff5e\uff18\u65e5, \u56fd\u7acb\u5929\u6587\u53f0\u4e09\u9df9\u30ad\u30e3\u30f3\u30d1\u30b9, 70\u540d.<\/li>\n<li>\u68ee \u88d5\u6a39: \u300c\u304b\u306a\u305f\u671b\u9060\u93e1HONIR\u7528\u65b0\u691c\u51fa\u5668\u8aad\u307f\u51fa\u3057\u30b7\u30b9\u30c6\u30e0\u306e\u30ce\u30a4\u30ba\u6539\u5584\u306b\u5411\u3051\u305f\u7814\u7a76\u300d, \u5149\u8d64\u5916\u30e6\u30fc\u30b6\u30fc\u30ba\u30df\u30fc\u30c6\u30a3\u30f3\u30b0,2016\u5e74\uff19\u6708\uff17\uff5e\uff18\u65e5, \u7acb\u5929\u6587\u53f0\u4e09\u9df9\u30ad\u30e3\u30f3\u30d1\u30b9, 70\u540d.<\/li>\n<li>\u5ddd\u7aef\u7f8e\u7a42: \u300c\u7279\u7570\u306aIa\u578b\u8d85\u65b0\u661fSN 2014dt\u306e\u53ef\u8996\u8fd1\u8d64\u5916\u306b\u304a\u3051\u308b\u4e2d\u671f\u30fb\u5f8c\u671f\u89b3\u6e2c\u300d, \u5149\u8d64\u5916\u30e6\u30fc\u30b6\u30fc\u30ba\u30df\u30fc\u30c6\u30a3\u30f3\u30b0,2016\u5e74\uff19\u6708\uff17\uff5e\uff18\u65e5, \u56fd\u7acb\u5929\u6587\u53f0\u4e09\u9df9\u30ad\u30e3\u30f3\u30d1\u30b9, 70\u540d.<\/li>\n<li>\u6cb3\u539f\u76f4\u8cb4: \u300c\u5149\u5ea6\u9032\u5316\u306e\u9045\u3044Ib\u578b\u8d85\u65b0\u661fSN 2016bau\u306e\u53ef\u8996\u8fd1\u8d64\u5916\u89b3\u6e2c\u300d, \u5149\u8d64\u5916\u30e6\u30fc\u30b6\u30fc\u30ba\u30df\u30fc\u30c6\u30a3\u30f3\u30b0,2016\u5e74\uff19\u6708\uff17\uff5e\uff18\u65e5, \u56fd\u7acb\u5929\u6587\u53f0\u4e09\u9df9\u30ad\u30e3\u30f3\u30d1\u30b9, 70\u540d.<\/li>\n<li><span class=\"underline\">\u690d\u6751 \u8aa0<\/span>: \u300c\u5e83\u5cf6\u5927\u5b66\u306e\u53d6\u308a\u7d44\u307f\u3068\u6210\u679c\u300d,\u5149\u8d64\u5916\u7dda\u5927\u5b66\u9593\u9023\u643a\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d7, 2016\u5e7411\u670821\uff5e22\u65e5, \u4eac\u90fd\u5927\u5b66, 60\u540d.<\/li>\n<li><span class=\"underline\">\u89b3\u5c71\u6b63\u898b<\/span>: \u300c\u5149\u8d64\u5916\u7dda\u5927\u5b66\u9023\u643a\u306e\u53d6\u308a\u7d44\u307f\u306b\u3064\u3044\u3066\u306e\u30b3\u30e1\u30f3\u30c8\u300d,\u5149\u8d64\u5916\u7dda\u5927\u5b66\u9593\u9023\u643a\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d7, 2016\u5e7411\u670821\uff5e22\u65e5, \u4eac\u90fd\u5927\u5b66, 60\u540d.<\/li>\n<li><span class=\"underline\">\u5ddd\u7aef\u5f18\u6cbb<\/span>: \u300cGRB\u521d\u671f\u53ef\u8996\u6b8b\u5149\u306e\u504f\u5149\u89b3\u6e2c\u3053\u306e\uff16\u5e74\u300d,\u5149\u8d64\u5916\u7dda\u5927\u5b66\u9593\u9023\u643a\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d7, 2016\u5e7411\u670821\uff5e22\u65e5, \u4eac\u90fd\u5927\u5b66, 60\u540d.<\/li>\n<li><span class=\"underline\">\u7530\u4e2d\u5eb7\u4e4b<\/span>:\u300c\u5927\u5b66\u9593\u9023\u643a\u306b\u3088\u308b\u30cb\u30e5\u30fc\u30c8\u30ea\u30ce\u30a4\u30d9\u30f3\u30c8\u30d5\u30a9\u30ed\u30fc\u30a2\u30c3\u30d7\u89b3\u6e2c\u306e\u63d0\u6848\u300d, \u5149\u8d64\u5916\u7dda\u5927\u5b66\u9593\u9023\u643a\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d7,2016\u5e7411\u670821\uff5e22\u65e5,\u4eac\u90fd\u5927\u5b66, 60\u540d.<\/li>\n<li>\u4e2d\u5ca1\u7adc\u4e5f: \u300c\u4f4e\u5149\u5ea6IIP\u306b\u5c5e\u3059\u308b\u8d85\u65b0\u661fSN2016bkv\u306e\u65e9\u671f\u6e2c\u5149\u5206\u5149\u89b3\u6e2c\u300d, \u5149\u8d64\u5916\u7dda\u5927\u5b66\u9593\u9023\u643a\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d7,2016\u5e7411\u670821\uff5e22\u65e5, \u4eac\u90fd\u5927\u5b66,60\u540d.<\/li>\n<li>\u68ee \u88d5\u6a39: \u300c\u5e83\u5cf6\u5927\u5b66\u304b\u306a\u305f\u671b\u9060\u93e1\u5468\u8fba\u306e\u88c5\u7f6e\u958b\u767a\u306e\u73fe\u72b6\u300d, \u5149\u8d64\u5916\u7dda\u5927\u5b66\u9593\u9023\u643a\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d7, 2016\u5e7411\u670821\uff5e22\u65e5,\u4eac\u90fd\u5927\u5b66, 60\u540d.<\/li>\n<li>\u5ddd\u7aef\u7f8e\u7a42: \u300c\u7279\u7570\u306aIa\u578b\u8d85\u65b0\u661fSN 2014dt \u306e\u53ef\u8996\u30fb\u8fd1\u8d64\u5916\u306b\u304a\u3051\u308b\u4e2d\u671f\u30fb\u5f8c\u671f\u89b3\u6e2c\u300d, \u5149\u8d64\u5916\u7dda\u5927\u5b66\u9593\u9023\u643a\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d7,2016\u5e7411\u670821\uff5e22\u65e5,\u4eac\u90fd\u5927\u5b66, 60\u540d.<\/li>\n<li>\u6cb3\u539f\u76f4\u8cb4: \u300c\u5178\u578b\u7684\u306a\u53ef\u8996\u5149\u5ea6\u5909\u5316\u3092\u793a\u3057\u305fIb\u578b\u8d85\u65b0\u661fSN2016bau\u306e\u53ef\u8996\u8fd1\u8d64\u5916\u6e2c\u5149\u30fb\u53ef\u8996\u5206\u5149\u89b3\u6e2c\u300d,\u5149\u8d64\u5916\u7dda\u5927\u5b66\u9593\u9023\u643a\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d7, 2016\u5e7411\u670821\uff5e22\u65e5, \u4eac\u90fd\u5927\u5b66, 60\u540d.<\/li>\n<li>\u4e2d\u5ca1\u7adc\u4e5f: \u300cLow-Luminosity IIP SN2016bkv + IIL\u300d, \u8d85\u65b0\u661f\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d72016,2016\u5e7412\u670814\uff5e16\u65e5, \u30e1\u30fc\u30d7\u30eb\u6709\u99ac\uff08\u795e\u6238\u5e02\uff09, 10\u540d.<\/li>\n<li>\u5ddd\u7aef\u7f8e\u7a42: \u300cSN 2014dt\u3068Iax\u578b\u8d85\u65b0\u661f\u300d, \u8d85\u65b0\u661f\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d72016, 2016\u5e7412\u670814\uff5e16\u65e5,\u30e1\u30fc\u30d7\u30eb\u6709\u99ac\uff08\u795e\u6238\u5e02\uff09, 10\u540d.<\/li>\n<li>\u6cb3\u539f\u76f4\u8cb4: \u300cType Ibc SN\u300d, \u8d85\u65b0\u661f\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d72016, 2016\u5e7412\u670814\uff5e16\u65e5, \u30e1\u30fc\u30d7\u30eb\u6709\u99ac\uff08\u795e\u6238\u5e02\uff09,10\u540d.<\/li>\n<li>\u4e2d\u5ca1\u7adc\u4e5f: \u300c\u4f4e\u5149\u5ea6IIP\u306b\u5c5e\u3059\u308b\u8d85\u65b0\u661fSN2016bkv\u306e\u6e2c\u5149\u5206\u5149\u89b3\u6e2c\u300d, \u5929\u4f53\u30b9\u30da\u30af\u30c8\u30eb\u7814\u7a76\u4f1a, 2017\u5e74\uff13\u6708\uff14\uff5e\uff15\u65e5,\u4ed9\u53f0\u5e02\u5929\u6587\u53f0, 50\u540d.<\/li>\n<li>\u5ddd\u7aef\u7f8e\u7a42: \u300c\u7279\u7570\u306aIa\u578b\u8d85\u65b0\u661fSN 2014dt\u306e\u9577\u671f\u306b\u4e98\u308b\u53ef\u8996\u8fd1\u8d64\u5916\u89b3(\u2161)\u300d,\u5929\u4f53\u30b9\u30da\u30af\u30c8\u30eb\u7814\u7a76\u4f1a, 2017\u5e74\uff13\u6708\uff14\uff5e\uff15\u65e5,\u4ed9\u53f0\u5e02\u5929\u6587\u53f0, 50\u540d.<\/li>\n<li>\u68ee \u88d5\u6a39: \u300c\u5e83\u5cf6\u5927\u5b66\u304b\u306a\u305f\u671b\u9060\u93e1\u5468\u8fba\u306e\u88c5\u7f6e\u958b\u767a\u306e\u73fe\u72b6\u300d, \u53ef\u8996\u8d64\u5916\u7dda\u89b3\u6e2c\u88c5\u7f6e\u6280\u8853\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d7, 2016\u5e7411\u670824\uff5e25\u65e5,\u56fd\u7acb\u5929\u6587\u53f0\u4e09\u9df9\u30ad\u30e3\u30f3\u30d1\u30b9,60\u540d.<\/li>\n<li>\u6cb3\u539f\u76f4\u8cb4: \u300cIIb\/Ib\u9077\u79fb\u8d85\u65b0\u661fSN 2016bau\u306e\u53ef\u8996\u8fd1\u8d64\u5916\u89b3\u6e2c\u300d, \u5929\u4f53\u30b9\u30da\u30af\u30c8\u30eb\u7814\u7a76\u4f1a, 2017\u5e74\uff13\u6708\uff14\uff5e\uff15\u65e5,\u4ed9\u53f0\u5e02\u5929\u6587\u53f0, 50\u540d.<\/li>\n<li>\u68ee \u88d5\u6a39: \u300c\u5e83\u5cf6\u5927\u5b66\u304b\u306a\u305f\u671b\u9060\u93e1\u5468\u8fba\u306e\u88c5\u7f6e\u958b\u767a\u306e\u73fe\u72b6\u300d, \u53ef\u8996\u8d64\u5916\u7dda\u89b3\u6e2c\u88c5\u7f6e\u6280\u8853\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d7, 2016\u5e7411\u670824\uff5e25\u65e5,\u56fd\u7acb\u5929\u6587\u53f0\u4e09\u9df9\u30ad\u30e3\u30f3\u30d1\u30b9, 60\u540d.<\/li>\n<li>\u68ee \u88d5\u6a39: \u300c\u5e83\u5cf6\u5927\u5b66\u65b0\u8aad\u307f\u51fa\u3057\u30b7\u30b9\u30c6\u30e0\u306e\u30ce\u30a4\u30ba\u8abf\u67fb\u3068\u65b0InGaAs\u691c\u51fa\u5668\u306e\u6027\u80fd\u8a55\u4fa1\u300d, \u30bf\u30a4\u30e0\u30c9\u30e1\u30a4\u30f3\u5929\u6587\u5b66\u7814\u7a76\u4f1a,2017\u5e74\uff12\u670820\uff5e22\u65e5, 60\u540d.<\/li>\n<li>\u5ddd\u7aef\u7f8e\u7a42: \u300cIa\u578b\u8d85\u65b0\u661f\u306e\u89b3\u6e2c\u7684\u7814\u7a76\u3068\u753b\u50cf\u30c7\u30fc\u30bf\u89e3\u6790\u300d, \u7b2c\uff11\u56de\u8ab2\u984c\u63d0\u6848\u578b\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d7\u300c\u30d3\u30c3\u30b0\u30c7\u30fc\u30bf\u306e\u5229\u6d3b\u7528\u306b\u3064\u3044\u3066\u8003\u3048\u308b\u300d,2016\u5e74\uff16\u6708\uff12\u65e5,\u770c\u7acb\u5e83\u5cf6\u5927\u5b66, 80\u540d.<\/li>\n<li>\u5ddd\u7aef\u7f8e\u7a42: \u300c\u7279\u7570\u306aIa\u578b\u8d85\u65b0\u661fSN 2014dt\u306e\u53ef\u8996\u30fb\u8fd1\u8d64\u5916\u7dda\u89b3\u6e2c\u300d,2016\u5e74\u5ea6\u5149\u8d64\u5929\u9023\u30b7\u30f3\u30dd\u30b8\u30a6\u30e0 \u5171\u540c\u5229\u7528\u3068\u5927\u898f\u6a21\u89b3\u6e2c\u306e\u8abf\u548c, 2016\u5e74\uff19\u670826\uff5e28\u65e5, \u56fd\u7acb\u5929\u6587\u53f0\u4e09\u9df9\u30ad\u30e3\u30f3\u30d1\u30b9, 90\u540d.<\/li>\n<li><span class=\"underline\">\u5ddd\u7aef\u5f18\u6cbb<\/span>: \u300c\u53ef\u8996\u8d64\u5916\u30fb\u30b5\u30d6\u30df\u30ea\u504f\u5149\u89b3\u6e2c\u3068\u8f03\u6b63\u6cd5\u306b\u95a2\u3059\u308b\u8003\u5bdf\u300d,DTA\u30b7\u30f3\u30dd\u30b8\u30a6\u30e0\uff1a\u661f\u5f62\u6210\u3092\u8ef8\u306b\u4fef\u77b0\u3059\u308b\u78c1\u5834\u306e\u5f79\u5272\u3068\u305d\u306e\u89b3\u6e2c\u7684\u691c\u8a3c, 2016\u5e7411\u670824\uff5e25\u65e5, \u56fd\u7acb\u5929\u6587\u53f0\u30fb\u4e09\u9df9, 40\u540d.<\/li>\n<li><span class=\"underline\">\u5ddd\u7aef\u5f18\u6cbb<\/span>: \u300c\u53ef\u8996\u504f\u5149\u30b5\u30fc\u30d9\u30a4SGMAP\u3068\u30bf\u30a4\u30e0\u30c9\u30e1\u30a4\u30f3\u5929\u6587\u5b66\u300d,\u6728\u66fd\u5e83\u8996\u91ce\u30b5\u30fc\u30d9\u30a4\u3068\u4eac\u90fd3.8m\u5373\u6642\u5206\u5149\u306b\u3088\u308b\u30bf\u30a4\u30e0\u30c9\u30e1\u30a4\u30f3\u5929\u6587\u5b66\u306e\u63a8\u9032, 2017\u5e74\uff12\u670820\uff5e22\u65e5, \u4eac\u90fd\u5927\u5b66, 60\u540d.<\/li>\n<li><span class=\"underline\">\u7530\u4e2d\u5eb7\u4e4b<\/span>:\u300cIceCube\u9ad8\u30a8\u30cd\u30eb\u30ae\u30fc\u30cb\u30e5\u30fc\u30c8\u30ea\u30ce\u4e8b\u8c61\u306e\u53ef\u8996\u8fd1\u8d64\u5916\u7dda\u30d5\u30a9\u30ed\u30fc\u30a2\u30c3\u30d7\u89b3\u6e2c\u300d,\u6728\u66fd\u5e83\u8996\u91ce\u30b5\u30fc\u30d9\u30a4\u3068\u4eac\u90fd3.8m\u5373\u6642\u5206\u5149\u306b\u3088\u308b\u30bf\u30a4\u30e0\u30c9\u30e1\u30a4\u30f3\u5929\u6587\u5b66\u306e\u63a8\u9032, 2017\u5e74\uff12\u670820\uff5e22\u65e5, \u4eac\u90fd\u5927\u5b66, 60\u540d.<\/li>\n<li><span class=\"underline\">\u7530\u4e2d\u5eb7\u4e4b<\/span>: \u300cIceCubeneutrino\u306e\u96fb\u78c1\u6ce2ToO\u89b3\u6e2c\u306e\u73fe\u72b6\u3068\u4eca\u5f8c\u300d, \u8328\u57ce\u5927\u5b66\u91cd\u70b9\u7814\u7a76 \u7814\u7a76\u4f1a\uff1a\u300c\u7a81\u767a\u30fb\u5909\u52d5\u5929\u4f53\u306e\u591a\u6ce2\u9577\u9023\u643a\u89b3\u6e2c\u300d,2016\u5e74\uff13\u6708\uff16\uff5e\uff17\u65e5, \u8328\u57ce\u5927\u5b66, 40\u4eba.<\/li>\n<li><span class=\"underline\">\u690d\u6751 \u8aa0<\/span> : \u300cIa\u578b\u8d85\u65b0\u661f\u306e\u6975\u5927\u7b49\u7d1a\u306e\u5909\u6570\u9078\u629e\u300d,\u9023\u661f\u7cfb\u30fb\u5909\u5149\u661f\u30fb\u4f4e\u6e29\u5ea6\u661f\u7814\u7a76\u4f1a 2016, 2016\u5e7410\u670829\uff5e31\u65e5, \u6176\u5fdc\u5927\u5b66 \u65e5\u5409\u30ad\u30e3\u30f3\u30d1\u30b9,50\u540d.<\/li>\n<li><span class=\"underline\">\u5c71\u672c\u4e00\u535a<\/span>\uff1a\u300c\u30a6\u30f3\u30eb\u30fc\u653e\u5c04\u306f\u5b58\u5728\u3059\u308b\u306e\u304b?\u300d,\u71b1\u5834\u306e\u91cf\u5b50\u8ad6,\u7406\u5316\u5b66\u7814\u7a76\u6240, \u5e73\u621028\u5e74\uff18\u670824\u65e5, \u4e00\u822c\uff0885\u540d\uff09.<\/li>\n<li><span class=\"underline\">\u5ca1\u90e8\u4fe1\u5e83<\/span>\uff1a&ldquo;LoCuSS &amp; NECSUS : ClusterWeak-lensing Studies&rdquo; \u7b2c\uff15\u56de\u89b3\u6e2c\u7684\u5b87\u5b99\u8ad6\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d7 Nov, 24-26, 2016,\u5e83\u5cf6\u5927\u5b66 \u4e2d\u592e\u56f3\u66f8\u9928 \u30e9\u30a4\u30d6\u30e9\u30ea\u30fc\u30db\u30fc\u30eb.<\/li>\n<li><span class=\"underline\">\u5c0f\u5d8c\u5eb7\u53f2<\/span>\uff1a\u300cComment on primordial magneticfield\u300d\u7b2c\uff15\u56de\u89b3\u6e2c\u7684\u5b87\u5b99\u8ad6\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d7 \uff08\u5e73\u621028\u5e7411\u670824-26\u65e5,\u5e83\u5cf6\u5927\u5b66\uff09.<\/li>\n<li><span class=\"underline\">\u5c0f\u5d8c\u5eb7\u53f2<\/span>\uff1a\u300c\u30de\u30b0\u30cd\u30bf\u30fc\u306e\u5de8\u5927\u30d5\u30ec\u30a2\u6642\u306e\u91cd\u529b\u6ce2\u653e\u51fa\u300d\u65e5\u672c\u5929\u6587\u5b66\u4f1a\u79cb\u5b63\u5e74\u4f1a\uff08\u5e73\u621028\u5e74\uff19\u670814-16\u65e5,\u611b\u5a9b\u5927\u5b66\uff09.<\/li>\n<li><span class=\"underline\">\u5ca1\u90e8\u4fe1\u5e83<\/span>\uff1a&ldquo;LoCuSS: Weak-lensing masscalibration of galaxy clusters&rdquo; \u65e5\u672c\u5929\u6587\u5b66\u4f1a\u5e73\u621028\u5e74 \u79cb\u5b63\u5e74\u4f1a, Sep 14-16 2016,\u611b\u5a9b\u5927\u5b66.<\/li>\n<li>\u690d\u91ce\u826f\u7d00,<span class=\"underline\">\u5c71\u672c\u4e00\u535a<\/span>\uff1a\u300c\u30a2\u30eb\u30d5\u30a1\u30a2\u30c8\u30e9\u30af\u30bf\u30fc\u30a4\u30f3\u30d5\u30ec\u30fc\u30b7\u30e7\u30f3\u3068\u518d\u52a0\u71b1\u671f\u306e\u5236\u9650\u300d\u65e5\u672c\u7269\u7406\u5b66\u4f1a2016\u79cb\u671f\u5927\u4f1a,\u5e73\u621028\u5e74\uff19\u670821\u65e5.<\/li>\n<li>\u5357 \u5cb3,<span class=\"underline\">\u5c71\u672c\u4e00\u535a<\/span>,\u65e5\u5f71\u5343\u79cb\uff1a\u7b2c\uff15\u56de\u89b3\u6e2c\u7684\u5b87\u5b99\u8ad6\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d7,\u5e73\u621028\u5e7411\u670825\u65e5.<\/li>\n<li><span class=\"underline\">\u5c0f\u5d8c\u5eb7\u53f2<\/span>\uff1a\u300c\u30de\u30b0\u30cd\u30bf\u30fc\u78c1\u6c17\u570f\u3067\u306e\u30d5\u30ec\u30a2\u524d\u306e\u30a8\u30cd\u30eb\u30ae\u30fc\u84c4\u7a4d\u300d\u65e5\u672c\u5929\u6587\u5b66\u4f1a\u6625\u5b63\u5e74\u4f1a\uff08\u5e73\u621029\u5e74\uff13\u670815\u65e5-18\u65e5,\u4e5d\u5dde\u5927\u5b66\uff09.<\/li>\n<li><span class=\"underline\">\u5fd7\u57a3\u8ce2\u592a<\/span>\uff1a\u300cLHC\u52a0\u901f\u5668\u306b\u304a\u3051\u308b\u9ad8\u6e29QCD\u7269\u8cea\u306e\u5b9f\u9a13\u7814\u7a76\u300d,\u65e5\u672c\u7269\u7406\u5b66\u4f1a\u30b7\u30f3\u30dd\u30b8\u30a6\u30e0\u300c\u539f\u5b50\u6838\u30b3\u30e9\u30a4\u30c0\u30fc\u306b\u304a\u3051\u308bQCD\u7269\u7406- \u30af\u30a9\u30fc\u30af\u30fb\u30b0\u30eb\u30fc\u30aa\u30f3\u30fb\u30d7\u30e9\u30ba\u30de\u306e\u767a\u898b\u3092\u4e2d\u5fc3\u306b -\u300d\uff08\u5927\u962a\u5927\u5b66,2017\u5e74\uff13\u670817\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\u30af\u30a9\u30fc\u30af\u306e\u76f8\u95a2\u3068\u30af\u30e9\u30b9\u30bf\u30fc\u300d,\u7814\u7a76\u4f1a\u300c\u30af\u30e9\u30b9\u30bf\u30fc\u304c\u3064\u306a\u3050\u30af\u30a9\u30fc\u30af,\u30cf\u30c9\u30ed\u30f3,\u539f\u5b50\u6838\u305d\u3057\u3066\u539f\u5b50\u300d\uff08\u5927\u962a\u5927\u5b66,2017\u5e74\uff13\u670816\u65e5\uff09.<\/li>\n<li><span class=\"underline\">\u4e09\u597d\u9686\u535a<\/span>,\u7c11\u5cf6 \u656c,\u677e\u672c\u6d0b\u4ecb\uff1a\u300c\u78c1\u6c17\u6d41\u4f53\u529b\u5b66\u65b9\u7a0b\u5f0f\u306b\u5bfe\u3059\u308b\u9ad8\u6b21\u7cbe\u5ea6\u91cd\u307f\u4ed8\u304d\u30b3\u30f3\u30d1\u30af\u30c8\u5dee\u5206\u6cd5\u300d\u65e5\u672c\u5730\u7403\u60d1\u661f\u79d1\u5b66\u9023\u54082016\u5e74\u5927\u4f1a (\u5e55\u5f35\u30e1\u30c3\u30bb,2016\u5e74\uff15\u670822\u65e5-26\u65e5).<\/li>\n<li>\u7c11\u5cf6 \u656c,<span class=\"underline\">\u4e09\u597d\u9686\u535a<\/span>,\u4eca\u7530\u664b\u4eae\uff1a\u300cImpact of DiffusionProcesses on Magnetic Reconnection\u300d\u65e5\u672c\u5730\u7403\u60d1\u661f\u79d1\u5b66\u9023\u54082016\u5e74\u5927\u4f1a (\u5e55\u5f35\u30e1\u30c3\u30bb,2016\u5e74\uff15\u670822\u65e5-26\u65e5).<\/li>\n<li>\u67f4\u5c71\u62d3\u4e5f,\u8349\u91ce\u5b8c\u4e5f,<span class=\"underline\">\u4e09\u597d\u9686\u535a<\/span>,\u4e2d\u574a\u5b5d\u53f8,GrigoryVekstein\uff1a\u300cFast Magnetic Reconnection Supported by SporadicSmall-scale Petschek-type Shocks\u300d\u65e5\u672c\u5730\u7403\u60d1\u661f\u79d1\u5b66\u9023\u54082016\u5e74\u5927\u4f1a (\u5e55\u5f35\u30e1\u30c3\u30bb,2016\u5e74\uff15\u670822\u65e5-26\u65e5).<\/li>\n<li><span class=\"underline\">\u4e09\u597d\u9686\u535a<\/span>\uff1a\u300c\u5b8c\u5168\u4e8c\u6d41\u4f53\u65b9\u7a0b\u5f0f\u306b\u5bfe\u3059\u308b\u9ad8\u6b21\u7cbe\u5ea6\u6570\u5024\u89e3\u6cd5\u306e\u57fa\u790e\u7684\u7814\u7a76\u300d\u30d7\u30e9\u30ba\u30de\u30b7\u30df\u30e5\u30ec\u30fc\u30bf\u30b7\u30f3\u30dd\u30b8\u30a6\u30e02016 (\u6838\u878d\u5408\u79d1\u5b66\u7814\u7a76\u6240,2015\u5e74\uff19\u6708\uff17\u65e5-\uff18\u65e5).<\/li>\n<li>\u67f4\u5c71\u62d3\u4e5f,\u8349\u91ce\u5b8c\u4e5f,<span class=\"underline\">\u4e09\u597d\u9686\u535a<\/span>,\u4e2d\u574a\u5b5d\u53f8,GrigoryVekstein\uff1a\u300c\u30d7\u30e9\u30ba\u30e2\u30a4\u30c9\u9ad8\u901f\u30ea\u30b3\u30cd\u30af\u30b7\u30e7\u30f3\u306b\u304a\u3051\u308b\u52d5\u7684\u307a\u30c1\u30a7\u30c3\u30af\u904e\u7a0b\u306e\u5f79\u5272\u300d\u65e5\u672c\u5929\u6587\u5b66\u4f1a2016\u5e74\u79cb\u5b63\u5e74\u4f1a (\u611b\u5a9b\u5927\u5b66,2016\u5e74\uff19\u670814\u65e5-16\u65e5).<\/li>\n<li><span class=\"underline\">\u4e09\u597d\u9686\u535a<\/span>,\u8349\u91ce\u5b8c\u4e5f,\u4e95\u4e0a \u8aed\uff1a\u300c\u975e\u30d5\u30a9\u30fc\u30b9\u30d5\u30ea\u30fc\u592a\u967d\u5927\u6c17\u78c1\u5834\u30e2\u30c7\u30eb\u306b\u5bfe\u3059\u308b\u65b0\u3057\u3044\u78c1\u6c17\u6d41\u4f53\u529b\u5b66\u7684\u7de9\u548c\u6cd5\u300d\u65e5\u672c\u5929\u6587\u5b66\u4f1a2017\u5e74\u6625\u5b63\u5e74\u4f1a (\u4e5d\u5dde\u5927\u5b66,2017\u5e74\uff13\u670815\u65e5-18\u65e5).<\/li>\n<li>\u67f4\u5c71\u62d3\u4e5f,\u8349\u91ce\u5b8c\u4e5f,<span class=\"underline\">\u4e09\u597d\u9686\u535a<\/span>,GrigoryVekstein\uff1a\u300c\uff13\u6b21\u5143\u30ea\u30b3\u30cd\u30af\u30b7\u30e7\u30f3\u9818\u57df\u306b\u304a\u3051\u308b\u30d7\u30e9\u30ba\u30e2\u30a4\u30c9\u306e\u81ea\u767a\u7684\u69cb\u9020\u5f62\u6210\u300d\u65e5\u672c\u5929\u6587\u5b66\u4f1a2017\u5e74\u6625\u5b63\u5e74\u4f1a (\u4e5d\u5dde\u5927\u5b66,2017\u5e74\uff13\u670815\u65e5-18\u65e5).<\/li>\n<li><span class=\"underline\">Takuya Morozumi<\/span>, &ldquo;Flavor violationand New Physics in Rare decays&rdquo;, Mini-Workshop in Osaka 2016 on Quarks,Leptons and Family Gauge Bosons, 26<sup>th<\/sup> Dec.2016, Osaka Univ.<\/li>\n<li><span class=\"underline\">\u77f3\u5ddd\u5065\u4e00<\/span>, \u91d1\u68ee\u9038\u4f5c:\u300c\u683c\u5b50QCD\u306b\u304a\u3051\u308b\u8efd\u3044\u30e2\u30fc\u30c9\u3092\u53d6\u308a\u9664\u3044\u305f\u524d\u51e6\u7406\u4ed8\u304d\u30af\u30a9\u30fc\u30af\u30bd\u30eb\u30d0\u30fc\u306e\u958b\u767a\u300d, \u65e5\u672c\u7269\u7406\u5b66\u4f1a 2016\u5e74\u79cb\u5b63\u5927\u4f1a (\uff19\u670822\u65e5,\u5bae\u5d0e\u5927\u5b66 \u6728\u82b1\u30ad\u30e3\u30f3\u30d1\u30b9).<\/li>\n<li><span class=\"underline\">\u77f3\u5ddd\u5065\u4e00<\/span>,\u6751\u4e0a\u7950\u5b50\uff1a\u300c\u683c\u5b50QCD\u306b\u304a\u3051\u308b\u30e1\u30d3\u30a6\u30b9\u30c9\u30e1\u30a4\u30f3\u30a6\u30a9\u30fc\u30eb\u3092\u7528\u3044\u305fQCD\u30e9\u30e0\u30c0\u30d1\u30e9\u30e1\u30fc\u30bf\u306e\u8a08\u7b97\u300d,\u65e5\u672c\u7269\u7406\u5b66\u4f1a\u7b2c72\u56de\u5e74\u6b21\u5927\u4f1a\uff082017\u5e74\uff09(\uff13\u670819\u65e5, \u5927\u962a\u5927\u5b66\u8c4a\u4e2d\u30ad\u30e3\u30f3\u30d1\u30b9).<\/li>\n<li><span class=\"underline\">Takuya Morozumi<\/span>, &ldquo;Rare B decays andNew Physics&rdquo;, HEP Matsue workshop 2017, 25th March 2017, ShimaneUniversity.<\/li>\n<li><span class=\"underline\">\u4e21\u89d2\u5353\u4e5f<\/span>, Apriadi Salim Adam, \u9577\u5c3e\u6842\u5b50,\u9ad8\u7530\u6d69\u884c: \u300c\u81a8\u5f35\u5b87\u5b99\u4e0b\u306b\u304a\u3051\u308b\u7c92\u5b50\u6570\u306e\u6642\u9593\u767a\u5c55\u306e\u30e2\u30c7\u30eb\u306e\u7814\u7a76\u300d\u65e5\u672c\u7269\u7406\u5b66\u4f1a 2016\u5e74\u79cb\u5b63\u5927\u4f1a(\uff19\u670823\u65e5, \u5bae\u5d0e\u5927\u5b66\u6728\u82b1\u30ad\u30e3\u30f3\u30d1\u30b9),.<\/li>\n<li>\u6728\u6751\u5927\u81ea(\u767b\u58c7\u8005), \u6885\u679d\u5b8f\u4e4b, <span class=\"underline\">\u4e21\u89d2\u5353\u4e5f<\/span>\uff1a\u300c\u56fa\u6709\u30d1\u30ea\u30c6\u30a3\u306e\u7834\u308c\u3068\u30a2\u30a4\u30bd\u30b9\u30d4\u30f3\u306e\u7834\u308c\u3092\u8003\u616e\u3057\u305f\u03c4\u2192\u03b7\u03c0\u03c0\u03bd\u5d29\u58ca\u306e\u7814\u7a76\u300d,\u65e5\u672c\u7269\u7406\u5b66\u4f1a2016\u5e74\u79cb\u5b63\u5927\u4f1a(\uff19\u670823\u65e5, \u5bae\u5d0e\u5927\u5b66 \u6728\u82b1\u30ad\u30e3\u30f3\u30d1\u30b9).<\/li>\n<li><span class=\"underline\">\u4e21\u89d2\u5353\u4e5f<\/span>, Apriadi Salim Adam, \u9577\u5c3e\u6842\u5b50,\u9ad8\u7530\u6d69\u884c\uff1a &ldquo;The creation of the particle number asymmetry in theuniverse of arbitrary time dependent scale factor usingperturbation method&rdquo;, \u65e5\u672c\u7269\u7406\u5b66\u4f1a\u7b2c72\u56de\u5e74\u6b21\u5927\u4f1a, \u8c4a\u4e2d\u5e022017\u5e74\uff13\u6708.<\/li>\n<li>\u9ad8\u6a4b\u96bc\u4e5f,<span class=\"underline\">\u4e21\u89d2\u5353\u4e5f<\/span>,\u6e05\u6c34\u52c7\u4ecb,\u6885\u679d\u5b8f\u4e4b:\u300c\u30af\u30a9\u30fc\u30af\u30b7\u30fc\u30bd\u30fc\u6a21\u578b\u306e\u4f4e\u30a8\u30cd\u30eb\u30ae\u30fc\u6709\u52b9\u7406\u8ad6\u3092\u7528\u3044\u305f\u73fe\u8c61\u8ad6\u300d,\u702c\u6238\u5185\u30b5\u30de\u30fc\u30a4\u30f3\u30b9\u30c6\u30a3\u30c6\u30e5\u30fc\u30c8 2016,\u6771\u5e83\u5cf6\u5e02,2016 \u5e74\uff18\u6708\u2015\uff19\u6708.<\/li>\n<li>\u9ad8\u6a4b\u96bc\u4e5f,<span class=\"underline\">\u4e21\u89d2\u5353\u4e5f<\/span>,\u6e05\u6c34\u52c7\u4ecb,\u6885\u679d\u5b8f\u4e4b:\u300c\u30af\u30a9\u30fc\u30af\u30b7\u30fc\u30bd\u30fc\u6a21\u578b\u306e\u4f4e\u30a8\u30cd\u30eb\u30ae\u30fc\u6709\u52b9\u7406\u8ad6\u3092\u7528\u3044\u305f\u73fe\u8c61\u8ad6\u300d\u65e5\u672c\u7269\u7406\u5b66\u4f1a2016\u5e74\u79cb\u5b63\u5927\u4f1a,\u5bae\u5d0e\u5e02,2016\u5e74\uff19\u6708.<\/li>\n<li>\u9ad8\u6a4b\u96bc\u4e5f,<span class=\"underline\">\u4e21\u89d2\u5353\u4e5f<\/span>,\u6e05\u6c34\u96c4\u4ecb,\u6885\u679d\u535a\u4e4b:\u300cvector like\u30af\u30a9\u30fc\u30af\u306b\u56e0\u308b\u4e09\u4e16\u4ee3\u306eCKM\u30e6\u30cb\u30bf\u30ea\u30c6\u30a3\u306e\u7834\u308c\u300d, B \u30d5\u30a1\u30af\u30c8\u30ea\u30fc\u7269\u7406\u52c9\u5f37\u4f1a,\u7b2c19\u56de\u30df\u30fc\u30c6\u30a3\u30f3\u30b0 \u3064\u304f\u3070\u5e02,2016\u5e7412\u6708.<\/li>\n<li>\u9ad8\u6a4b\u96bc\u4e5f,<span class=\"underline\">\u4e21\u89d2\u5353\u4e5f<\/span>,\u6e05\u6c34\u52c7\u4ecb,\u6885\u679d\u5b8f\u4e4b\uff1a\u300cVectorlike\u30af\u30a9\u30fc\u30af\u6a21\u578b\u306b\u304a\u3051\u308b\u4e09\u4e16\u4ee3CKM\u30e6\u30cb\u30bf\u30ea\u30c6\u30a3\u306e\u7834\u308c\u300d\u65e5\u672c\u7269\u7406\u5b66\u4f1a\u7b2c72\u56de\u5e74\u6b21\u5927\u4f1a,\u8c4a\u4e2d\u5e022017\u5e74\uff13\u6708.<\/li>\n<li>\u5927\u517c\u82f1\u6717,<span class=\"underline\">\u4e21\u89d2\u5353\u4e5f<\/span>\uff1a\u300c\u96fb\u5f31\u771f\u7a7a\u306e\u5b89\u5b9a\u6027\u306b\u57fa\u3065\u3044\u305f\u30b7\u30fc\u30bd\u30fc\u6a21\u578b\u306e\u30d1\u30e9\u30e1\u30fc\u30bf\u306b\u5bfe\u3059\u308b\u5236\u9650\u300d;2017\u5e74\uff13\u670817-20\u65e5; \u65e5\u672c\u7269\u7406\u5b66\u4f1a2017\u5e74 \u6625\u5b63\u5927\u4f1a; \u5927\u962a\u5927\u5b66 .<\/li>\n<li>\u6885\u679d\u5b8f\u4e4b, \u6728\u6751\u5927\u81ea, \u6e05\u6c34\u52c7\u4ecb, <span class=\"underline\">\u4e21\u89d2\u5353\u4e5f<\/span>,\u7531\u5b87\u6717\u5927\uff1a\u300cNeutrino oscillation and leptogenesis in Type-I seesaw modelwith four-zero textures\u300d, 2017\u5e74\uff13\u670820\u65e5, \u65e5\u672c\u7269\u7406\u5b66\u4f1a\u7b2c72\u56de\u5e74\u6b21\u5927\u4f1a, \u5927\u962a\u5927\u5b66\u8c4a\u4e2d\u30ad\u30e3\u30f3\u30d1\u30b9.<\/li>\n<li>\u6885\u679d\u5b8f\u4e4b, \u6728\u6751\u5927\u81ea, <span class=\"underline\">\u4e21\u89d2\u5353\u4e5f<\/span>\uff1a\u300cResonance ChiralLagrangian\u306b\u57fa\u3065\u304f\u30bf\u30a6\u5d29\u58ca\u5206\u5e03\u306e\u89e3\u6790\u300d,2016\u5e74\uff19\u6708\uff18\u65e5, \u57fa\u7814\u7814\u7a76\u4f1a \u7d20\u7c92\u5b50\u7269\u7406\u5b66\u306e\u9032\u5c552016,\u57fa\u790e\u7269\u7406\u5b66\u7814\u7a76\u6240.<\/li>\n<li>\u6885\u679d\u5b8f\u4e4b, \u6728\u6751\u5927\u81ea, <span class=\"underline\">\u4e21\u89d2\u5353\u4e5f<\/span>\uff1a\u300cResonance ChiralLagrangian \u3092\u7528\u3044\u305fDalitz\u5d29\u58ca\u306e\u89e3\u6790\u300d,2016\u5e74\uff19\u6708\uff11\u65e5,\u702c\u6238\u5185\u30b5\u30de\u30fc\u30a4\u30f3\u30b9\u30c6\u30a3\u30c6\u30e5\u30fc\u30c82016,\u3072\u308d\u3057\u307e\u56fd\u969b\u30d7\u30e9\u30b6.<\/li>\n<li>Apriadi Salim Adam, <span class=\"underline\">T. Morozumi<\/span>, K.I. Nagao and H. Takata\uff1a\u300cTime evolution of particle number asymmetryin an expanding universe\u300d, SSI 2016, Aug.31th-Sep.2nd 2016, atHigashi-Hiroshima.<\/li>\n<li>\u9ad8\u6728\u5805\u592a, <span class=\"underline\">\u4e21\u89d2\u5353\u4e5f<\/span>, \u6e05\u6c34\u52c7\u4ecb, \u6885\u679d\u5b8f\u4e4b, \u5927\u517c\u82f1\u6717,\u5742\u672c\u5f18\u6a39\uff1a\u300c\u300eA4\u00d7Z3\u30d5\u30ec\u30fc\u30d0\u30fc\u30e2\u30c7\u30eb\u300f\u306e\u53d6\u308a\u3046\u308b\u5404\u771f\u7a7a\u671f\u5f85\u5024\u3068\u305d\u308c\u3089\u306e\u73fe\u8c61\u8ad6\u7684\u306a\u9055\u3044\u300d, 2017\u5e74\uff13\u670820\u65e5,\u65e5\u672c\u7269\u7406\u5b66\u4f1a\u7b2c72\u56de\u5e74\u6b21\u5927\u4f1a, \u5927\u962a\u5927\u5b66\u8c4a\u4e2d\u30ad\u30e3\u30f3\u30d1\u30b9.<\/li>\n<li>\u5742\u672c\u5f18\u6a39, \u7a32\u57a3\u77e5\u5b8f: Sergei D. Odintsov\uff1a\u300cGauged Nambu-Jona-Lasinio\u6a21\u578b\u306b\u304a\u3051\u308bCMB\u63fa\u3089\u304e\u306e\u30a2\u30c8\u30e9\u30af\u30bf\u30fc\u69cb\u9020\u300d, 2017\u5e74\uff13\u670817\u65e5, \u65e5\u672c\u7269\u7406\u5b66\u4f1a\u7b2c72\u56de\u5e74\u6b21\u5927\u4f1a, \u5927\u962a\u5927\u5b66\u8c4a\u4e2d\u30ad\u30e3\u30f3\u30d1\u30b9.<\/li>\n<li>\u5742\u672c\u5f18\u6a39, \u7a32\u57a3\u77e5\u5b8f, Sergei D. Odintsov\uff1a\u300c\u6709\u9650\u306a\u8907\u5408\u30b9\u30b1\u30fc\u30eb\u3092\u6301\u3064GaugedNambu-Jona-Lasinio \u6a21\u578b\u306b\u3088\u308b\u30a4\u30f3\u30d5\u30ec\u30fc\u30b7\u30e7\u30f3\u300d, 2016\u5e74\uff19\u670823\u65e5, \u65e5\u672c\u7269\u7406\u5b66\u4f1a2016\u5e74\u79cb\u5b63\u5927\u4f1a,\u5bae\u5d0e\u5927\u5b66.<\/li>\n<li>\u6751\u4e0a\u7950\u5b50, \u7a32\u57a3\u77e5\u5b8f:\uff08\u6700\u512a\u79c0\u30dd\u30b9\u30bf\u30fc\u8cde\u53d7\u8cde\uff09\u300c\u60c5\u5831\u502b\u7406\u30b8\u30ec\u30f3\u30de\u6559\u6750\u306e\u5206\u6790\u300d, 2016\u5e7412\u670815\u65e5,\u5927\u5b66ICT\u63a8\u9032\u5354\u8b70\u4f1a\u5e74\u6b21\u5927\u4f1a, \u56fd\u7acb\u4eac\u90fd\u56fd\u969b\u4f1a\u9928.<\/li>\n<li>\u6751\u4e0a\u7950\u5b50, \u7a32\u57a3\u77e5\u5b8f:\u300c\u60c5\u5831\u502b\u7406\u30b8\u30ec\u30f3\u30de\u6559\u6750\u306e\u5206\u6790\u300d, 2016\u5e7412\u670817\u65e5, \u30b7\u30f3\u30dd\u30b8\u30a6\u30e0\u300c\u3053\u308c\u304b\u3089\u306e\u5927\u5b66\u306e\u60c5\u5831\u6559\u80b2\u300d, \u4eac\u90fd\u5927\u5b66.<\/li>\n<\/ul>\n\n<p><a id=\"events_H28\"><\/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-1079","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/core-u.hiroshima-u.ac.jp\/en\/wp-json\/wp\/v2\/pages\/1079","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=1079"}],"version-history":[{"count":1,"href":"https:\/\/core-u.hiroshima-u.ac.jp\/en\/wp-json\/wp\/v2\/pages\/1079\/revisions"}],"predecessor-version":[{"id":1080,"href":"https:\/\/core-u.hiroshima-u.ac.jp\/en\/wp-json\/wp\/v2\/pages\/1079\/revisions\/1080"}],"wp:attachment":[{"href":"https:\/\/core-u.hiroshima-u.ac.jp\/en\/wp-json\/wp\/v2\/media?parent=1079"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}