CRCの皆様 2002年9月25--28日に千葉県柏市で行われる国際シンポジウム 　"The Universe Viewed in Gamma-rays" の2nd circularです。関心のある方ぜひご参加ください。 茨城大理　柳田昭平 東大ICRR　森 正樹 ----------------------------------------------- ===== SECOND CIRCULAR ===== August 30, 2002 International Symposium "The Universe Viewed in Gamma-rays --- Univ. Tokyo Workshop 2002 ---" September 25-28, 2002, Kashiwa, Chiba, Japan (Visit the Symposium Website: http://icrhp9.icrr.u-tokyo.ac.jp/Symp2002.html where this circular with information links is available.) [[[ Outline ]]] "The Universe viewed in gamma-rays ---The University of Tokyo Workshop 2002---" will be held on September 25-28, 2002 in Kashiwa, Chiba, Japan. The purpose of this symposium is to discuss the new views of the universe grasped mainly in the rapidly developing high energy gamma-ray astrophysics in the energy range above 10 GeV. New ground-based observatories of very high energy gamma-rays are being built, energy threshold are being lowered, and stereoscopic observations with new telescopes will be started soon. The symposium will cover observational and theoretical aspects of Galactic and extragalactic sources of gamma-rays which contribute to the existence of nonthermal particles in the universe. Information of the photons in other energy regime is mandatory to uncover the secret of very high energy phenomena in the universe and multiwavelength campaigns will be also. This symposium is hosted by ICRR, University of Tokyo and sponsored by the Ministry of Education, Culture, Sports, Science and Technology of Japan. [[[ Program ]]] (* to be confirmed. Online version http://icrhp9.icrr.u-tokyo.ac.jp/abstract/Symp2002/ includes links to abstract bodies.) September 25 (Wed) 15:00- Registration ("Sawayaka Chiba Kenmin Plaza") 18:00- Welcome Party (6F of ICRR Kashiwa campus) September 26 (Thu) Welcome address 09:00-09:10 M. Yoshimura Invited review (1) 09:10-10:10 P. Slane Chandra Studies of Nonthermal Emission from Supernova Remnants and Pulsar Wind Nebulae COFFEE BREAK Galactic sources 10:40-11:10 T.Tanimori TeV gamma rays from synchrotron X-ray SNRs 11:10-11:50 E. Berezhko Gamma -ray emission expected from young supernova remnants LUNCH BREAK 13:30-14:00 O. de Jager Pulsars and Plerions from a Multiwavelength Perspective 14:00-14:30 M. Pohl Diffuse emission from the Galactic plane and unidentified EGRET sources Status of high energy gamma-ray observation (contributed papers) 14:30-14:50 D. Hanna STACEE OBSERVATIONS OF EXTRAGALACTIC SOURCES 14:50-15:10 F. Piron The Crab nebula and Mkn 421 high-energy gamma-ray spectra above 50 GeV from CELESTE observations in 1999-2000 15:10-15:30 F. Krennrich Results from the VERITAS Collaboration COFFEE BREAK 16:00-16:20 D. Horns Recent results and status of the HEGRA imaging air Cherenkov telescopes 16:20-16:35 K. Okumura Results from CANGAROO (Extragalactic objects) 16:35-16:50 A. Kawachi Results from CANGAROO (Galactic objects) 16:50-17:05 J. Holder Observations of 1ES1959+650 with the Whipple 10m telescope 17:05-17:20 G. Rowell Evidence for an Unidentified TeV Source in the Vicinity of Cygnus OB2 17:20-17:35 G. Puehlhofer Scans of the TeV gamma-ray sky with the HEGRA system of Cherenkov Telescopes 17:35-17:50 B. Achara Pachmarhi Array of Cherenkov Telescopes f17:50-18:05 N. Hotta Recent status of the Tibet AS gamma experiment 18:05-18:20 M. Teshima Evidence for point sources of Extremely High Energy Cosmic Rays 18:20-18:35 J. McEnery The Milagro Gamma-Ray Observatory September 27 (Fri) Invited review (2) 09:00-10:00 E.Dwek Diffuse infrared background radiation* COFFEE BREAK Extragalactic sources 10:30-11:00 P.Coppi Blazars (theoretical aspects)* 11:00-11:30 R.Mukherjee High Energy Emission from Blazars (Observations) 11:30-12:00 H.Voelk Origin and distribution of cosmic rays associated with cluster of galaxies and with starburst galaxies* LUNCH BREAK Techniques and projects (contributed papers) 13:30-13:50 R. Ong STATUS OF THE VERITAS PROJECT 13:50-14:10 E. Lorenz Status of the 17 m diameter MAGIC Telescope 14:10-14:30 H. Hoffman H.E.S.S. project* 14:30-14:45 M. Ohishi Status of CANGAROO-III 14:45-15:00 R. Mirzoyan The MAGIC Telescope Project: Phase II COFFEE BREAK General gamma-ray astrophysics (contributed papers) 15:30-15:45 S. Shibata The Crab Nebula: 3-dimensional modeling 15:45-16:00 A. Bamba Fine Structures of the Thermal and Non-Thermal X-Rays in the SN1006 Shell 16:00-16:15 F. Pacini Quenching of the pulsar wind by Inverse Compton Scattering against thermalradiation from the neutron star 16:15-16:30 T. Tamagawa Properties of Gamma-ray Bursts localized by the HETE-2 satellite 16:30-16:45 P. Edwards Parsec-scale VLBI observations of TeV gamma-ray sources 16:45-17:00 F. Miniati Investigating Galaxy Clusters through Gamma-ray Emission 17:00-17:15 V. Pavlidou The Guaranteed Gamma Ray Background Banquet September 28 (Sat) Invited review (3) 09:00-10:00 L.Bergstroem Gamma ray signatures of dark matter particles COFFEE BREAK Cosmic Rays 10:30-11:00 D.Kieda High Resolution Cosmic Ray Measurements using Next Generation Ground-based Gamma Ray Observatories 11:00-11:30 M.Hoshino Plasma Physics View of Particle Acceleration 11:30-12:00 R.Schlickeiser Relativistic and nonrelativistic shock acceleration in various objects LUNCH BREAK 13:30-14:15 F. Takahara Summary 14:15-14:30 T. Kifune Concluding remarks Adjourn (evening) ((((( Poster session ))))) (First author) (Title) Status of high energy gamma-ray observation (contributed papers) V.G. Sinitsyna The detection of the new active galactic gamma-sources NGC 1275, 3c454.3 and 17399+522 and comparison with early known metagalactic and galactic sources K.Okumura Observation of gamma-rays greater than 10TeV from Markarian421 during the flaring state in 2001 P.Majumdar Preliminary Results on Crab from Pachmarhi Array of Cerenkov Telescopes K. Tsuchiya Very High Energy Gamma Rays from Galactic Center S.S. Borisov Evidence of TeV gamma-ray radiation in supernova remnants CYGNUS X-3 H.Katagiri The observation of TeV gamma rays from RXJ0852.0-4622 with CANGAROO-II 10m telescope S. Molkov The Study of Evolution of Hard X-ray Emission from transients LMXBs During a Outburst by INTEGRAL. (2 accepted AO-1 INTEGRAL's proposals) M. Schroedter Multi-wavelength Observations of 1ES1959 in a Flaring State L. M. Boone STACEE Observations of Markarian 421 During the 2001 Flare J. Cortina HEGRA CT1 Spectrum and Light Curve of Mrk-421 during its 2001 flare S. Hayashi Observation of Very High Energy Gamma Rays from SS433/W50 with CANGAROO-II Telescope D. Horns Observations of 1ES1959+650 with the HEGRA system of imaging air Cherenkov telescopes C.Itoh Study of the nearest starburst Galaxy: NGC253 A. Kawachi TeV Gamma-ray Observations of the PSRB1259-63/SS2883 Binary System with the CANGAROO-II 10m Telescope J. Kushida Study of TeV gamma-ray emission mechanism of PSR 1706-44 based on multi-wavelength spectrum S. Osone Long periodicity of Blazars with RXTE ASM, TA and HEGRA M. Sakata A wide sky survey for flare type TeV gamma-ray sources using the Tibet-HD data M. Ueno Non-thermal emission from an X-ray shell near at 30 Dor C S.Watanabe TeV gamma-ray observations of the Supernova Remnant RCW86 with the CANGAROO-II telescope Y.Yamamoto Upper Limits of Diffuse Gamma Rays from the Galactic Plane at 10 TeV with the Tibet-II and III Arrays T. Nakase Observation of Southern High Energy Peaked BL Lacerate Object PKS 2155-304 with CANGAROO-II Telescope T.Hattori Search for gamma-ray clusters of galaxies with CANGAROO-II telescope Techniques and projects (contributed papers) R. Cowsik High Altitude Gamma Ray Observatory at Hanle (HAGAR) V.Y. Sinitsyna Efficiency of selection of gamma - quanta from a proton background in experiment SHALON on observation results of extragalactic sources NGC1275, 1739+522, 3c454.3 and Mkn421, Mkn501. A.Lutovinov Organization of Russian Science Data Center of the INTEGRAL project S.Kabuki Development of an atmospheric Cherenkov imaging camera for the CANGAROO-III experiment J. Cortina THE CONTROL SYSTEM OF THE MAGIC TELESCOPE G. Puehlhofer Technical performance of the HEGRA IACT system R. Cornils Mirror alignment and optical quality of the H.E.S.S. imaging atmospheric Cherenkov telescopes J. Cortina An absolute light flux calibration for the MAGIC telescope J. Cortina THE DATA ACQUISITION OF THE MAGIC TELESCOPE C.E. Covault Performance Characteristics of the STACEE Gamma-Ray Observatory F. Kajino High-Resolution Cherenkov Telescopes for the Observation of High Energy Gamma rays D.Nishida Development of the data acquisition system of the CANGAROO-III telescope K. Nishijima Development of trigger module for CANGAROO-III M. Ohishi Performance of the plastic spherical mirrors of CANGAROO-III telescope S. Osone Concept of new gamma ray detector A.Asahara Performance of 10 - 100 ~GeV gamma ray camera, "CheSS" for SUBARU optical-infrared telescope F. Krennrich Short GAmma Ray Front Air Cherenkov Experiment S. LeBohec Calibration of Atmospheric Cherenkov Telescopes using Cosmic Ray Background Events General gamma-ray astrophysics (contributed papers) S.I. Nikolsky The distinction of spectra both cosmic rays and gamma-quanta of local sources and formation of uniform cosmic ray spectrum J.Dyks Signatures of pulsar polar-gap emission at the high-energy spectral cutoff K. George Missing afterglows of GRBs G. Ter-Ghazaryan Neutrino cooling of AGN's superdense core at presence of spherical symmetric accretion and origin of extragalactic high energy gamma-rays. A. Pozanenko High frequencies in the power spectrum of Gamma-Ray Burst O. Kurtanidze Study of AGNs by Multiband Optical BVRI CCD Photometry A.Lutovinov Hard X-ray observations of the X-ray pulsar GX301-2 S.V. Molkov X-RAY SPECTRAL VARIABILITY OF THE Z-SOURCE GX340+0 K. Oka Gamma-ray Emission from an Accretion Flow around a Kerr Black Hole S. Inoue Gamma-rays and Cosmic Rays from Large-Scale Shocks in the Universe J. Takata Gamma-ray emission from Outer-Gap of pulsar magnetosphere M. Ohishi Galactic diffuse gamma-ray spectrum from cosmic-ray proton interactions with gas clouds H. Muraishi Extragalactic cosmic rays modulated by the galactic wind and its implication for the origin of the `knee' N. Shibazaki X-Ray and Gamma-Ray Emission from the PSR1259-63/Be Star System N.Tateyama High Energy Diffuse Gamma-Rays from Galactic Plane T. Naito High energy gamma-ray emission from merging clusters of galaxies R. Clay Our Galaxy Close to a Source of EeV Cosmic Rays P. Tinyakov Evidence for a connection between gamma-ray and UHECR emissions by BL Lacs [[[ Presentation ]]] The official language of the Symposium is English. For oral presentation you can use an overhead projector or an LCD projector with XGA (1024x768) resolution. For poster presentation, the panel size is 150cm x 150cm. LOC will supply pins for posting your poster paper. ** Important notice ** Every presenters are kindly requested to bring a set of hardcopies (in color if possible) of your transparencies or a poster (reduced in size up to A3 [297mm x 420mm]) to the registration desk, or send or bring the file (on your notebook PC or on CD-R / MS PowerPoint, MS Word, MS Publisher, PDF, HTML formats are preferred) of your presentation beforehand or at the Symposium. These will be posted to the Symposium Website afterwards for a convenience of participants and community. Note 1. You can use the file you sent for presentation with a PC prepared by LOC, but you may want to bring your notebook PC to avoid possible compatibility problems [font, format etc.]) Note 2. You can send your file to Ms Kobayashi by e-mail as a MIME-attachment file, or you can show us a URL to access your file. Note 3. LOC will prepare a USB flash memory to transfer files on site: this will utilize USB1.1 port and can be used if you are using Windows Me, 2000 or XP without installing drivers. [[[ Proceedings ]]] The Symposium proceedings will be published as a hardcover book. Both invited talks and contributed papers will be included. Authors are required to prepare a camera-ready manuscript. Electronic submission is preferred (the details will be informed at the Symposium). The deadline for submission will be November 30, 2002. [[[ Calender of Events ]]] March 28, 2002 Announcement June 13, 2002 1st Circular June 13, 2002 Registration start August 01, 2002 Deadline for abstract submission August, 2002 2nd Circular September 01, 2002 Deadline for late registration September 25-28, 2002 Symposium November 30, 2002 Deadline for proceedings manuscript Spring 2003 Publication of proceedings [[[ Location ]]] The venue of the symposium will be the main hall of "Sawayaka Chiba Kenmin Plaza" near the Institute for Cosmic Ray Research (ICRR) of the University Tokyo, in Kashiwa, Chiba, Japan, which locates in Kashiwa campus, the newest major campus of University of Tokyo. An overhead projector and an LCD projector with a CCD camera and an RGB interface (XGA resolution) will be equipped for presentation. Kashiwa City is located 30 kilometers northeast of Tokyo. The access map to our institute is here. The "Sawayaka Chiba Kenmin Plaza" is 5-min walk from ICRR. [[[ Travel information ]]] New Tokyo International (Narita) airport to Kashiwa You can use railway or bus services. Detailed instruction is found on the Web. (You can obtain a detailed railway map in greater Tokyo area here.) Kashiwa station to ICRR Univ.Tokyo/Kenmin Plaza You can use bus services or taxis. See "Location" and transfer instruction and the map on the Web. There are image files of some Japanese words which can be used as signs to show your taxi/bus driver. http://www.icrr.u-tokyo.ac.jp/can/images/sheets.html Maps of Kashiwa city and station etc. are now available: http://www.icrr.u-tokyo.ac.jp/can/images/maps.html Visa For many countries visa is not required to enter Japan for a visit less than 90 days, but depends on your nationality. See the Web for detailed information. Weather September is the time weather is changing into autumn and rather good season to visit Japan. The average temperature is about 23degree Celsius (average maximum: 26.5degree, average minimum: 20.2degree) and the relative humidity is 78% on average. General travel information: Yahoo travel: Japan Chiba prefecture tourist information (on the Web) [[[ Banquet ]]] Symposium banquet will be held on September 27 (Fri) evening at the Cafeteria of the Kashiwa campus of University of Tokyo (5-min walk from the Symposium venue). A ticket will be JPY 6,000 per person (JPY 4,000 per accompanying person) including drinks. Limited number of tickets are still available: Please contact Ms Kobayashi (noriko [at] icrr.u-tokyo.ac.jp) promptly. [[[ Registration ]]] The deadline for early registration is past but you can still participate in the Symposium at your own arrangement of accommodation. Please register using this form or directly send an E-mail to Ms. Noriko Kobayashi (noriko [at] icrr.u-tokyo.ac.jp). The registration fee includes the fees for the Proceedings, coffee breaks which should be paid in Japanese yen (cash only) upon your arrival at the registration desk. After August 1, the late registration fee of JPY 25,000 will be applied. [[[ Registration desk ]]] The registration desk will be open at 15:00-17:30 on Sep.25 (Wed) and during the Symposium at the "Sawayaka Chiba Kenmin Plaza". During the reception, 18:00-20:00, Sep.25, however, the desk is at the sixth floor of Institute for Cosmic Ray Research, where the reception will be held. For your help, call 090-5552-0251 (Dr.Enomoto) during the Symposium. [[[ Reception ]]] On September 25, there is a reception party at the sixth floor of Institute for Cosmic Ray Research, Kashiwa campus during 18:00-20:00. Every participants including accompanying persons are invited. Drinks and snacks will be served at free of charge. [[[ Network facility ]]] There is no network facility at the site. However, a room of ICRR Kashiwa campus will be open with several terminals for networking and 10/100base-T ports (DHCP capable) for your PC connection during the Symposium. It locates less than 10-min walk from the site. Please consult the registration desk for details. [[[ Foreign Currencies ]]] Only Japanese yen in cash is acceptable as payment at the registration desk. Neither credit cards nor checks are acceptable there. No banks are located near the symposium site and ICRR. However, an ATM of Post Office is located at "Kokuritsu Gan Centre" (National Cancer Centre), about 5-minute walk from the site, and open weekdays from 9:00 to 18:00. Major credits cards such as Visa and MasterCard are accepted. Consumer tax: You have to pay consumer tax of additional 5% when you purchase goods or services in Japan. [[[ Scientific Advisory Committee ]]] Geoffrey Bicknell (Mt Stromlo and Siding Spring Observatories, Australian National Univ.) Bernard Degrange (LPNHE-X, Ecole Ploytechnique) Masataka Fukugita (ICRR, Univ. Tokyo) Werner Hofmann (MPI, Heidelberg) Ocker de Jager(Potchefstroom Univ.) Tadashi Kifune (Shinshuu Univ.) Katsuji Koyama (Kyoto Univ.) Eckart Lorenz (Max-Planck-Institut fur Physik, Munchen) Rene Ong (Univ. California, Los Angeles) Reinhard Schlickeiser (Lehrstuhl fur Theoretische Physik IV der Ruhr-Universitat Bochum) Simon Swordy (Univ. Chicago) Fumio Takahara (Osaka Univ.) Heinrich Voelk (MPI, Heidelberg) Trevor Weekes (Smithsonian Astrophys. Obs.) [[[ Local Organizing Committee ]]] Ryoji Enomoto (Co-chair of LOC, ICRR) Shuichi Gunji (Yamagata Univ.) Masaki Mori (Co-chair of LOC, ICRR) Kyoshi Nishijima (Tokai Univ.) Toru Tanimori (Kyoto Univ.) Shohei Yanagita (Co-chair of LOC, Ibaraki Univ.) [[[ Secretary ]]] Ms. Noriko Kobayashi (noriko [at] icrr.u-tokyo.ac.jp) Telephone: +81-4-7136-3135 Facsimile: +81-4-7136-3133