China’s Future Missions in Space High Energy Astrophysics Shuang Nan Zhang 张双南 Tsinghua University and Institute of High Energy Physics, Chinese Academy.

Slides:

Advertisements

Similar presentations

Observation of the Universe from the Moon – Elisabetta Cavazzuti – LNF May 7, 2007 ITALIAN VISION FOR MOON EXPLORATION OBSERVATION OF THE UNIVERSE FROM.

Advertisements

The MAGIC telescope and the GLAST satellite La Palma, Roque de los Muchacos (28.8° latitude ° longitude, 2225 m asl) INAUGURATION: 10/10/2003 LAT.

The Science of Gamma-Ray Bursts: caution, extreme physics at play Bruce Gendre ARTEMIS.

Bruce Gendre Osservatorio di Roma / ASI Science Data Center Recent activities from the TAROT/Zadko network.

Web: Contact: HAWC is a collaborative effort between institutions in the United States of America.

Gamma-Ray Bursts & High Energy Astrophysics Kunihito Ioka (KEK) 井岡邦仁.

NuSTAR CIT JPL Columbia LLNL DSRI UCSC SLAC Spectrum The Nuclear Spectroscopic Telescope Array (NuSTAR) Hard X-ray ( keV) Small Explorer (SMEX) mission.

X-ray polarisation: Science

Vicky Kaspi McGill University Lorne Trottier Chair in Astrophysics and Cosmology.

Science Drivers for the Next Generation VHE Telescope(s?) G. Sinnis with much help from C. Dermer, J. Buckley, H. Krawczynski, S. LeBohec, R. Ong, M. Pohl,

HXMT – A Chinese High Energy Astrophysics Mission Li Ti-Pei Inst. Of High Energy Physics, Chinese Academy of Sciences Center for Astrophysics, Tsinghua.

The Transient Universe: AY 250 Spring 2007 Existing Transient Surveys: High Energy II: X-ray Binaries Geoff Bower.

The Hard X-ray Modulation Telescope (HXMT) Fangjun Lu (Institute of High Energy Physics, Chinese Academy of Sciences) On behalf of the HXMT group.

Julie McEnery1 GLAST: Multiwavelength Science with a New Mission Julie Mc Enery Gamma-ray Large Area Space Telescope.

Early Results from SWIFT's BAT AGN Survey: XMM Follow-up Observations for 22 BAT AGNs Lisa Winter Lisa Winter (Grad Student at UMD) Richard Mushotzky (GSFC),

The Transient Universe: AY 250 Spring 2007 Existing Transient Surveys: High Energy I: Gamma-Ray Bursts Geoff Bower.

3rd Potsdam Thinkshop Robotic Astronomy Gamma-ray burst optical follow-ups with robotic telescopes M.I. Andersen Gamma-ray burst optical follow-ups with.

14 July 2009Keith Bechtol1 GeV Gamma-ray Observations of Galaxy Clusters with the Fermi LAT Keith Bechtol representing the Fermi LAT Collaboration July.

The ANTARES Neutrino Telescope Mieke Bouwhuis 27/03/2006.

Shu Zhang (on behalf of the HXMT team) Institute of High Energy Physics, Chinese Academy of Science The current status of HXMT and its calibrations.

High-energy emission from the tidal disruption of stars by massive black holes Xiang-Yu Wang Nanjing University, China Collaborators: K. S. Cheng(HKU),

Shuang-Nan Zhang (张双南) Center for Particle Astrophysics 粒子天体物理中心

Brief Overview of China’s Future Space X-ray Astronomy Program

X-ray Timing and Polarization mission & instrumentation DONG Yongwei Center for Particle Astrophysics Institute of High Energy Physics, Chinese Academy.

Gravitational-wave research in China: overview Eric O. L EBIGOT Tsinghua University, Beijing University of Paris 7 / CNRS (APC) 1.

1 Arecibo Synergy with GLAST (and other gamma-ray telescopes) Frontiers of Astronomy with the World’s Largest Radio Telescope 12 September 2007 Dave Thompson.

LU Fangjun (on behalf of the HXMT team) Institute of High Energy Physics, Chinese Academy of Science Current Status of the Hard X-ray Modulation Telescope.

The Project of Space Experiment with Wide Field Gamma-Ray Telescope (“GAMMASCOPE”) Skobeltsyn Institute of Nuclear Physics, Moscow State University.

RELEC project (Relativistic ELECtrons). Unified platform “Karat” for small spacecraft 2 MICROSATELLITE KARAT FOR PLANETARY MISSIONS, ASTROPHYSICAL AND.

High-Energy Astrophysics

The Hard X-ray Modulation Telescope Mission

SRG 1 X-RAY Astronomy 2009, Bologna, 11 September, 2009 Spectrum-Roentgen-Gamma astrophysical project, current status Mikhail Pavlinsky (IKI, Moscow) on.

International research project GALA: Monitoring of high energy gamma-ray astrophysical sources.

Prospects in space-based Gamma-Ray Astronomy Jürgen Knödlseder Centre d’Etude Spatiale des Rayonnements, Toulouse, France On behalf of the European Gamma-Ray.

Black Holes Regions of space from which nothing, not even light, can escape because gravity is so strong. First postulated in 1783 by John Michell Term.

Study performed by Donghua Zhao during her one year stay in France Ms. Donghua is a IHEP PhD student. Her stay was founded by the CSC-FCPPL PhD grants.

Summary(3) -- Dynamics in the universe -- T. Ohashi (Tokyo Metropolitan U) 1.Instrumentation for dynamics 2.Cluster hard X-rays 3.X-ray cavities 4.Dark.

Pace Multi-bandariablebjectsonitor Space Multi-band Variable Objects Monitor -----A Chinese-French Mission for GRBs WEI Jianyan NAOC, Beijing Jacques PAUL.

Prospects in space-based Gamma-Ray Astronomy for Europe --- Objective of the meeting Jürgen Knödlseder Centre d’Etude Spatiale des Rayonnements, Toulouse,

19/02/09ARC Meeting, Colonster The Simbol-X mission and the investigation of hard X-rays from massive stars Michaël De Becker (Groupe d'AstroPhysique des.

Current and Future Space X-ray astronomy Missions in China Chen Zhang represent Prof. Shuang-Nan Zhang Institute of High Energy Physics National Astronomical.

Fermi Observations of Gamma-ray Bursts Masanori Ohno(ISAS/JAXA) on behalf of Fermi LAT/GBM collaborations April 19, Deciphering the Ancient Universe.

High sensitivity all sky X-ray monitor and survey with MAXI Mihara, M. kohama, M. Suzuki (RIKEN), M. Matsuoka, S. Ueno, H. Tomida (JAXA), N. Kawai, J.

Gamma-Ray Bursts Energy problem and beaming * Mergers versus collapsars GRB host galaxies and locations within galaxy Supernova connection Fireball model.

Prof. Steven Boggs UCB Space Sciences Laboratory SPI Instrument Team Activities Prof. Steven Boggs (PI) Dr. Cornelia Wunderer (SPI CoI) Dr. Emrah Kalemci.

Space Part 06, Beijing, China, April 21, Lobster-Eye (LE) Novel Wide Field X-ray Telescopes FOV of 100 sq. deg. and more easily possible (classical.

06/02/2009Diego Götz - The SVOM Mission1 La Thuile Italy 06/ th Rencontres de Moriond SVOM A new mission for Gamma-Ray Bursts Studies Diego Götz.

Tobias Jogler Max – Planck Institute für Physik MAGIC Observations of the HMXB LS I in VHE gamma rays Tobias Jogler on behalf.

Observation of cosmic gamma-ray bursts and solar flares in the ''RELEC'' experiment on the ''VERNOV'' satellite.

25s detection of the Sy1 galaxy NGC3516 The Palermo BAT survey project Application to a sample of SDSS LINERs V. La Parola, A.Segreto, G. Cusumano, V.

Gamma-Ray Bursts with the ANTARES neutrino telescope S. Escoffier CNRS/CPPM, Marseille.

Sources emitting gamma-rays observed in the MAGIC field of view Jelena-Kristina Željeznjak , Zagreb.

FIRST LIGHT A selection of future facilities relevant to the formation and evolution of galaxies Wavelength Sensitivity Spatial resolution.

Exploring an evidence of supermassive black hole binaries in AGN with MAXI Naoki Isobe (RIKEN, ) and the MAXI

Cleared for export. High Energy X-ray Probe Fiona Harrison Caltech.

The Search for Black Holes

Stochastic wake field particle acceleration in Gamma-Ray Bursts Barbiellini G., Longo F. (1), Omodei N. (2), Giulietti D., Tommassini P. (3), Celotti A.

Swift-BAT as a Triggering Facility Amy Lien Scott Barthelmy, Hans Krimm NASA Goddard Space Flight Center The 4 th AMON workshop, Penn State University,

Overview on XTP sciences Zhang Shu (on behalf of the XTP science team) Institute of High Energy Physics.

Science Drivers for Small Missions in High Energy Astrophysics Luigi PiroCAS-ESA Workshop – Chengdu Feb. 25, 2014 Science Drivers for Small Missions in.

Gamma-ray bursts Tomasz Bulik CAM K, Warsaw. Outline ● Observations: prompt gamma emission, afterglows ● Theoretical modeling ● Current challenges in.

For the 11th IACHEC meeting , Pune, India POLAR status and beam test with ESRF in 2015 Bobing WU Institute of High Energy Physics, CAS On behalf.

Tobias Jogler Max-Planck Institut für Physik IMPRS YSW Ringberg 2007 VHE emission from binary systems Outline Binary systems Microquasar Pulsar binaries.

for Lomonosov-GRB collaboration

The HXMT in-flight calibration plan Shaolin XIONG, Shijie ZHENG, Liming SONG On behalf of HXMT SGS team Institue of High Energy Physics, China 11th.

Simulations for WXT aboard Einstein Probe mission with Geant4

Monitor of All sky X-ray Image (MAXI)

(National Astronomical Observatory of Japan)

Magnetars with Insight-HXMT

Presentation transcript:

China’s Future Missions in Space High Energy Astrophysics Shuang Nan Zhang 张双南 Tsinghua University and Institute of High Energy Physics, Chinese Academy of Sciences

HXMT in space: planned for launch around 2010 Payload Cabin Service Cabin

Low Energy X-ray Telescope (LE) (1-15 keV) SCD, 384 cm 2 ) Medium Energy X-ray Telescope (ME) (5-30 keV) (SiPIN, 952 cm 2 ) Detectors onboard High Energy X-ray Telescope (HE) ( keV, 18 modules, 5000 cm 2 )

HXMT Full Sky Survey

1 year exposure map HXMT full sky survey

Hard X-ray sky survey with highest sensitivity Hard X-ray full sky map: diffuse background and cosmic variance Discover highly obscured supermassive BHs: galaxy formation and evolution Discover new types of high energy objects: usual surprises of new surveys Main science of HXMT (1)

HXMT Pointed Observation

Broad band and large collection area pointed observations of high energy objects Space-time in strong gravitational field: dynamics and radiation near BH horizons of stellar mass and supermassive BHs High energy particle acceleration: AGN, SNR, shock and relativistic jets Large scale structure: through hard X-ray detection of galaxy clusters Main science of HXMT (2)

Variability of X-ray binaries Power spectrum Light curve

AGN Broad band spectrum Reflection component not fitted

A multi-λGRB project: SVOM France: keV France: keV China: 30 keV-5 MeV China: 45 cm diameter Launch time:

Instrument concept proposed by N. Produit, et al., NIM (2005) Onboard China’s spacelab TG-2: launch time A China-led international collaboration FOV of POLAR: ~½ sky Requires directionality and energy spectrum known after the fact Tian-Gong天宫 Palace in Heaven POLAR Gamma-ray burst polarization experiment onboard China’s Spacelab: POLAR

POLAR capability summary 10 GRBs per year down to 8%, or 60 GRBs per year down to 30%, or 100 GRBs per year down to 50% polarization, if all POLAR GRBs are localized independently to ~degrees accuracy by other GRB instruments.