A broadband x-ray imaging spectroscopy with high-angular resolution: the FORCE mission
暂无分享,去创建一个
William W. Zhang | Tadayuki Takahashi | Kazuhiro Nakazawa | Takashi Okajima | Hiroshi Murakami | Yasushi Fukazawa | Hironori Matsumoto | Hiroshi Tsunemi | Koji Mori | Yoshihiro Ueda | Takeshi Go Tsuru | Hisamitsu Awaki | H. Murakami | T. Tsuru | Y. Fukazawa | T. Okajima | K. Nakazawa | H. Awaki | H. Matsumoto | K. Mori | Tadayuki Takahashi | H. Tsunemi | Y. Ueda | Will Zhang | H. Matsumoto | H. Murakami
[1] Leon P. Van Speybroeck. Grazing Incidence Optics For The U.S. High-Resolution X-Ray Astronomy Program , 1988, Optics & Photonics.
[2] Hideyo Kunieda,et al. The X-ray telescope on board ASCA , 1995 .
[3] Naomi Ota,et al. X-ray spectroscopy of clusters of galaxies , 2012, 1211.0679.
[4] Yoshiharu Namba,et al. Characterization of the supermirror hard-x-ray telescope for the InFOCmuS balloon experiment. , 2002, Applied optics.
[5] Kai-Wing Chan,et al. Production and performance of the inFOCmicroS 20-40-keV graded multilayer mirror. , 2013, Applied optics.
[6] Makoto Sawada,et al. Synchrotron X-ray diagnostics of cutoff shape of nonthermal electron spectrum at young supernova remnants , 2013, 1301.7499.
[7] G. Neugebauer,et al. Ultraluminous infrared galaxies and the origin of quasars , 1988 .
[8] Takao Nakagawa,et al. A Spitzer IRS Low-Resolution Spectroscopic Search for Buried AGNs in Nearby Ultraluminous Infrared Galaxies: A Constraint on Geometry between Energy Sources and Dust , 2007, astro-ph/0702136.
[9] P. Hopkins,et al. Determining the Properties and Evolution of Red Galaxies from the Quasar Luminosity Function , 2005, astro-ph/0508167.
[10] P A de Korte. High-throughput replica optics. , 1988, Applied optics.
[11] Aya Kubota,et al. The Nature of Ultraluminous Compact X-Ray Sources in Nearby Spiral Galaxies , 2000, astro-ph/0001009.
[12] M. Turler,et al. INTEGRAL hard X-ray spectra of the cosmic X-ray background and Galactic ridge emission , 2010, 1001.2110.
[13] Riccardo Giacconi,et al. A “telescope” for soft X‐ray astronomy , 1960 .
[14] William W. Zhang,et al. Lightweight and high-resolution single crystal silicon optics for x-ray astronomy , 2016, Astronomical Telescopes + Instrumentation.
[15] Motohide Kokubun,et al. The hard x-ray imager (HXI) onboard ASTRO-H , 2016, Astronomical Telescopes + Instrumentation.
[16] Yoshiharu Namba,et al. The ASTRO-H X-ray astronomy satellite , 2014, Astronomical Telescopes and Instrumentation.
[17] S. Reynolds,et al. Maximum Energies of Shock-accelerated Electrons in Young Shell Supernova Remnants , 1999 .
[18] Shunsaku Okada,et al. The X-Ray Telescope onboard Suzaku , 2007 .
[19] Kristin K. Madsen,et al. NuSTAR OBSERVATIONS OF THE BULLET CLUSTER: CONSTRAINTS ON INVERSE COMPTON EMISSION , 2014, 1403.2722.
[20] Laura Brenneman,et al. THE BROAD-BAND X-RAY SPECTRUM OF IC 4329A FROM A JOINT NuSTAR/SUZAKU OBSERVATION , 2014, 1404.7486.
[21] Philippe Gondoin,et al. X-ray multi-mirror (XMM) telescope , 1994, Optics & Photonics.
[22] Aya Bamba,et al. Small-Scale Structure of the SN 1006 Shock with Chandra Observations , 2003 .
[23] Motohide Kokubun,et al. Suzaku Detection of Extended/Diffuse Hard X-Ray Emission from the Galactic Center , 2007, 0709.1580.
[24] Luigi Gallo,et al. The Canadian Astro-H metrology system , 2012, Other Conferences.
[25] Ronald A. Remillard,et al. X-Ray Properties of Black-Hole Binaries , 2006, astro-ph/0606352.
[26] Hideyuki Mori,et al. First peek of ASTRO-H Soft X-ray Telescope (SXT) in-orbit performance , 2016, Astronomical Telescopes + Instrumentation.
[27] R. Petre,et al. Evidence for shock acceleration of high-energy electrons in the supernova remnant SN1006 , 1995, Nature.
[28] Shoji Kawahito,et al. Development and performance of Kyoto's x-ray astronomical SOI pixel (SOIPIX) sensor , 2014, Astronomical Telescopes and Instrumentation.
[29] Takamitsu Miyaji,et al. TOWARD THE STANDARD POPULATION SYNTHESIS MODEL OF THE X-RAY BACKGROUND: EVOLUTION OF X-RAY LUMINOSITY AND ABSORPTION FUNCTIONS OF ACTIVE GALACTIC NUCLEI INCLUDING COMPTON-THICK POPULATIONS , 2014 .
[30] Yoshiharu Namba,et al. Performance of ASTRO-H hard x-ray telescope (HXT) , 2016, Astronomical Telescopes + Instrumentation.
[31] Joern Wilms,et al. THE REFLECTION COMPONENT FROM CYGNUS X-1 IN THE SOFT STATE MEASURED BY NuSTAR AND SUZAKU , 2013, 1310.3830.
[32] Paolo Conconi,et al. Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series , 2012 .
[33] Felix A. Aharonian,et al. Extremely fast acceleration of cosmic rays in a supernova remnant , 2007, Nature.
[34] William W. Zhang,et al. Manufacture of mirror glass substrates for the NuSTAR mission , 2009, Optical Engineering + Applications.
[35] Kristin K. Madsen,et al. Extended hard-X-ray emission in the inner few parsecs of the Galaxy , 2015, Nature.
[36] D. J. Walton,et al. A rapidly spinning supermassive black hole at the centre of NGC 1365 , 2013, Nature.
[37] Gordon Tajiri,et al. Fabrication of the NuSTAR flight optics , 2011, Optical Engineering + Applications.
[38] Mark J. Devlin,et al. First light of a hard-x-ray imaging experiment: the InFOCμS balloon flight , 2005, SPIE Optics + Photonics.
[39] T. Nakamura,et al. Emission from Isolated Black Holes and MACHOs Accreting from the Interstellar Medium , 1997, astro-ph/9712284.
[40] Hiroshi Tsunemi,et al. Thermal X-ray emission with intense 6.7-keV iron line from the galactic ridge. , 1986 .
[41] Bernd Aschenbach. Design, Construction, And Performance Of The ROSAT High-Resolution X-Ray Mirror Assembly , 1988, Optics & Photonics.
[42] P J Serlemitsos. Conical foil x-ray mirrors: performance and projections. , 1988, Applied optics.
[43] Van Speybroeck. Design, Fabrication And Expected Performance Of The HEAO-B X-Ray Telescope , 1977 .