The FORCE mission: science aim and instrument parameter for broadband x-ray imaging spectroscopy with good angular resolution
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Manabu Ishida | William W. Zhang | Tadayuki Takahashi | Kazuhiro Nakazawa | Takashi Okajima | Hiroshi Murakami | Yasushi Fukazawa | Hironori Matsumoto | Hiroshi Tsunemi | Takeshi G. Tsuru | Koji Mori | Yoshihiro Ueda | Hisamitsu Awaki | H. Murakami | T. Tsuru | Y. Fukazawa | T. Okajima | K. Nakazawa | H. Awaki | M. Ishida | H. Matsumoto | K. Mori | Tadayuki Takahashi | H. Tsunemi | Y. Ueda | Will Zhang
[1] Ryuichi Fujimoto,et al. The High-Resolution X-Ray Microcalorimeter Spectrometer, SXS, on Astro-H , 2012 .
[2] Ann E. Hornschemeier,et al. SPATIALLY RESOLVING A STARBURST GALAXY AT HARD X-RAY ENERGIES: NuSTAR, CHANDRA, AND VLBA OBSERVATIONS OF NGC 253 , 2014, 1411.1089.
[3] The Ligo Scientific Collaboration,et al. Observation of Gravitational Waves from a Binary Black Hole Merger , 2016, 1602.03837.
[4] Philip Kaaret,et al. Ultraluminous X-Ray Sources , 2017, 1703.10728.
[5] Michael J. Pivovaroff,et al. NuSTAR Hard X-Ray Survey of the Galactic Center Region. II. X-Ray Point Sources , 2016, 1605.03882.
[6] Mamoru Doi,et al. X-RAY AND OPTICAL CORRELATION OF TYPE I SEYFERT NGC 3516 STUDIED WITH SUZAKU AND JAPANESE GROUND-BASED TELESCOPES , 2016, 1605.08050.
[7] William W. Zhang,et al. THE NUCLEAR SPECTROSCOPIC TELESCOPE ARRAY (NuSTAR) HIGH-ENERGY X-RAY MISSION , 2013, Astronomical Telescopes and Instrumentation.
[8] Ronald A. Remillard,et al. X-Ray Properties of Black-Hole Binaries , 2006, astro-ph/0606352.
[9] Hideyo Kunieda,et al. X-Ray Evidence for Seyfert Activity Buried in the Infrared Galaxy NGC 4945 , 1993 .
[10] Matteo Guainazzi,et al. Concept of the X-ray Astronomy Recovery Mission , 2018, Astronomical Telescopes + Instrumentation.
[11] F. Tazaki,et al. ASTRO-H White Paper - AGN Reflection , 2014 .
[12] Tadayuki Takahashi,et al. Design and performance of Soft Gamma-ray Detector onboard the Hitomi (ASTRO-H) satellite , 2018 .
[13] Franz E. Bauer,et al. A density cusp of quiescent X-ray binaries in the central parsec of the Galaxy , 2018, Nature.
[14] W. W. Zhang,et al. Affordable and lightweight high-resolution x-ray optics for astronomical missions , 2014, Astronomical Telescopes and Instrumentation.
[15] Takashi Yoshida,et al. COMPTONIZED PHOTON SPECTRA OF SUPERCRITICAL BLACK HOLE ACCRETION FLOWS WITH APPLICATION TO ULTRALUMINOUS X-RAY SOURCES , 2012 .
[16] Hiroshi Nakajima,et al. Soft X-ray Imager aboard Hitomi (ASTRO-H) , 2018, 1801.06932.
[17] 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 .
[18] Didier Barret,et al. An intermediate-mass black hole of over 500 solar masses in the galaxy ESO 243-49 , 2009, Nature.
[19] Matteo Guainazzi,et al. Hitomi (ASTRO-H) X-ray Astronomy Satellite , 2018 .
[20] Masatoshi Imanishi,et al. Shedding Light on the Compton-thick Active Galactic Nucleus in the Ultraluminous Infrared Galaxy UGC 5101 with Broadband X-Ray Spectroscopy , 2016, 1612.07450.
[21] Richard Mushotzky,et al. The close environments of accreting massive black holes are shaped by radiative feedback , 2017, Nature.
[22] Liyi Gu,et al. Discovery of a nearby early-phase major cluster merger CIZA J1358.9-4750 , 2015 .
[23] Motohide Kokubun,et al. Hard x-ray imager onboard Hitomi (ASTRO-H) , 2018 .
[24] Shin Mineshige,et al. Supercritical Accretion onto a Non-magnetized Neutron Star: Why is it Feasible? , 2017, 1712.02068.
[25] D. Walton,et al. An ultraluminous X-ray source powered by an accreting neutron star , 2014, Nature.
[26] Kristin K. Madsen,et al. NuSTAR OBSERVATIONS OF THE BULLET CLUSTER: CONSTRAINTS ON INVERSE COMPTON EMISSION , 2014, 1403.2722.
[27] K. Ioka,et al. Can isolated single black holes produce X-ray novae? , 2017, 1704.05047.
[28] Department of Physics,et al. The deeply obscured AGN of NGC4945 I. Spitzer-IRS maps of [Ne V], [Ne II], H2 0-0 S(1), S(2), and other tracers , 2011, 1107.0224.
[29] Shunya Takekawa,et al. SIGNATURE OF AN INTERMEDIATE-MASS BLACK HOLE IN THE CENTRAL MOLECULAR ZONE OF OUR GALAXY , 2015, Proceedings of the International Astronomical Union.
[30] T. Sakamoto,et al. The X-ray counterpart to the gravitational-wave event GW170817 , 2017, Nature.
[31] The Ligo Scientific Collaboration,et al. GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral , 2017, 1710.05832.
[32] William W. Zhang,et al. A broadband x-ray imaging spectroscopy with high-angular resolution: the FORCE mission , 2016, Astronomical Telescopes + Instrumentation.
[33] Teruaki Enoto,et al. Magnetar Broadband X-Ray Spectra Correlated with Magnetic Fields: Suzaku Archive of SGRs and AXPs Combined with NuSTAR, Swift, and RXTE , 2017, 1704.07018.
[34] Yasuhiro Hashimoto,et al. Suzaku Observations of Active Galactic Nuclei Detected in the Swift BAT Survey: Discovery of a “New Type” of Buried Supermassive Black Holes , 2007, 0706.1168.
[35] Fumie Tazaki,et al. SUZAKU OBSERVATIONS OF MODERATELY OBSCURED (COMPTON-THIN) ACTIVE GALACTIC NUCLEI SELECTED BY SWIFT/BAT HARD X-RAY SURVEY , 2016, 1606.04941.
[36] Tomonori Totani,et al. X-ray detectability of accreting isolated black holes in our Galaxy , 2018, 1801.04667.
[37] Yoshiharu Namba,et al. Hard x-ray telescopes to be onboard ASTRO-H. , 2014, Applied optics.