Zobrazeno 1 - 10
of 42
pro vyhledávání: '"Jeng-Lun Chiu"'
Autor:
Hung-Hsiang Liang, Yi-Chi Chang, Hsiang-Yue, Jerome Rodriguez, Jeng-Lun Chiu, Chien-Ying Yang, Philippe Laurent, Che-Yen Chu, Chih-Hsun Lin, Hsiang-Kuang Chang
Publikováno v:
Astron.J.
Astron.J., 2020, 160 (1), pp.54. ⟨10.3847/1538-3881/ab9caf⟩
Astron.J., 2020, 160 (1), pp.54. ⟨10.3847/1538-3881/ab9caf⟩
Instruments flown on CubeSats are small. Meaningful applications of CubeSats in astronomical observations rely on the choice of a particular subject that is feasible for CubeSats. Here we report the result of a feasibility study for observing gamma-r
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c39abedd5ea2124796b99fe7c39c6446
https://hal.science/hal-02416913
https://hal.science/hal-02416913
Autor:
Chien-Ying Yang, C.-H. Lin, Jeng-Lun Chiu, B. Mochizuki, P. von Ballmoos, Andreas Zoglauer, Hsiang-Kuang Chang, Y.-C. Chang, John A. Tomsick, P. Jean, C. Sleator, A. Lowell, Mark Amman, S. E. Boggs, H.-H. Liang, Che-Yen Chu, S. McBride, Carolyn Kierans
Publikováno v:
Space Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray.
The Compton Spectrometer and Imager (COSI) is a compact Compton telescope which is inherently sensitive to gamma-ray polarization in the energy range of 0.2-2.0 MeV. A long duration gamma-ray burst, GRB 160530A, was detected by COSI during its 2016 C
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e3e33b2cdd58668df5774d0dd287585d
https://doi.org/10.1117/12.2312556
https://doi.org/10.1117/12.2312556
Autor:
Maïca Clavel, Dominic J. Walton, Victoria Grinberg, Felix Fürst, John A. Tomsick, Jon M. Miller, Javier A. García, Katja Pottschmidt, Poshak Gandhi, Michael Parker, Jeng-Lun Chiu, Didier Barret, Andrew C. Fabian, Kazutaka Yamaoka
Publikováno v:
Astrophys.J.
Astrophys.J., 2018, 855 (1), pp.3. ⟨10.3847/1538-4357/aaaab1⟩
NASA Astrophysics Data System
Astrophys.J., 2018, 855 (1), pp.3. 〈10.3847/1538-4357/aaaab1〉
Astrophys.J., 2018, 855 (1), pp.3. ⟨10.3847/1538-4357/aaaab1⟩
NASA Astrophysics Data System
Astrophys.J., 2018, 855 (1), pp.3. 〈10.3847/1538-4357/aaaab1〉
Here we study a 1-200 keV energy spectrum of the black hole binary Cygnus X-1 taken with NuSTAR and Suzaku. This is the first report of a NuSTAR observation of Cyg X-1 in the intermediate state, and the observation was taken during the part of the bi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bebaf7e4d853943a66a41f8867b6c33d
https://resolver.caltech.edu/CaltechAUTHORS:20180227-133907106
https://resolver.caltech.edu/CaltechAUTHORS:20180227-133907106
Autor:
Alex Lowell, Andreas Zoglauer, Carolyn Kierans, Hsiang-Kuang Chang, P. von Ballmoos, Steven E. Boggs, Y. H. Chang, J.-R. Shang, C.-H. Lin, Mark Amman, Chien-Ying Yang, Chih-Kuo Tseng, Yi Chou, John A. Tomsick, Jeng-Lun Chiu, Pierre Jean
Publikováno v:
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment. 784:359-363
The Compton Spectrometer and Imager (COSI), formerly known as the Nuclear Compton Telescope (NCT), is a balloon-borne soft gamma-ray telescope (0.2–5 MeV) designed to study astrophysical sources of nuclear-line emission and gamma-ray polarization.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e0b069fbd15b94a5fee4b99e7407544d
https://doi.org/10.1016/j.nima.2014.11.099
https://doi.org/10.1016/j.nima.2014.11.099
Autor:
Chih-Hsun Lin, Clio Sleator, Pierre Jean, Jeng-Lun Chiu, Peter von Ballmoos, Chao-Hsiung Tseng, Andreas Zoglauer, Mark Amman, Chien-Ying Yang, Steven E. Boggs, Carolyn Kierans, Hsiang-Kuang Chang, John A. Tomsick, Che-Yen Chu, Alex Lowell
Publikováno v:
PoS
35th International Cosmic Ray Conference
35th International Cosmic Ray Conference, Jul 2017, Busan, South Korea. pp.796, ⟨10.22323/1.301.0796⟩
35th International Cosmic Ray Conference
35th International Cosmic Ray Conference, Jul 2017, Busan, South Korea. pp.796, ⟨10.22323/1.301.0796⟩
International audience; The Compton Spectrometer and Imager (COSI) is a balloon-borne, soft gamma-ray (0.2-5 MeV) telescope designed to study astrophysical sources of nuclear-line emission and gamma-ray polarization. The heart of COSI is a compact ar
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::245523993e45de54ed6e148afd7964c6
https://hal.archives-ouvertes.fr/hal-01890897
https://hal.archives-ouvertes.fr/hal-01890897
Autor:
Carolyn Kierans, Pierre Jean, P. vonBallmoos, Steven E. Boggs, Mark Amman, Clio Sleator, Chao-Hsiung Tseng, Hsiang-Kuang Chang, Chih-Hsun Lin, Jeng-Lun Chiu, Chien-Ying Yang, John A. Tomsick, Andreas Zoglauer, Alex Lowell
The Compton Spectrometer and Imager (COSI) is a balloon-borne gamma-ray (0.2-5 MeV) telescope with inherent sensitivity to polarization. COSI's main goal is to study astrophysical sources such as $\gamma$-ray bursts, positron annihilation, Galactic n
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::96978ee8e8763daecd7ec1932c5d9752
http://arxiv.org/abs/1701.05563
http://arxiv.org/abs/1701.05563
Autor:
Alex Lowell, Chien-Ying Yang, Pierre Jean, Chao-Hsiung Tseng, Carolyn Kierans, Mark Amman, Chih-Hsun Lin, Clio Sleator, Hsiang-Kuang Chang, Peter von Ballmoos, John A. Tomsick, Andreas Zoglauer, Steven E. Boggs, Jeng-Lun Chiu
The Compton Spectrometer and Imager (COSI) is a balloon-borne, soft-gamma ray imager, spectrometer, and polarimeter with sensitivity from 0.2 to 5 MeV. Utilizing a compact Compton telescope design with twelve cross-strip, high-purity germanium detect
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cc5b275eba1d5b1666cad5f80431b610
http://arxiv.org/abs/1701.05558
http://arxiv.org/abs/1701.05558
Autor:
Ming-Huey Huang, S. E. Boggs, Chih-Hsun Lin, Paul N. Luke, Hsiang-Kuang Chang, Yuan-Hann Chang, Zong-Kai Liu, Mark Amman, Jau-Shian Liang, Eric C. Bellm, Jeng-Lun Chiu, Mark S. Bandstra, Andreas Zoglauer, C. B. Wunderer, Daniel Perez-Becker, Wei-Che Hung
Publikováno v:
IEEE Transactions on Nuclear Science. 56:2303-2308
The Nuclear Compton Telescope (NCT) is a balloon-borne telescope based on the 3D-positioning germanium detectors. It is designed to study astrophysical sources of gamma-ray emission in the energy range of 0.2 MeV to 10 MeV. The data readout system of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b277d65e8644b1f1d7fe66f644a24856
https://doi.org/10.1109/tns.2009.2022624
https://doi.org/10.1109/tns.2009.2022624
Autor:
Minghuey A. Huang, Wei-Che Hung, Pierre Jean, Mark S. Bandstra, Mark Amman, Eric C. Bellm, Hsiang-Kuang Chang, Steven E. Boggs, Jau-Shian Liang, Daniel Perez-Becker, Zong-Kai Liu, Yuan-Hann Chang, J.D. Bowen, Andreas Zoglauer, C. B. Wunderer, Jeng-Lun Chiu, Chih-Hsun Lin, Paul N. Luke
Publikováno v:
IEEE Transactions on Nuclear Science. 56:1250-1256
The Nuclear Compton Telescope (NCT) is a balloon-borne telescope designed to study astrophysical sources of nuclear line emission and polarization at soft gamma-ray (0.2-10 MeV) energies. NCT uses high-purity germanium strip detectors for 3D tracking
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::73d286c08770b4c4ec71f7198266239d
https://doi.org/10.1109/tns.2009.2016091
https://doi.org/10.1109/tns.2009.2016091
Autor:
Yuan-Hann Chang, Paul N. Luke, Eric C. Bellm, Wei-Che Hung, Mark Amman, Chih-Hsun Lin, Jau-Shian Liang, S. E. Boggs, Daniel Perez-Becker, Zong-Kai Liu, J.D. Bowen, Mark S. Bandstra, Cornelia B. Wunderer, Jeng-Lun Chiu, Hsiang-Kuang Chang, Andreas Zoglauer
Publikováno v:
IEEE Transactions on Nuclear Science. 56:1210-1214
The Nuclear Compton Telescope (NCT) is a balloon-borne soft gamma ray (0.2-10 MeV) telescope designed to study astrophysical sources of nuclear line emission and polarization. The heart of NCT is an array of 12 cross-strip germanium detectors, design
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ee1ec38c6ee25399f1b196f76cbbf91b
https://doi.org/10.1109/tns.2009.2012857
https://doi.org/10.1109/tns.2009.2012857