Zobrazeno 1 - 10
of 16
pro vyhledávání: '"Daniel Perez-Becker"'
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
Autor:
Daniel Perez-Becker, Eugene Chiang
Short-period exoplanets can have dayside surface temperatures surpassing 2000 K, hot enough to vaporize rock and drive a thermal wind. Small enough planets evaporate completely. We construct a radiative-hydrodynamic model of atmospheric escape from s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2132d45f28251a9323bdcb8dec8b7ebc
Autor:
Adam P. Showman, Daniel Perez-Becker
Infrared lightcurves of transiting hot Jupiters present a trend in which the atmospheres of the hottest planets are less efficient at redistributing the stellar energy absorbed on their daysides---and thus have a larger day-night temperature contrast
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e8e2d7dbc209eb75553afa152791eebe
Autor:
Daniel Perez-Becker, Eugene Chiang
Whether protoplanetary disks accrete at observationally significant rates by the magnetorotational instability (MRI) depends on how well ionized they are. Disk surface layers ionized by stellar X-rays are susceptible to charge neutralization by small
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0dfa0223261f3d22ae60f50d4b787ebc
http://arxiv.org/abs/1104.2320
http://arxiv.org/abs/1104.2320
Autor:
J.-L. Chiu, S. E. Boggs, Mark S. Bandstra, P. von Ballmoos, Wei-Che Hung, Minghuey A. Huang, S. J. Chiang, Paul N. Luke, Jau-Shian Liang, Hsiang-Kuang Chang, Ray-Shine Run, Eric C. Bellm, Mark Amman, P. Jean, Yuan-Hann Chang, Daniel Perez-Becker, Andreas Zoglauer, Chih-Hsun Lin, C. B. Wunderer, Zong-Kai Liu
The Nuclear Compton Telescope (NCT) is a balloon-borne Compton telescope designed for the study of astrophysical sources in the soft gamma-ray regime (200 keV--20 MeV). NCT's ten high-purity germanium crossed-strip detectors measure the deposited ene
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::37c159ca07da73e042c9ba69cc666a41
Autor:
Minghuey A. Huang, C.-H. Lin, Jau-Shian Liang, Mark Amman, Hsiang-Kuang Chang, Ray-Shine Run, Jeng-Lun Chiu, Yuan-Hann Chang, Wei-Che Hung, Daniel Perez-Becker, Mark S. Bandstra, Zhong-Kai Liu, Cornelia B. Wunderer, Eric C. Bellm, Steven E. Boggs, Paul N. Luke, Andreas Zoglauer
Publikováno v:
SPIE Proceedings.
The Nuclear Compton Telescope (NCT) is a balloon-borne telescope designed to study astrophysical sources of gammaray emission with high spectral resolution, moderate angular resolution, and novel sensitivity to gamma-ray polarization. The heart of NC
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a89e661d62845523c6f6540f979d0c24
https://doi.org/10.1117/12.860921
https://doi.org/10.1117/12.860921
Autor:
Yuan-Hann Chang, Wei-Che Hung, Eric C. Bellm, Chih-Hsun Lin, Paul N. Luke, Jeng-Lun Chiu, Andreas Zoglauer, Jau-Shian Liang, Minghuey A. Huang, Mark S. Bandstra, Pierre Jean, Mark Amman, Ray-Shine Run, Daniel Perez-Becker, Steven E. Boggs, Hsiang-Kuang Chang, Zhong-Kai Liu
Publikováno v:
Space Telescopes and Instrumentation 2010: Ultraviolet to Gamma Ray.
The Nuclear Compton Telescope (NCT) is a balloon-borne soft gamma-ray telescope. Its compact design uses cross-strip germanium detectors, allowing for wide-field imaging with excellent efficiency from 0.2-10 MeV. Additionally, the Compton imaging pri
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::90099290d45fcc58bf1795a27fa6057b
https://doi.org/10.1117/12.857526
https://doi.org/10.1117/12.857526
Autor:
Wei-Che Hung, Zhong-Kai Liu, Daniel Perez-Becker, Jeng-Lun Chiu, Chih-Hsun Lin, Ray-Shine Run, Shiuan-Juang Chiang, Mark Amman, Jau-Shian Liang, Yuan-Hann Chang, Mark S. Bandstra, Minghuey A. Huang, Hsiang-Kuang Chang, Eric C. Bellm, Steven E. Boggs, Cornelia B. Wunderer, Andreas Zoglauer, Paul N. Luke
Publikováno v:
Space Telescopes and Instrumentation 2010: Ultraviolet to Gamma Ray.
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_________::c7ed786edea0bf85a9fb9d5c40e2ad34
https://doi.org/10.1117/12.857876
https://doi.org/10.1117/12.857876