The spring 2009 balloon flight of the nuclear compton telescope

Mark S. Bandstra; Eric C. Bellm; Jeng Lun Chiu; Jau Shian Liang; Zong Kai Liu; Daniel Perez-Becker; Andreas Zoglauer; Steven E. Boggs; Hsiang Kuang Chang; Yuan Hann Chang; Ming Huey A. Huang; Mark Amman; Shiuan Juang Chiang; Wei Che Hung; Pierre Jean; Chih Hsun Lin; Paul N. Luke; Ray Shine Run; Cornelia B. Wunderer

doi:10.1109/NSSMIC.2009.5402108

The spring 2009 balloon flight of the nuclear compton telescope

Mark S. Bandstra, Eric C. Bellm, Jeng Lun Chiu, Jau Shian Liang, Zong Kai Liu, Daniel Perez-Becker, Andreas Zoglauer, Steven E. Boggs, Hsiang Kuang Chang, Yuan Hann Chang, Ming Huey A. Huang, Mark Amman, Shiuan Juang Chiang, Wei Che Hung, Pierre Jean, Chih Hsun Lin, Paul N. Luke, Ray Shine Run, Cornelia B. Wunderer

研究成果: 書貢獻/報告類型 › 會議論文篇章 › 同行評審

7 引文斯高帕斯（Scopus）

摘要

The Nuclear Compton Telescope (NCT) is a balloonborne soft gamma-ray (0.2-10 MeV) telescope designed to study astrophysical sources of nuclear line emission and polarization. NCT consists of twelve high-purity germanium cross-strip detectors (GeDs) that measure both the position and energy of gamma-ray interactions. A 10-GeD version was flown on May 17-18 2009 from the Columbia Scientific Balloon Facility in Fort Sumner, NM, with a total flight duration of 38.5 hours. Here we summarize the instrument, the calibrations, the flight, and our preliminary science results.

原文	???core.languages.en_GB???
主出版物標題	2009 IEEE Nuclear Science Symposium Conference Record, NSS/MIC 2009
頁面	2131-2139
頁數	9
DOIs	https://doi.org/10.1109/NSSMIC.2009.5402108
出版狀態	已出版 - 2009
事件	2009 IEEE Nuclear Science Symposium Conference Record, NSS/MIC 2009 - Orlando, FL, United States 持續時間: 25 10月 2009 → 31 10月 2009

出版系列

名字	IEEE Nuclear Science Symposium Conference Record
ISSN（列印）	1095-7863

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???event.eventtypes.event.conference???	2009 IEEE Nuclear Science Symposium Conference Record, NSS/MIC 2009
國家/地區	United States
城市	Orlando, FL
期間	25/10/09 → 31/10/09

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10.1109/NSSMIC.2009.5402108

引用此

Bandstra, M. S., Bellm, E. C., Chiu, J. L., Liang, J. S., Liu, Z. K., Perez-Becker, D., Zoglauer, A., Boggs, S. E., Chang, H. K., Chang, Y. H., Huang, M. H. A., Amman, M., Chiang, S. J., Hung, W. C., Jean, P., Lin, C. H., Luke, P. N., Run, R. S., & Wunderer, C. B. (2009). The spring 2009 balloon flight of the nuclear compton telescope. 於 2009 IEEE Nuclear Science Symposium Conference Record, NSS/MIC 2009 (頁 2131-2139). 文章 5402108 (IEEE Nuclear Science Symposium Conference Record). https://doi.org/10.1109/NSSMIC.2009.5402108

@inproceedings{57de1514c16c4b43a97e828790bb4d29,

title = "The spring 2009 balloon flight of the nuclear compton telescope",

abstract = "The Nuclear Compton Telescope (NCT) is a balloonborne soft gamma-ray (0.2-10 MeV) telescope designed to study astrophysical sources of nuclear line emission and polarization. NCT consists of twelve high-purity germanium cross-strip detectors (GeDs) that measure both the position and energy of gamma-ray interactions. A 10-GeD version was flown on May 17-18 2009 from the Columbia Scientific Balloon Facility in Fort Sumner, NM, with a total flight duration of 38.5 hours. Here we summarize the instrument, the calibrations, the flight, and our preliminary science results.",

keywords = "Compton imaging, Gamma-ray astronomy detectors, Gamma-ray imaging, Germanium detectors",

author = "Bandstra, {Mark S.} and Bellm, {Eric C.} and Chiu, {Jeng Lun} and Liang, {Jau Shian} and Liu, {Zong Kai} and Daniel Perez-Becker and Andreas Zoglauer and Boggs, {Steven E.} and Chang, {Hsiang Kuang} and Chang, {Yuan Hann} and Huang, {Ming Huey A.} and Mark Amman and Chiang, {Shiuan Juang} and Hung, {Wei Che} and Pierre Jean and Lin, {Chih Hsun} and Luke, {Paul N.} and Run, {Ray Shine} and Wunderer, {Cornelia B.}",

year = "2009",

doi = "10.1109/NSSMIC.2009.5402108",

language = "???core.languages.en_GB???",

isbn = "9781424439621",

series = "IEEE Nuclear Science Symposium Conference Record",

pages = "2131--2139",

booktitle = "2009 IEEE Nuclear Science Symposium Conference Record, NSS/MIC 2009",

note = "2009 IEEE Nuclear Science Symposium Conference Record, NSS/MIC 2009 ; Conference date: 25-10-2009 Through 31-10-2009",

}

Bandstra, MS, Bellm, EC, Chiu, JL, Liang, JS, Liu, ZK, Perez-Becker, D, Zoglauer, A, Boggs, SE, Chang, HK, Chang, YH, Huang, MHA, Amman, M, Chiang, SJ, Hung, WC, Jean, P, Lin, CH, Luke, PN, Run, RS & Wunderer, CB 2009, The spring 2009 balloon flight of the nuclear compton telescope. 於 2009 IEEE Nuclear Science Symposium Conference Record, NSS/MIC 2009., 5402108, IEEE Nuclear Science Symposium Conference Record, 頁 2131-2139, 2009 IEEE Nuclear Science Symposium Conference Record, NSS/MIC 2009, Orlando, FL, United States, 25/10/09. https://doi.org/10.1109/NSSMIC.2009.5402108

TY - GEN

T1 - The spring 2009 balloon flight of the nuclear compton telescope

AU - Bandstra, Mark S.

AU - Bellm, Eric C.

AU - Chiu, Jeng Lun

AU - Liang, Jau Shian

AU - Liu, Zong Kai

AU - Perez-Becker, Daniel

AU - Zoglauer, Andreas

AU - Boggs, Steven E.

AU - Chang, Hsiang Kuang

AU - Chang, Yuan Hann

AU - Huang, Ming Huey A.

AU - Amman, Mark

AU - Chiang, Shiuan Juang

AU - Hung, Wei Che

AU - Jean, Pierre

AU - Lin, Chih Hsun

AU - Luke, Paul N.

AU - Run, Ray Shine

AU - Wunderer, Cornelia B.

PY - 2009

Y1 - 2009

N2 - The Nuclear Compton Telescope (NCT) is a balloonborne soft gamma-ray (0.2-10 MeV) telescope designed to study astrophysical sources of nuclear line emission and polarization. NCT consists of twelve high-purity germanium cross-strip detectors (GeDs) that measure both the position and energy of gamma-ray interactions. A 10-GeD version was flown on May 17-18 2009 from the Columbia Scientific Balloon Facility in Fort Sumner, NM, with a total flight duration of 38.5 hours. Here we summarize the instrument, the calibrations, the flight, and our preliminary science results.

AB - The Nuclear Compton Telescope (NCT) is a balloonborne soft gamma-ray (0.2-10 MeV) telescope designed to study astrophysical sources of nuclear line emission and polarization. NCT consists of twelve high-purity germanium cross-strip detectors (GeDs) that measure both the position and energy of gamma-ray interactions. A 10-GeD version was flown on May 17-18 2009 from the Columbia Scientific Balloon Facility in Fort Sumner, NM, with a total flight duration of 38.5 hours. Here we summarize the instrument, the calibrations, the flight, and our preliminary science results.

KW - Compton imaging

KW - Gamma-ray astronomy detectors

KW - Gamma-ray imaging

KW - Germanium detectors

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M3 - 會議論文篇章

AN - SCOPUS:77951186567

SN - 9781424439621

T3 - IEEE Nuclear Science Symposium Conference Record

SP - 2131

EP - 2139

BT - 2009 IEEE Nuclear Science Symposium Conference Record, NSS/MIC 2009

T2 - 2009 IEEE Nuclear Science Symposium Conference Record, NSS/MIC 2009

Y2 - 25 October 2009 through 31 October 2009

ER -

The spring 2009 balloon flight of the nuclear compton telescope

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