MISC

2009年

GRB Polarimetry with POET

GAMMA-RAY BUSTS
  • M. L. McConnell
  • L. Angelini
  • M. G. Baring
  • S. Barthelmy
  • J. K. Black
  • P. F. Bloser
  • B. Dennis
  • A. G. Emslie
  • J. Greiner
  • W. Hajdas
  • A. K. Harding
  • D. H. Hartmann
  • J. E. Hill
  • K. Ioka
  • P. Kaaret
  • G. Kanbach
  • D. Kniffen
  • J. S. Legere
  • J. R. Macri
  • R. Morris
  • T. Nakamura
  • N. Produit
  • J. M. Ryan
  • T. Sakamoto
  • K. Toma
  • X. Wu
  • R. Yamazaki
  • B. Zhang
  • 全て表示

1133
開始ページ
64
終了ページ
+
記述言語
英語
掲載種別
DOI
10.1063/1.3155969
出版者・発行元
AMER INST PHYSICS

POET (Polarimeters for Energetic Transients) represents a concept for a Small Explorer (SMEX) satellite mission, whose principal scientific goal is to understand the structure of GRB sources through sensitive X-ray and gamma-ray polarization measurements. The payload consists of two wide field-of-view (FoV) instruments: a Low Energy Polarimeter (LEP) capable of polarization measurements in the energy range from 2-15 keV and a high energy polarimeter (Gamma-Ray Polarimeter Experiment or GRAPE) that would measure polarization in the 60-500 keV energy range. The POET spacecraft provides a zenith-pointed platform for maximizing the exposure to deep space. Spacecraft rotation provides a means of effectively dealing with any residual systematic effects in the polarization response. POET provides sufficient sensitivity and sky coverage to measure statistically significant polarization (for polarization levels in excess of 20%) for similar to 80 GRBs in a two-year mission. High energy polarization data would also be obtained for SGRs, solar flares, pulsars and other sources of astronomical interest.

リンク情報
DOI
https://doi.org/10.1063/1.3155969
Web of Science
https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=JSTA_CEL&SrcApp=J_Gate_JST&DestLinkType=FullRecord&KeyUT=WOS:000267717300017&DestApp=WOS_CPL
URL
https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=70450170550&origin=inward
ID情報
  • DOI : 10.1063/1.3155969
  • ISSN : 0094-243X
  • SCOPUS ID : 70450170550
  • Web of Science ID : WOS:000267717300017

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