The High-Resolution Spectroscopic Imaging (HSI) Mission

F. A. Harrison; S. E. Boggs; F. E. Christensen; N. Gehrels; J. E. Grindlay; C. M.H. Chen; W. W. Craig; C. J. Hailey; P. Pinto; S. E. Thorsett; J. Tueller; D. Windt; S. E. Woosley

doi:10.1117/12.461280

The High-Resolution Spectroscopic Imaging (HSI) Mission

F. A. Harrison
, S. E. Boggs
, F. E. Christensen
, N. Gehrels
, J. E. Grindlay
, C. M.H. Chen
, W. W. Craig
, C. J. Hailey
, P. Pinto
, S. E. Thorsett
, J. Tueller
, D. Windt
, S. E. Woosley

Research output: Contribution to journal › Conference article › peer-review

4 Scopus citations

Abstract

The High-Resolution Spectroscopic Imaging Mission is designed to be the first instrument to make true images of the hard X-ray/soft gamma-ray (2 - 600 keV) sky. By focusing energetic X-rays and low-energy gamma-rays, HSI will observe the cosmos with an unprecedented combination of sensitivity, spectral resolution, and angular resolving power. HSI is based on an array of multilayer grazing-incidence optics focusing onto high-resolution solid-state germanium pixel detectors with a focal length of 30 - 50 m. This paper describes the primary scientific objectives, technical approach to the instrumentation, and mission design.

Original language	English (US)
Pages (from-to)	345-352
Number of pages	8
Journal	Proceedings of SPIE - The International Society for Optical Engineering
Volume	4851
Issue number	1
DOIs	https://doi.org/10.1117/12.461280
State	Published - 2002
Event	X-ray and Gamma-Ray telescopes and Instruments for Astronomy - Waikoloa, HI, United States Duration: Aug 24 2002 → Aug 28 2002

ASJC Scopus subject areas

Electronic, Optical and Magnetic Materials
Condensed Matter Physics
Computer Science Applications
Applied Mathematics
Electrical and Electronic Engineering

Access to Document

10.1117/12.461280

Cite this

Harrison, F. A., Boggs, S. E., Christensen, F. E., Gehrels, N., Grindlay, J. E., Chen, C. M. H., Craig, W. W., Hailey, C. J., Pinto, P., Thorsett, S. E., Tueller, J., Windt, D., & Woosley, S. E. (2002). The High-Resolution Spectroscopic Imaging (HSI) Mission. Proceedings of SPIE - The International Society for Optical Engineering, 4851(1), 345-352. https://doi.org/10.1117/12.461280

@article{1b68f5a20ece428abfe86d96f158c2c8,

title = "The High-Resolution Spectroscopic Imaging (HSI) Mission",

abstract = "The High-Resolution Spectroscopic Imaging Mission is designed to be the first instrument to make true images of the hard X-ray/soft gamma-ray (2 - 600 keV) sky. By focusing energetic X-rays and low-energy gamma-rays, HSI will observe the cosmos with an unprecedented combination of sensitivity, spectral resolution, and angular resolving power. HSI is based on an array of multilayer grazing-incidence optics focusing onto high-resolution solid-state germanium pixel detectors with a focal length of 30 - 50 m. This paper describes the primary scientific objectives, technical approach to the instrumentation, and mission design.",

author = "Harrison, \{F. A.\} and Boggs, \{S. E.\} and Christensen, \{F. E.\} and N. Gehrels and Grindlay, \{J. E.\} and Chen, \{C. M.H.\} and Craig, \{W. W.\} and Hailey, \{C. J.\} and P. Pinto and Thorsett, \{S. E.\} and J. Tueller and D. Windt and Woosley, \{S. E.\}",

year = "2002",

doi = "10.1117/12.461280",

language = "English (US)",

volume = "4851",

pages = "345--352",

journal = "Proceedings of SPIE - The International Society for Optical Engineering",

issn = "0277-786X",

publisher = "SPIE",

number = "1",

note = "X-ray and Gamma-Ray telescopes and Instruments for Astronomy ; Conference date: 24-08-2002 Through 28-08-2002",

}

TY - JOUR

T1 - The High-Resolution Spectroscopic Imaging (HSI) Mission

AU - Harrison, F. A.

AU - Boggs, S. E.

AU - Christensen, F. E.

AU - Gehrels, N.

AU - Grindlay, J. E.

AU - Chen, C. M.H.

AU - Craig, W. W.

AU - Hailey, C. J.

AU - Pinto, P.

AU - Thorsett, S. E.

AU - Tueller, J.

AU - Windt, D.

AU - Woosley, S. E.

PY - 2002

Y1 - 2002

N2 - The High-Resolution Spectroscopic Imaging Mission is designed to be the first instrument to make true images of the hard X-ray/soft gamma-ray (2 - 600 keV) sky. By focusing energetic X-rays and low-energy gamma-rays, HSI will observe the cosmos with an unprecedented combination of sensitivity, spectral resolution, and angular resolving power. HSI is based on an array of multilayer grazing-incidence optics focusing onto high-resolution solid-state germanium pixel detectors with a focal length of 30 - 50 m. This paper describes the primary scientific objectives, technical approach to the instrumentation, and mission design.

AB - The High-Resolution Spectroscopic Imaging Mission is designed to be the first instrument to make true images of the hard X-ray/soft gamma-ray (2 - 600 keV) sky. By focusing energetic X-rays and low-energy gamma-rays, HSI will observe the cosmos with an unprecedented combination of sensitivity, spectral resolution, and angular resolving power. HSI is based on an array of multilayer grazing-incidence optics focusing onto high-resolution solid-state germanium pixel detectors with a focal length of 30 - 50 m. This paper describes the primary scientific objectives, technical approach to the instrumentation, and mission design.

UR - https://www.scopus.com/pages/publications/0037620252

UR - https://www.scopus.com/pages/publications/0037620252#tab=citedBy

U2 - 10.1117/12.461280

DO - 10.1117/12.461280

M3 - Conference article

AN - SCOPUS:0037620252

SN - 0277-786X

VL - 4851

SP - 345

EP - 352

JO - Proceedings of SPIE - The International Society for Optical Engineering

JF - Proceedings of SPIE - The International Society for Optical Engineering

IS - 1

T2 - X-ray and Gamma-Ray telescopes and Instruments for Astronomy

Y2 - 24 August 2002 through 28 August 2002

ER -

The High-Resolution Spectroscopic Imaging (HSI) Mission

Abstract

ASJC Scopus subject areas

Access to Document

Other files and links

Fingerprint

Cite this