THE SPEAR INSTRUMENT AND ON-ORBIT PERFORMANCE

被引：56

作者：

Edelstein, J. ^{[1
]}

Korpela, E. J. ^{[1
]}

Adolf, J. ^{[1
]}

Bowen, M. ^{[1
]}

Feuerstein, M. ^{[1
]}

Hull, J. ^{[1
]}

Jelinsky, S. ^{[1
]}

Nishikida, K. ^{[1
]}

McKee, K. ^{[1
]}

Berg, P. ^{[1
]}

Chung, R. ^{[1
]}

Fischer, J. ^{[1
]}

Min, K-W ^{[2
]}

Oh, S-H ^{[2
]}

Rhee, J-G ^{[2
]}

Ryu, K. ^{[2
]}

Shinn, J-H ^{[2
]}

Han, W. ^{[3
]}

Jin, H. ^{[3
]}

Lee, D-H ^{[3
]}

Nam, U-W ^{[3
]}

Park, J-H ^{[3
]}

Seon, K-, I ^{[3
]}

Yuk, I. S. ^{[3
]}

机构：

[1] Univ Calif Berkeley, Space Sci Lab, 7 Gauss Way, Berkeley, CA 94720 USA

[2] Korea Adv Inst Sci & Technol KAIST, Dajeon 305701, South Korea

[3] Korea Astron & Space Sci Inst KASI, Dajeon 305348, South Korea

来源：

ASTROPHYSICAL JOURNAL | 2006年 / 644卷 / 02期

关键词：

instrumentation: spectrographs; ultraviolet: ISM;

D O I：

10.1086/505205

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The SPEAR (or "FIMS") instrumentation has been used to conduct the first large-scale spectral mapping of diffuse cosmic far-ultraviolet (FUV; 900-1750 angstrom) emission, including important diagnostics of interstellar hot (10(4)-10(6) K) and photoionized plasmas, H-2, and dust-scattered starlight. The instrumentation's performance has allowed for the unprecedented detection of astrophysical diffuse FUV emission lines. A spectral resolution of lambda/Delta lambda similar to 550 and an imaging resolution of 5' is achieved on-orbit in the Short (900-1150 angstrom) and Long (1350-1750 angstrom) bandpass channels within their respective 4 degrees.0 x 4'.6 and 7 degrees.4 x 4'.3 fields of view. We describe the SPEAR imaging spectrographs, their performance, and the nature and handling of their data.

引用

页码：L159 / L162

页数：4

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