Calibration and performance of the LWS

被引:4
作者
Burgdorf, MJ
Caux, E
Clegg, PE
Davis, GR
Emery, RJ
Ewart, JD
Griffin, MJ
Gry, C
Harwood, AS
King, KJ
Lim, T
Lord, S
Molinari, S
Swinyard, BM
Texier, D
Tommasi, E
Trams, N
Unger, SJ
机构
[1] ESA, Div Astrophys, Sci Operat Ctr, ISO, E-28080 Madrid, Spain
[2] Ctr Etud Spatiale Rayonnements, F-31029 Toulouse, France
[3] Univ London Queen Mary & Westfield Coll, London E1 4NS, England
[4] Univ Saskatchewan, Inst Space & Atmospher Studies, Saskatoon, SK S7N 5E2, Canada
[5] Rutherford Appleton Lab, Didcot OX11 0QX, Oxon, England
[6] Lab Astrophys Spatiale, F-13376 Marseille, France
[7] CALTECH, IPAC, Pasadena, CA 91125 USA
[8] CNR, Ist Fis Spazio Interplanetario, I-00044 Frascati, Italy
来源
SPACE BASED ASTRONOMY: ISO, AGN, RADIOPULSARS AND THE SUN | 1998年 / 21卷 / 1-2期
关键词
D O I
10.1016/S0273-1177(97)00825-9
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
The status of calibration and performance of the ISO Long-Wavelength Spectrometer eleven months after launch is described. The strategy followed for the calibration observations and first results are summarized. The overall performance of the instrument essentially fulfills the expectations; certain changes in sensitivity of the detectors are reported. Some improvements in the way observations are executed, which resulted from the in-flight experience, are explained. (C)1998 COSPAR. Published by Elsevier Science Ltd.
引用
收藏
页码:5 / 9
页数:5
相关论文
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Clegg PE, 1996, ASTRON ASTROPHYS, V315, pL38
[2]  
DELETTREZ C, 1994, EXPT ASTRONOMY, V4, P213
[3]  
Kessler MF, 1996, ASTRON ASTROPHYS, V315, pL27
[4]  
Swinyard BM, 1996, ASTRON ASTROPHYS, V315, pL43