ISOPHOT-S: Capabilities and calibration

被引：0

作者：

Klaas, U ^{[1
]}

Acosta-Pulido, JA ^{[1
]}

Abraham, P ^{[1
]}

Castaneda, HO ^{[1
]}

Cornwall, L ^{[1
]}

Garzon, F ^{[1
]}

Hammersley, P ^{[1
]}

Heinrichsen, I ^{[1
]}

Kinkel, U ^{[1
]}

Lemke, D ^{[1
]}

Schubert, J ^{[1
]}

Wells, M ^{[1
]}

机构：

[1] Max Planck Inst Astron, D-69117 Heidelberg, Germany

来源：

FIRST ISO WORKSHOP ON ANALYTICAL SPECTROSCOPY: WITH SWS, LWS, PHT-S, AND CAM-CVF | 1997年 / 419卷

关键词：

space vehicles; instrumentation; spectrographs; methods; data analysis; techniques; spectroscopic;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The in-flight characteristics of ISOPHOT-S are presented, in particular spectral response function, beam profile, dark current, straylight suppression, and wavelength calibration. Photometric calibration of point-like and extended sources is described. Sensitivity limits and the actual error budget are discussed. The validation of the pipeline products is addressed. Correction methods for signal transients in staring and chopped mode are outlined.

引用

页码：113 / 118

页数：6

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