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On-orbit sky background measurements Faint Object Spectrograph

机译:在轨天空背景测量微弱物体光谱仪

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Abstract: Observations of the sky background obtained with the Faint Object Spectrograph during 1991 - 1992 are discussed. Sky light can be an important contributor to the observed count rate in several of the instrument configurations especially when large apertures are used. In general, the sky background is consistent with the pre-launch expectations and showed the expected effects of zodiacal light and diffuse galactic light. In addition to these sources, there is, particularly during the daytime, a highly variable airglow component which includes a number of emission lines. The sky background will have an impact on the reduction and possibly the interpretation of some spectra.!11
机译:摘要:讨论了1991年至1992年使用微弱物体光谱仪获得的天空背景观测结果。在某些仪器配置中,尤其是使用大光圈时,天光可能是导致观察到的计数率的重要因素。通常,天空背景与发射前的预期一致,并显示了黄道光和银河漫射光的预期效果。除这些来源外,尤其是在白天,还存在高度可变的气辉成分,其中包括许多排放管线。天空背景会影响光谱的减少,甚至可能影响某些光谱的解释。!11

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