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InfraRed Standards Used for SpectrophotometricCalibration — Application to the Medium ResolutionSpectrometer of MIRI

机译:用于分光光度法的红外标准 - 应用于Miri的介质分辨率

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One of the main ingredients in establishing the relation betweeninput signal and output flux from a spectrometer, is the accurate determinationof the spectrophotometric calibration. In case of spectrometers onboard satel-lites, the accuracy of this part of the calibration pedigree is ultimately linkedto the reliability of the candidate calibrators as being fiducial. In this contribu-tion, we deal with the spectrophotometric calibration of infrared spectrometersin the 2-200 pm wavelength range. We outline a general selection procedure toarrive at a set of fiducial IR calibrators, and apply the method to the MediumResolution Spectrometer of MIRI which will be onboard the James Webb SpaceTelescope.
机译:在从光谱仪建立信号和输出通量之间建立关系的主要成分之一,是分光光度校准的准确确定。在Spel-Lites上的光谱仪的情况下,校准谱系的这一部分的精度最终将候选校准器的可靠性联系在于基准。在这方面,我们处理红外光谱仪的分光光度校准2-200pm波长范围。我们概述了一组基准IR校准器的一般选择程序,并将该方法应用于Miri的中型频谱仪,这将是詹姆斯韦布斯·斯普法普克斯库普。

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