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The photodetector array camera and spectrometer (PACS) for the Herschel Space Observatory

机译:光电探测器阵列相机和光谱仪(PACS),用于Herschel Space天文台

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The Photodetector Array Camera and Spectrometer (PACS) is one of the three science instruments for ESA's far infrared and submillimetre observatory, Herschel. It employs two Ge:Ga photoconductor arrays (stressed and unstressed) with 16 x 25 pixels, each, and two filled Si bolometer arrays with 16 x 32 and 32 x 64 pixels, respectively, to perform imaging line spectroscopy and imaging photometry in the 57-210 micron wavelength band. In photometry mode, it will simultaneously image two bands, 60-85 micron or 85-130 micron and 130-210 micron, over a field of view of ~ 1.75'x3.5', with full beam sampling in each band. In spectroscopy mode, it will image a field of ~ 50"x50", resolved into 5 x 5 pixels, with an instantaneous spectral coverage of ~ 1500 km/s and a spectral resolution of ~ 75 - 300 km/s. In both modes background-noise limited peformance is expected, with sensitivities (5σ in 1h) of ~3 mJy or 3-10x10-18 W/m2, respectively.
机译:光电探测器阵列摄像头和光谱仪(PACS)是ESA远红外线和亚瑟伊斯氏郡观测台的三种科学仪器之一。它采用两种GE:GA光电导体阵列(应力和不受重音),分别具有16×25像素,每个填充的SI钻头阵列,分别具有16×32和32×64像素,在57中执行成像线光谱和成像光度测量-210微米波长带。在光度测定模式中,它将同时以〜1.75'x3.5'的视野相同图像,在〜1.75'x3.5'的视野上,在每个频段中采样全光束采样。在光谱模式下,它将图像〜50“X50”的字段,分离成5×5像素,瞬时光谱覆盖率为约1500 km / s,光谱分辨率为约75-300 km / s。在两种模式中,期望背景噪声限制性的PEFormance,敏感性(5σ,1h)分别为3米或3-10x10-18 w / m2。

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