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Guide star catalog for the Spitzer Space Telescope pointing calibration and reference sensor

机译:Spitzer空间望远镜指向校准和参考传感器的指南星目录

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The pointing calibration and reference sensor (PCRS) of the Spitzer Space Telescope (SST) consists of two 4 by 4 pixel visible band detectors plus associated electronics per redundant side. Located in the cryogenic multi instrument chamber of the science telescope system, these detectors, which have a field of view of 40 by 40 arcsec each, define the telescope coordinate frame. Employing guide stars in the range from 7 to 10 magnitude, the PCRS is used, among other things, for measuring the alignment of the active external autonomous star tracker twice per day. To ensure adequate accuracy, the standard radial position error of the guide stars needs to be less than 120 milliarcsec (mas) out to J2009.5. Initial selection of guide star candidates is performed using the Tycho, Tycho-2, Hipparcos, and Tycho Double Star catalogs. To obtain sufficient depth, the 2MASS PSC, USNO A2.0, 2MASS XSC, and PGC catalogs are used for computing the disturbing effect of neighboring objects. In addition, the DSS is employed for determining the perturbing effect of the sky background for each of the guide star candidates. The paper describes the guide star requirements, the methodology used for computing star position error due to neighboring objects and sky background, and the staged development approach that resulted in a ground-based catalog with 196,087 high-quality guide stars for the PCRS.
机译:Spitzer太空望远镜(SST)的定点校准和参考传感器(PCRS)由两个4×4像素可见波段检测器以及每个冗余侧的相关电子设备组成。这些探测器位于科学望远镜系统的低温多仪器室中,每个探测器的视场为40 x 40 arcsec,它们确定了望远镜的坐标系。 PCRS使用7至10级的引导星,除其他外,PCRS每天用于两次测量主动外部自主恒星跟踪仪的对准。为了确保足够的精度,根据J2009.5,导星的标准径向位置误差必须小于120毫秒(质量)。使用Tycho,Tycho-2,Hipparcos和Tycho Double Star目录执行引导星候选者的初始选择。为了获得足够的深度,使用2MASS PSC,USNO A2.0、2MASS XSC和PGC目录来计算相邻对象的干扰效果。此外,DSS用于确定每个导星候选者的天空背景的干扰效果。本文介绍了制导星的要求,用于计算由于邻近物体和天空背景而引起的星位误差的方法,以及分阶段开发的方法,该方法最终形成了基于地面的目录,其中包含用于PCRS的196,087颗优质制星。

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