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

机译:指示校准和参考传感器的Spitzer Space望远镜导牌星目录

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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 Space望远镜(SST)的指向校准和参考传感器(PCR)由两个4×4像素可见带检测器加上每个冗余侧的相关电子。位于科学望远镜系统的低温多仪器室,这些探测器,每个探测器每个都有40×40弧度,定义望远镜坐标框架。在7到10级的范围内采用导游恒星,除其他外,使用PCR,用于测量每天两次活性外部自动星跟踪器的对准。为了确保足够的准确性,导向恒星的标准径向位置误差需要小于120 millarcsec(MAS)到J2009.5。使用Tycho,Tycho-2,Hipparcos和Tycho双星目录进行指南明星候选的初始选择。为了获得足够的深度,2mass PSC,USNO A2.0,2MASS XSC和PGC目录用于计算相邻对象的干扰效果。此外,DSS用于确定每个引导星候选的天空背景的扰动效果。本文介绍的导星要求,用于计算恒星位置误差是由于邻近的对象和天空背景的方法,以及上演,导致基于地面的目录,196087高品质的导航星的PCRS开发方法。

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