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首页> 外文期刊>The Astrophysical journal >THE PPMXL CATALOG OF POSITIONS AND PROPER MOTIONS ON THE ICRS. COMBINING USNO-B1.0 AND THE TWO MICRON ALL SKY SURVEY (2MASS)
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THE PPMXL CATALOG OF POSITIONS AND PROPER MOTIONS ON THE ICRS. COMBINING USNO-B1.0 AND THE TWO MICRON ALL SKY SURVEY (2MASS)

机译:ICRS上PPMXL的位置和正确动作目录。结合USNO-B1.0和两个MICRON ALL SKY调查(2质量)

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摘要

USNO-B1.0 and the Two Micron All Sky Survey (2MASS) are the most widely used all-sky surveys. However, 2MASS has no proper motions at all, and USNO-B1.0 published only relative, not absolute (i.e., on the International Celestial Reference Frame (ICRS), proper motions. We performed a new determination of mean positions and proper motions on the ICRS system by combining USNO-B1.0 and 2MASS astrometry. This catalog is called PPMXL (VO access to the catalog is possible via http://vo.uni-hd.de/ppmxl), and it aims to be completed from the brightest stars down to about V ≈ 20 all sky. PPMXL contains about 900 million objects, some 410 million with 2MASS photometry, and is the largest collection of ICRS proper motions at present. As representative for the ICRS, we chose PPMX. The recently released UCAC3 could not be used because we found plate-dependent distortions in its proper motion system north of –20° declination. UCAC3 served as an intermediate system for δ ≤ –20°. The resulting typical individual mean errors of the proper motions range from 4?mas?yr–1 to more than 10?mas?yr–1 depending on observational history. The mean errors of positions at epoch 2000.0 are 80-120?mas, if 2MASS astrometry could be used, 150-300?mas else. We also give correction tables to convert USNO-B1.0 observations of, e.g., minor planets to the ICRS system.
机译:USNO-B1.0和“两微米全天候测量”(2MASS)是使用最广泛的全天候测量。但是,2MASS根本没有适当的运动,而USNO-B1.0仅发布了相对的,而不是绝对的(即,在国际天文参考系(ICRS)上,是适当的运动。)结合USNO-B1.0和2MASS占星术的ICRS系统,该目录称为PPMXL(可以通过http://vo.uni-hd.de/ppmxl进入VO目录),其目标是从PPMXL包含约9亿个物体,其中约4.1亿个通过2MASS光度法测量,是目前ICRS正常运动的最大集合,作为ICRS的代表,我们选择了PPMX。释放的UCAC3无法使用,因为我们发现其固有运动在–20°偏北以北与板块有关的变形; UCAC3作为δ≤–20°的中间系统。 4?mas?yr–1到10?mas?yr–1 de等待观察历史。如果可以使用2MASS占星术,则在2000.0时代的平均位置误差为80-120 mas,否则为150-300 mas。我们还提供了校正表,以将例如小行星的USNO-B1.0观测值转换为ICRS系统。

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