• For astrometric purposes, dark frame and flat field calibration is recommended.

    出于天文测量要求,暗场图和平场图校准是被推荐的。

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  • Astrometric Limit: The maximum residual in the place of a reference star, specified in arc seconds.

    天文测量误差极限:参考星位置对应的最大误差,用角秒表示。

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  • The accuracy of the future international celestial reference frame obtained from astrometric satellites: SIM and GAIA are given.

    介绍由天体测量卫星GAIA和SIM给出的天球参考架可能逵到的精度。

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  • If you save the images after astrometric data reduction has been performed, the software will add WCS keywords to the FITS header.

    如果你的图片经过天文测量数据分类转换后储存,本软件将在FITS文件头部分添加wcs关键词。

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  • Some ordinary forms of sparse matrix and the application of sparse matrix technology in astrometric and geodetic VLBI data analysis are introduced.

    介绍了稀疏矩阵的四种常见形式以及稀疏矩阵技术在天测与测地VLBI数据处理中的应用。

    youdao

  • Pressing the [OK] button will start the astrometric data reduction process. After a while, colored circles will be drawn around the objects detected by the software.

    点OK后,天文数据分类将会开始,过一会儿,软件识别后的结果就会以彩色圈的形式显示出来。

    youdao

  • The Problem of astrometric photometry is discussed in this paper. The photometric capabilities on both the ground-based astrometric instruments and space telescopes are presented.

    讨论有关天体测量中的测光问题,介绍一些地面天体测量仪器和空间天体测量望远镜的测光研究。

    youdao

  • The Problem of astrometric photometry is discussed in this paper. The photometric capabilities on both the ground-based astrometric instruments and space telescopes are presented.

    讨论有关天体测量中的测光问题,介绍一些地面天体测量仪器和空间天体测量望远镜的测光研究。

    youdao

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