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Guo Bifeng, Peng Qingyu, Lin Furong. Applications and Technology Research for Astrometrica and MaxIm DL in Astrometry[J]. Astronomical Research and Technology, 2021, 18(2): 195-202. DOI: 10.14005/j.cnki.issn1672-7673.20200701.001
Citation: Guo Bifeng, Peng Qingyu, Lin Furong. Applications and Technology Research for Astrometrica and MaxIm DL in Astrometry[J]. Astronomical Research and Technology, 2021, 18(2): 195-202. DOI: 10.14005/j.cnki.issn1672-7673.20200701.001

Applications and Technology Research for Astrometrica and MaxIm DL in Astrometry

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  • Received Date: May 26, 2020
  • Revised Date: June 20, 2020
  • Available Online: November 20, 2023
  • In order to explore the difference of Astrometrica and MaxIm DL for application and CCD image processing in Astrometry, overall introduction, loading, saving and transforming CCD images, flat calibration, data reduction and stacking of the two suites of software are detailedly compared and technically researched in this paper. Taking the example of two sets of observations of M35 Cluster photographed by the 1 m optical telescope of Yunnan Observatories of Chinese Academy of Sciences, this paper explores the output results of the 6 stacking methods including Mean, Median of Astrometrica and Mean, Median, Sigma Clip and SD Mask of MaxIm DL. Referring to Gaia DR2 Catalog, this paper reduces the 6 output results above and compares their precision of the star images. In this paper, we find anomalies in the position accuracy of the output images using Astrometrica's Median stacking. At the end of this paper, we put forward some methods of using the two suites software in combination for astrometry and survey.
  • [1]
    RAAB H. Astrometrica software[CP/OL].[2020-05-27]. http://www.astrometrica.at.
    [2]
    Diffraction Limited. MaxIm DL software[CP/OL].[2020-05-27]. https://diffractionlimited.com/product/maxim-dl.
    [3]
    孙浩民, 邓辉, 梅盈, 等. 基于Python-casacore的射电测量集文件生成方法[J]. 天文研究与技术, 2020, 17(2):210-216.

    SUN H M, DENG H, MEI Y, et al. Measurement Set file generating method based on Python-casacore[J]. Astronomical Research & Technology, 2020, 17(2):210-216.
    [4]
    张珊瑚, 邱丹, 聂嘉潞, 等. 基于MATLAB的一维光谱可视化与分析工具的设计与实现[J]. 天文研究与技术, 2020, 17(1):121-128.

    ZHANG S H, QIU D, NIE J L, et al. Design and implementation of visualization and analysis tool for 1-D spectrum based on MATLAB[J]. Astronomical Research & Technology, 2020, 17(1):121-128.
    [5]
    QIAO R C, XI X J, DOURNEAU G, et al. CCD astrometric observations of Phoebe in 2005-2008[J]. Monthly Notices of the Royal Astronomical Society, 2011, 413(2):1079-1082.
    [6]
    VADUVESCU O, HUDIN L, MOCNIK T, et al. 280 one-opposition near-Earth asteroids recovered by the EURONEAR with the Isaac Newton Telescope[J]. Astronomy & Astrophysics, 2011, 609:A105.
    [7]
    GUPTA A C, GAUR H, WⅡTA P J, et al. Characterizing optical variability of OJ 287 in 2016-2017[J]. The Astronomical Journal, 2019, 157(3):95.
    [8]
    JOYE W A, MANDEL E. New features of SAOImage DS9[C]//Astronomical Data Analysis Software and Systems XⅡ ASP Conference Series. 2003:489-492.
    [9]
    LANG D, HOGG D W, MIERLE K, et al. Astrometry.net:blind astrometric calibration of arbitrary astronomical images[J]. The Astronomical Journal, 2010, 139(5):1782-1800.
    [10]
    Gaia Collaboration, BROWN A G A, VALLENARI A, et al. Gaia data release 2. summary of the contents and survey properties[J]. Astronomy & Astrophysics, 2018, 616:A1.
    [11]
    LIN F R, PENG J H, ZHENG Z J, et al. Characterization of the precision premium in astrometry[J]. Monthly Notices of the Royal Astronomical Society, 2019, 490(3):4382-4387.
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