Deprojection technique for galaxy cluster considering the point spread function

被引:0
|
作者
WANG YuSa
机构
基金
中国国家自然科学基金;
关键词
PSF; Direct Demodulation; deprojection; Abell; 1835; galaxy cluster; XMM-Newton;
D O I
暂无
中图分类号
O174 [函数论];
学科分类号
070104 ;
摘要
We present a new method for the analysis of Abell 1835 observed by XMM-Newton.The method is a combination of the Direct Demodulation technique and deprojection.We eliminate the effects of the point spread function(PSF) with the Direct Demodulation technique.We then use a traditional deprojection technique to study the properties of Abell 1835.Compared to only using a deprojection method,the central electron density derived from this method increases by 30%,while the temperature profile is similar.
引用
收藏
页码:183 / 186
页数:4
相关论文
共 50 条
  • [1] Deprojection technique for galaxy cluster considering the point spread function
    Wang YuSa
    Jia ShuMei
    Chen Yong
    SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY, 2010, 53 : 183 - 186
  • [2] Deprojection technique for galaxy cluster considering the point spread function
    YuSa Wang
    ShuMei Jia
    Yong Chen
    Science China Physics, Mechanics and Astronomy, 2010, 53 : 183 - 186
  • [3] SMAUG: A new technique for the deprojection of galaxy clusters
    Pizzolato, F
    Molendi, S
    Ghizzardi, S
    De Grandi, S
    ASTROPHYSICAL JOURNAL, 2003, 592 (01): : 62 - 78
  • [4] Constraining the point spread function by using galaxy images
    Nie, Lin
    Li, Guoliang
    Zhang, Jun
    Fan, Zuhui
    Peterson, John R.
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2021, 508 (03) : 3785 - 3795
  • [5] Enhancing spectral unmixing by considering the point spread function effect
    Wang, Qunming
    Shi, Wenzhong
    Atkinson, Peter M.
    SPATIAL STATISTICS, 2018, 28 : 271 - 283
  • [6] An improved deprojection and PSF-deconvolution technique for galaxy-cluster X-ray surface-brightness profiles
    Croston, J.H.
    Arnaud, M.
    Pointecouteau, E.
    Pratt, G.W.
    Astronomy and Astrophysics, 1600, 459 (03): : 1007 - 1019
  • [7] Spectroscopic deprojection analysis of Chandra data of the galaxy cluster 3C 129
    Krawczynski, H
    ASTROPHYSICAL JOURNAL, 2002, 569 (01): : L27 - L30
  • [8] An improved deprojection and PSF-deconvolution technique for galaxy-cluster X-ray surface-brightness profiles
    Croston, J. H.
    Arnaud, M.
    Pointecouteau, E.
    Pratt, G. W.
    ASTRONOMY & ASTROPHYSICS, 2006, 459 (03) : 1007 - 1019
  • [9] Point-spread Function Deconvolution of the IFU Data and Restoration of Galaxy Stellar Kinematics
    Chung, Haeun
    Park, Changbom
    Park, Yong-Sun
    ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2021, 257 (02):
  • [10] The cluster galaxy luminosity function
    Molinari, E
    ASTROPHYSICS AND SPACE SCIENCE, 1999, 269 (0) : 655 - 656