• [1]

    D. W. Savin, AIP Conference Proceedings, 926: 124 (2007)

  • [2]

    T. R. Kallman, Space Sci. Rev., 157: 177 (2010)

  • [3]

    P. Bryans et al, Astrophys. J. suppl. S., 167: 343 (2006)

  • [4]

    C. S. Reynolds, A. Fabian, Mon. Not. R. Astron. Soc., 273: 1167 (1995)

  • [5]

    M. C. Weisskopf et al, X-Ray Optics, Instruments, and Missions Ⅲ, 4012: 2 (2000)

  • [6]

    F. Jansen et al, AA, 365: L1 (2001)

  • [7]

    D. W. Savin, AIP Conference Proceedings, 774: 297 (2005)

  • [8]

    A. Mler, Adv. Atom. Mol. Opt. Phys., 55: 293 (2008)

  • [9]

    S. Schippers et al, Int, Rev. At. Mol. Phys., 1: 109 (2010)

  • [10]

    O. Novotn et al, Astrophys. J., 753: 57 (2012)

  • [11]

    P. Mazzotta et al, Astron. Astrophys. Suppl. S., 133: 403 (1998)

  • [12]

    P. Bryans, E. Landi, D. W. Savin, Astrophys. J., 691: 1540 (2009)

  • [13]

    D. W. Savin et al, Astrophys. J. suppl. S., 123: 687 (1999)

  • [14]

    K. Arnaud, Astronomical Data Analysis Software and Systems V, 101: 17 (1996)

  • [15]

    R. K. Smith et al, Astrophys. J. Lett., 556: L91 (2001)

  • [16]

    T. Kallman, P. Palmeri, Rev. Mod. Phys., 79: 79 (2007)

  • [17]

    S. Schippers et al, Astron. Astrophys., 421: 1185 (2004)

  • [18]

    Z. Huang et al, Astrophys. J. suppl. S., 235: 2 (2018)

  • [19]

    S. Mahmood et al, Astrophys. J., 771: 78 (2013)

  • [20]

    N. R. Badnell, J. Phys. B: at. Mol. Opt., 39: 4825 (2006)

  • [21]

    S. Schippers et al, J. Phys.: Conf. Ser., 388: 062029 (2012)

  • [22]

    M. Sako et al, Astron. Astrophys., 365: L168 (2001)

  • [23]

    H. Netzer et al, Astrophys. J., 599: 933 (2003)

  • [24]

    G. Ferland et al, Publ. Astron. Soc. Pac., 110: 761 (1998)

  • [25]

    T. Kallman et al, Astrophys. J. suppl. S., 155: 675 (2004)

  • [26]

    S. Schippers et al, J. Phys.: Conf. Ser., 388: 062029 (2012)

  • [27]

    D. W. Savin et al, Astrophys. J. Lett., 489: L115 (1997)

  • [28]

    D. Savin et al, Astrophys. J., 642: 1275 (2006)

  • [29]

    G. J. Ferland, Annu. Rev. Astron. Astr., 41: 517 (2003)

  • [30]

    D. W. Savin, J. M. Laming, Astrophys. J., 566: 1166 (2002)

  • [31]

    M. F. Gu, Can. J. Phys., 86: 675 (2008)

  • [32]

    D. Bernhardt et al, Phys. Rev. A, 91: 012710 (2015)

  • [33]

    M. Lestinsky et al, Phys. Rev. Lett., 100: 033001 (2008)

  • [34]

    J.-W. Xia et al, Nucl. Instrum. Meth. A, 488: 11 (2002)

  • [35]

    Z. Huang et al, Phys. Scripta., 2015: 014023 (2015)

  • [36]

    M. Ling-Jie et al, Chinese Physics C, 37: 017004 (2013)

  • [37]

    W. Wen et al, Nucl. Instrum. Meth. B, 317: 731 (2013)

  • [38]

    T. Shirai et al, J. Phys. Chem. Ref. Data, 19: 127 (1990)

  • [39]

    S. Schippers et al, Phys. Rev. A, 62: 022708 (2000)

  • [40]

    C.-Y. Chen et al, J. Quant. Spectrosc. Ra, 111: 843 (2010)

  • [41]

    O. Zatsarinny et al, Astron. Astrophys., 447: 379 (2006)

  • [42]

    A. Mler, Int. J. Mass. Spectrom., 192: 9 (1999)

  • [43]

    M. Fogle et al, Astron. Astrophy., 409: 781 (2003)