\begin{document}$ ^{-1} $\end{document} of \begin{document}$ e^+e^- $\end{document} collision data at center-of-mass energies ranging from 4.13 to 4.44 GeV. These data samples are primarily used for the study of excited charmonium and charmoniumlike states. By analyzing the di-muon process \begin{document}$e^+e^- \to $\end{document}\begin{document}$ (\gamma_{\rm ISR/FSR}) \mu^+\mu^-$\end{document}, we measure the center-of-mass energies of the data samples with a precision of 0.6 MeV. Through a run-by-run study, we find that the center-of-mass energies were stable throughout most of the data-collection period."> Measurements of the center-of-mass energies of <inline-formula><tex-math id="Z-20210730092014">\begin{document}${{\boldsymbol e^+}{\boldsymbol e^-}} $\end{document}</tex-math><alternatives><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="//www.macurncorp.com/hepnp/article/app/id/12866c3e-6e1b-4342-b703-a3f208d77223/CPC-2020-0685_Z-20210730092014.jpg"/><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="//www.macurncorp.com/hepnp/article/app/id/12866c3e-6e1b-4342-b703-a3f208d77223/CPC-2020-0685_Z-20210730092014.png"/></alternatives></inline-formula> collisions at BESIII -
  • [1]

    M. Ablikimet al. (BESIII Collaboration), Nucl. Instrum. Meth. A614, 345 (2010)

  • [2]

    D. M. Asneret al., Int. J. Mod. Phys. A24, 499 (2009)

  • [3]

    C. H. Yuet al.,Proceedings of IPAC2016, Busan, Korea, 2016,doi:10.18429/JACoW-IPAC2016-TUYA01

  • [4]

    M. Ablikimet al. (BESIII Collaboration), Chin. Phys. C44, 040001 (2020)

  • [5]

    E. V. Abakumovaet al., Nucl. Instrum. Meth. A659, 21 (2011)

  • [6]

    M. Ablikimet al. (BESIII Collaboration), Chin. Phys. C40, 063001 (2016)

  • [7]

    X. Liet al., Radiat. Detect. Technol. Methods1, 13 (2017)

  • [8]

    Y. X. Guoet al., Radiat. Detect. Technol. Methods1, 15 (2017)

  • [9]

    P. Caoet al., Nucl. Instrum. Meth. A953, 163053 (2020)

  • [10]

    Yifan Yang,The Study of M1 Transitions of Charmonia at BESIII, Ph.D thesis, Institute of High Energy Physics, 2019http://www.irgrid.ac.cn/handle/1471x/2539883?mode=full

  • [11]

    S. Agostinelliet al. (GEANT4 Collaboration), Nucl. Instrum. Meth. A506, 250 (2003)

  • [12]

    G. Balossini, C. M. Carloni Calame, G. Montagnaet al., Nucl. Phys. B758, 227 (2006)

  • [13]

    S. Jadach, B. F. L. Ward, and Z. Was, Phys. Rev. D63, 113009 (2001)

  • [14]

    S. Jadach, B. F. L. Ward, and Z. Was, Comput. Phys. Commun.130, 260 (2000)

  • [15]

    T. Skwarnickiet al., Report No. DESY F31-86-02 1986 (unpublished)

  • [16]

    P. A. Zylaet al. (Particle Data Group), Theor. Exp. Phys.2020, 083C01 (2020)

  • [17]

    E. Barberio and Z. Was, Comput. Phys. Commun.79, 291 (1994)

  • [18]

    N. Brambilla, S. Eidelman, C. Hanhartet al., Phys. Rept.873, 1-154 (2020), arXiv:1907.07583[hep-ex

  • [19]

    M. Ablikimet al. (BESIII Collaboration), arXiv: 2004.13788 [hep-ex]

  • [20]

    M. Ablikimet al. (BESIII Collaboration), Phys. Rev. Lett.124, 242001 (2020)

  • [21]

    M. Ablikimet al. (BESIII Collaboration), Phys. Rev. D101, 012008 (2020)

  • [22]

    M. Ablikimet al. (BESIII Collaboration), Phys. Rev. Lett.122, 232002 (2019)

  • [23]

    M. Ablikimet al. (BESIII Collaboration), Phys. Rev. D99, 091103 (2019)

  • [24]

    M. Ablikimet al. (BESIII Collaboration), Phys. Rev. Lett.122, 202001 (2019)

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