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${{\mathit D}_{{{s1}}}^{*}{(2700)}^{+}}$ WIDTH

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M182W

VALUE (MeV) EVTS DOCUMENT ID TECN  COMMENT $\bf{ 122 \pm10}$ OUR AVERAGE $136$ $\pm19$ $\pm24$ 15.7k AAIJ 2016 AW LHCB ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit D}^{*+}}{{\mathit K}_S^0}$ ${{\mathit X}}$ at 7, 8 TeV $127$ ${}^{+24}_{-19}$ 1 LEES 2015 C BABR ${{\mathit B}}$ $\rightarrow$ ${{\mathit D}}{{\mathit D}^{0}}{{\mathit K}^{+}}$ $115.8$ $\pm7.3$ $\pm12.1$ 52k 2 AAIJ 2012 AU LHCB ${{\mathit p}}$ ${{\mathit p}}$ $\rightarrow$ ( ${{\mathit D}}{{\mathit K}}){}^{+}{{\mathit X}}$ at 7 TeV $149$ $\pm7$ ${}^{+39}_{-52}$ 10.4k 3 AUBERT 2009 AR BABR ${{\mathit e}^{+}}$ ${{\mathit e}^{-}}$ $\rightarrow$ ${{\mathit D}^{(*)}}{{\mathit K}}{{\mathit X}}$ $108$ $\pm23$ ${}^{+36}_{-31}$ 182 BRODZICKA 2008 BELL ${{\mathit B}^{+}}$ $\rightarrow$ ${{\mathit D}^{0}}{{\overline{\mathit D}}^{0}}{{\mathit K}^{+}}$ • • We do not use the following data for averages, fits, limits, etc. • • $145$ $\pm24$ ${}^{+22}_{-14}$ LEES 2015 C BABR ${{\mathit B}^{0}}$ $\rightarrow$ ${{\mathit D}^{-}}{{\mathit D}^{0}}{{\mathit K}^{+}}$ $113$ $\pm21$ ${}^{+20}_{-16}$ LEES 2015 C BABR ${{\mathit B}^{+}}$ $\rightarrow$ ${{\overline{\mathit D}}^{0}}{{\mathit D}^{0}}{{\mathit K}^{+}}$ $112$ $\pm7$ $\pm36$ 4 AUBERT,BE 2006 E BABR 10.6 ${{\mathit e}^{+}}$ ${{\mathit e}^{-}}$ $\rightarrow$ ${{\mathit D}}{{\mathit K}}{{\mathit X}}$ 1  From a combined analysis of ${{\mathit B}^{0}}$ $\rightarrow$ ${{\mathit D}^{-}}{{\mathit D}^{0}}{{\mathit K}^{+}}$and ${{\mathit B}^{+}}$ $\rightarrow$ ${{\overline{\mathit D}}^{0}}{{\mathit D}^{0}}{{\mathit K}^{+}}$. 2  From the combined fit of the ${{\mathit D}^{+}}{{\mathit K}_S^0}$ and ${{\mathit D}^{0}}{{\mathit K}^{+}}$ modes in the model including the ${{\mathit D}_{{{s2}}}^{*}{(2573)}^{+}}$, ${{\mathit D}_{{{s1}}}^{*}{(2700)}^{+}}$ and spin-0 ${{\mathit D}_{{{sJ}}}^{*}{(2860)}^{+}}$. 3  From simultaneous fits to the two ${{\mathit D}}{{\mathit K}}$ mass spectra and to the total ${{\mathit D}^{*}}{{\mathit K}}$ mass spectrum. 4  Superseded by AUBERT 2009AR.

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