Resonance Decay Br [\(10^{-4}\)] Measured by Reference
\(D_{s0}^{*}(2317)^{\pm}\) \(B^{0}\to D_{s0}^{*}(2317)^{+}(\to D^{+}_{s}\pi^{0})D^{-}\) \( 8\) \(.6^{+3.3}_{-2.6}\pm2.6 \) Belle  [1]
\( 18\) \(.0\pm 4.0{}^{+6.7}_{-5.0} \) BaBar  [2]
\( 10\) \(.1^{+1.3}_{-1.2}\pm 1.0\pm0.4 \) Belle  [3]
\( 10\) \(.2 \pm 1.5 \) Our average
\(B^{+}\to D_{s0}^{*}(2317)^{+}(\to D^{+}_{s}\pi^{0})\overline{D}{}^{0}\) \( 8\) \(.0^{+1.3}_{-1.2}\pm1.0\pm0.4 \) Belle  [3]
\(B^{0}\to D_{s0}^{*}(2317)^{+}(\to D^{+}_{s}\pi^{0})K^{-}\) \( 0\) \(.53^{+0.15}_{-0.13}\pm0.16 \) Belle  [4]
\(D_{s1}(2460)^{\pm}\) \(B^{0}\to D_{s1}(2460)^{+}(\to D^{*+}_{s}\pi^{0})D^{-}\) \( 22\) \(.7^{+7.3}_{-6.2}\pm6.8 \) Belle  [1]
\( 28\) \(.0\pm 8.0{}^{+11.2}_{-7.8} \) BaBar  [2]
\( 24\) \(.7 \pm 7.6 \) Our average
\(B^{0}\to D_{s1}(2460)^{+}(\to D^{*+}_{s}\gamma)D^{-}\) \( 8\) \(.2^{+2.2}_{-1.9}\pm2.5 \) Belle  [1]
\( 8\) \(.0\pm 2.0{}^{+3.2}_{-2.3} \) BaBar  [2]
\( 8\) \(.1 \pm 2.3 \) Our average
\(D_{s1}(2460)^{+}\to D^{*+}_{s}\pi^{0}\) \( (56\) \({}\pm13\pm9)\% \) BaBar  [5]
\(D_{s1}(2460)^{+}\to D^{*+}_{s}\gamma\) \( (16\) \({}\pm4\pm3)\% \) BaBar  [5]
\(B^{0}\to D_{s1}(2536)^{+}(\to D^{*0}K^{+})D^{-}\) \( 1\) \(.71\pm0.48\pm0.32 \) BaBar  [6]
\(B^{0}\to D_{s1}(2536)^{+}(\to D^{*+}K^{0})D^{-}\) \( 2\) \(.61\pm1.03\pm0.31 \) BaBar  [6]
\(B^{0}\to D_{s1}(2536)^{+}(\to D^{*0}K^{+})D^{*-}\) \( 3\) \(.32\pm0.88\pm0.66 \) BaBar  [6]
\(B^{0}\to D_{s1}(2536)^{+}(\to D^{*+}K^{0})D^{*-}\) \( 5\) \(.00\pm1.51\pm0.67 \) BaBar  [6]
\(B^{+}\to D_{s1}(2536)^{+}(\to D^{*0}K^{+})\overline{D}^{0}\) \( 2\) \(.16\pm0.52\pm0.45 \) BaBar  [6]
\(B^{+}\to D_{s1}(2536)^{+}(\to D^{*+}K^{0})\overline{D}^{0}\) \( 2\) \(.30\pm0.98\pm0.43 \) BaBar  [6]
\(B^{+}\to D_{s1}(2536)^{+}(\to D^{*0}K^{+})\overline{D}^{*0}\) \( 5\) \(.46\pm1.17\pm1.04 \) BaBar  [6]
\(B^{+}\to D_{s1}(2536)^{+}(\to D^{*+}K^{0})\overline{D}^{*0}\) \( 3\) \(.92\pm2.46\pm0.83 \) BaBar  [6]
\(D_{s2}^{\ast}(2573)^{\pm}\) \(B^{0}\to D_{s2}^{\ast}(2573)(\to D^{0}K^{+})D^{-}\) \( 0\) \(.34\pm0.17\pm0.05\) BaBar  [7]
\(B^{+}\to D_{s2}^{\ast}(2573)(\to D^{0}K^{+})\overline{D}{}^{0}\) \( 0\) \(.08\pm14\pm0.05 \) BaBar  [7]
\(D_{s1}{}^{\ast}(2700)^{\pm}\) [3pt]\(B^{+}\to D_{s1}{}^{\ast}(2700)^{+}(\to D^{0}K^{+})\overline{D}{}^{0}\) \( 11\) \(.3\pm2.2{}^{+1.4}_{-2.8} \) Belle  [8]
\( 5\) \(.02\pm0.71\pm0.93 \) BaBar  [7]
\( 5\) \(.83 \pm 1.09 \) Our average
\(B^{0}\to D_{s1}{}^{\ast}(2700)^{+}(\to D^{0}K^{+})D{}^{-}\) \( 7\) \(.14\pm0.96\pm0.69 \) BaBar  [7]

[1] P. Krokovny and others, Phys.Rev.Lett. 91, 262002 (2003).

[2] B. Aubert and others, Phys.Rev.Lett. 93, 181801 (2004).

[3] S. K. Choi and others, Phys. Rev. D91, 092011 (2015).

[4] A. Drutskoy and others, Phys.Rev.Lett. 94, 061802 (2005).

[5] B. Aubert and others, Phys.Rev. D74, 031103 (2006).

[6] B. Aubert and others, Phys.Rev. D77, 011102 (2008).

[7] J. P. Lees and others, Phys. Rev. D91, 052002 (2015).

[8] J. Brodzicka and others, Phys.Rev.Lett. 100, 092001 (2008).