\sqrt{1\over{105}} \; \widetilde{A}_{c\bar{s}} $                       0.8       0.3
  $D_s(D_{2}')(2926)$     ${D_s}_{2}'\to [D^*K]_P$       $-i \sqrt{5\over{27}} \; \widetilde{D}_{c\bar{s}} \cos(\theta+\phi)$       116     
                          ${D_s}_{2}'\to [D^*K]_F$       $+i \sqrt{1\over{15}}  \; \widetilde{A}_{c\bar{s}} \sin(\theta+\phi)$    $\sim 0$  
                          ${D_s}_{2}'\to [D^*\eta]_P$    $+i \sqrt{5\over{108}} \; \widetilde{D}_{c\bar{s}} \cos(\theta+\phi)$       17     
                          ${D_s}_{2}'\to [D^*\eta]_F$    $-i \sqrt{1\over{60}}  \; \widetilde{A}_{c\bar{s}} \sin(\theta+\phi)$    $\sim 0$  
  $D_s(D_{2})(2900)$      ${D_s}_{2}\to [D^*K]_P$        $-i \sqrt{5\over{27}} \; \widetilde{D}_{c\bar{s}} \sin(\theta+\phi)$     $\sim 0$  
                          ${D_s}_{2}\to [D^*K]_F$        $-i \sqrt{1\over{15}} \; \widetilde{A}_{c\bar{s}} \cos(\theta+\phi)$        20     
                          ${D_s}_{2}\to [D^*\eta]_P$     $+i \sqrt{5\over{108}} \; \widetilde{D}_{c\bar{s}} \sin(\theta+\phi)$    $\sim 0$  
                          ${D_s}_{2}\to [D^*\eta]_F$     $+i \sqrt{1\over{60}} \; \widetilde{A}_{c\bar{s}} \cos(\theta+\phi)$       1.0     
  $D_s^*(1^3D_1)(2899)$   $D_s^*(1^3D_1)\to DK$          $+i \sqrt{10\over{81}} \; \widetilde{D}_{c\bar{s}} $                       101       93
                          $D_s^*(1^3D_1)\to D^*K$        $-i \sqrt{5\over{81}} \; \widetilde{D}_{c\bar{s}} $                         36       32
                          $D_s^*(1^3D_1)\to D_s\eta$     $ -i \sqrt{5\over{162}} \; \widetilde{D}_{c\bar{s}} $                       18       16
                          $D_s^*(1^3D_1)\to D_s^*\eta$   $+i \sqrt{5\over{324}} \; \widetilde{D}_{c\bar{s}} $                       5.0        4
  ----------------------- ------------------------------ ----------------------------------------------------------------------- ---------- -------

Before proceeding to the discussion we make a brief digression regarding kinematically allowed decays to $DK^*$ final states. As pointed out above, decays to light vector mesons are beyond the scope of the pseudoscalar emission model. However, we can use heavy quark symmetry to estimate their partial widths. In the heavy quark limit the light quark angular momentum is separately conserved from the heavy quark spin. For the $1^3D_3$ state $j_q^P=5/2^-$ and for the $1^3D_1$ state $j_q^P=3/2^-$. For the decay $1^3D_3\to 