et.al. [@Kamal]. Also, the value of the branching ratio for $D^0\rightarrow  K\pi$ may have been overestimated [@ID].

Finally, we note that as the mass of the decaying particle increases the $SU(3)$ symmetry breaking becomes greater at $q^2 =
0$.

[**Acknowledgment**]{}

This work was supported in part by the Natural Sciences and Engineering Council of Canada and by the Scientific and Technical Research Council of Turkey.

  --------------------------------------------------------------------------------------------------------------------------------------------------
        Reference        $D\rightarrow \rho $   $D\rightarrow  K^{*}$   $D\rightarrow \rho /       $B\rightarrow  \rho $       $B\rightarrow K^{*}$
                                                                        D\rightarrow  K^{*}$                                  
  --------------------- ---------------------- ----------------------- ---------------------- ------------------------------- ----------------------
    [@WSB]$^{a,\dag}$           $0.67$                 $ 0.73$                 $0.92$                     $0.28$                       $-$

      [@GIW]$^{a}$              $0.85$                 $0.80$                  $1.06$                     $0.14$                       $-$

     [@GilSin]$^{a}$             $-$                $0.91 (0.84)$               $-$                       $-0.37$                      $-$

      [@FGM]$^{a}$                                 $0.74 \pm 0.12$              $-$                   $0.14 \pm 0.20$                  $-$

      [@Ball]$^{b}$        $0.57 \pm 0.40$         $0.45 \pm 0.30$      $1.27   \pm   1.23$         $0.79   \pm   0.80$                $-$

    [@CFS]$^{b,\dag}$      $0.52 \pm 0.05$         $0.58 \pm 0.05$        $0.90 \pm 0.12$             $0.24 \pm 0.02$            $0.30 \pm 0.03$

      [@Nar]$^{b}$               $-$                     $-$                    $-$                   $0.15 \pm 0.97$                  $-$

      [@Slob]$^{b}$              $-$                     $-$                    $-$                   $0.28 \pm 1.1 $                  $-$

     [@CDBFGN]$^{c}$            $0.74$                 $0.59$                  $1.25$                     $0.24$                       $-$

    [@BFO]$^{c,\dag}$      $0.73 \pm 0.17$        $0.65 \pm  0.14$        $1.12 \pm  0.36$           $1.10 \pm  0.30$                  $-$

     [@HusIT]$^{c}$              $-$              $0.39 \pm  0.13$              $-$                         $-$                        $-$

      [@Lub]$^{d}$         $0.76 \pm 0.25$        $0.72 \pm 0.17 $        