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Recently, BES\uppercase\expandafter{\romannumeral3} Collaboration updated thedata of exotic state, $D^{*}_{s0}(2317)$, with mass at $2318.3\pm1.2\pm1.2$ MeVin the positronium annihilation process. Inspired by experiment, We study thetwo hot exotic states, $D^{*}_{s0}(2317)$ and $D_{s1}(2460)$, in the morereasonable unquenched quark model with two modified factor: the one is distanceconvergence, while the other is energy suppression. Different from the otherworks, we first give all of possible the mass shift and component of$D^{*}_{s0}(2317)$ and $D_{s1}(2460)$ at the same time. All the calculation aredone with the help of Gaussian expansion method, which is very accurate fewbody system calculation method. In addition, not only $DK(D^*K)$ but also theother OZI allowed mesonium including $D_s\eta$ are all taken intoconsideration. We propose an unquenched quark model to give a unitivedescription for $D_s$ spectrum including four particles: $D_s$, $D_s^{*}$,$D^{*}_{s0}(2317)$ and $D_{s1}(2460)$, and the results show that$D^{*}_{s0}(2317)$ and $D_{s1}(2460)$ are a $c\bar{s}$ sate plus an extraimportant component due to continuum while $D_s$ and $D_s^{*}$ are almost purequark-antiquark state.

$D^*_{s0}(2317)$ and $D_{s1}(2460)$ in an unquenched quark model