Using the multiconfiguration Dirac–Hartree–Fock and the relativistic configuration interaction methods, a consistent set of transition energies and radiative transition data for the main states of the $2s^{2}2p^4$, $2s2p^5$, $2p^6$, $2s^{2}2p^{3}3s$, $2s^{2}2p^{3}3p$, $2s^{2}2p^{3}3d$, $2s2p^{4}3s$, $2s2p^{4}3p$, and $2s2p^{4}3d$ configurations in O-like Ions between Ar XI ($Z=18$) and Cr XVII ($Z=24$) is provided. Our data set is compared with the NIST compiled values and previous calculations. The data are accurate enough for identification and deblending of new emission lines from hot astrophysical and laboratory plasmas. The amount of data of high accuracy is significantly increased for the $n=3$ states of several O-like ions, where experimental data are very scarce.

使用多重配置Dirac–Hartree–Fock和相对论配置相互作用方法，获得了一组主要状态的跃迁能量和辐射跃迁数据的一致集合。 $2s^{2}2p^4$， $2s2p^5$， $2p^6$， $2s^{2}2p^{3}3s$， $2s^{2}2p^{3}3p$， $2s^{2}2p^{3}3d$， $2s2p^{4}3s$， $2s2p^{4}3p$和 $2s2p^{4}3d$ XI之间的O型离子中的构型（$ž=18$）和Cr XVII（$ž=24$）。将我们的数据集与NIST编译值和以前的计算进行比较。数据足够准确，可以识别和消除来自天体物理学和实验室等离子的新发射线。高精度的数据量大大增加了$ñ=3$ 几种O状离子的状态，实验数据非常稀少。