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Level energies, wavelengths, electric dipole, magnetic dipole, electricquadrupole, and magnetic quadrupole transition rates, oscillator strengths, andline strengths from combined relativistic configuration interaction andmany-body perturbation calculations are reported for the 201 fine-structurestates of the $2s^2 2p^6$, $2s^2 2p^5 3l$, $2s 2p^6 3l$, $2s^2 2p^5 4l$, $2s2p^6 4l$, $2s^2 2p^5 5l$, and $2s^2 2p^5 6l$ configurations in all Ne-like ionsbetween Cr XV and Kr XXVII. Calculated level energies and transition data arecompared with experiments from the NIST and CHIANTI databases, and other recentbenchmark calculations. The mean energy difference with the NIST experiments isonly 0.05%. The present calculations significantly increase the amount ofaccurate spectroscopic data for the $n >3$ states in a number of Ne-like ionsof astrophysics interest. A complete dataset should be helpful in analyzing newobservations from the solar and other astrophysical sources, and is also likelyto be useful for modeling and diagnosing a variety of plasmas includingastronomical and fusion plasma.

the astrophysical journal. supplement series/astrophysical journal. supplement series

Extended relativistic configuration interaction and many-body  perturbation calculations of spectroscopic data for the $n \leq 6$  configurationsin ne-like ions between Cr XV and Kr XXVII