Abstract The Coster–Kronig enhancement factor for M3 shell X-ray production cross sections was found to be incorrectly calculated in all versions of ISICS. The affected program has been corrected an
This dataset includes input files for the impact simulations, including the thermal profiles of the target planets discussed in a related paper (Manske et al., JGR 2025 under review). Key Points We qu
27 rotation energy levels / 70 radiative transitions / 351 collisional transitions for H (14 temperatures in the range 5-1500K) / 91 collisional transitions for electron (9 temperatures in the range 1
VizieR online Data Catalogue associated with article published in journal Astronomical Journal (AAS) with title 'Electron-impact multiple-ionization cross sections for atoms and ions of helium through
