Level-resolved photoionization cross-sections for modelling astrophysical plasma

Acknowledgements: GDZ and RPD acknowledge support from Science and Technologies Facilities Council (STFC, UK) via the consolidated grants to the atomic astrophysics group at DAMTP, University of Cambridge (ST/T000481/1). GDZ also acknowledges support from STFC via the large grant award to the SAMS project. Most of the atomic rates used in this study and in chianti were produced by the UK APAP network funded by STFC via several grants to the University of Strathclyde, led by the late Nigel R. Badnell.4 CHIANTI is a collaborative project involving the University of Cambridge (UK), the NASA Goddard Space Flight Center, the George Mason University, and the University of Michigan (USA).