“…This set came into existence first in a comparison between only three codes ( van Setten et al, 2015 ). In the meantime the developers of many other codes have used the set to test and benchmark their implementations, both for GW and other computational approaches aiming at the calculation of ionization energies and electron affinities ( Caruso et al, 2016 ; Vlček et al, 2017a ; Maggio et al, 2017 ; Wilhelm and Hutter, 2017 ; Govoni and Galli, 2018 ; Rodrigues Pela et al, 2018 ; Colonna et al, 2019 ; Gao and Chelikowsky, 2019 ; Brémond et al, 2020 ; Förster and Visscher, 2020 ; Gao and Chelikowsky, 2020 ; Bintrim and Berkelbach, 2021 ; Duchemin and Blase, 2021 ; Förster and Visscher, 2021 ; Wilhelm et al, 2021 ). At present over a hundred data sets have appeared for the GW100 set.…”