ner_tags: O O O O O O O B-ComputingFacility I-ComputingFacility I-ComputingFacility I-ComputingFacility I-ComputingFacility I-ComputingFacility B-ComputingFacility O O O O O O O O O O O O B-Software O O O O B-Organization I-Organization I-Organization I-Organization I-Organization I-Organization I-Organization I-Organization O O O O O B-Organization I-Organization I-Organization I-Organization I-Organization B-Person O O O O O O O B-Fellowship I-Fellowship I-Fellowship I-Fellowship O O B-Organization I-Organization I-Organization B-Person O O O O O B-Organization I-Organization I-Organization B-Grant I-Grant I-Grant B-Person O O O O O B-Organization I-Organization I-Organization B-Organization B-Organization I-Organization I-Organization B-Grant I-Grant I-Grant I-Grant I-Grant I-Grant I-Grant I-Grant O B-Organization B-Grant I-Grant I-Grant I-Grant I-Grant I-Grant I-Grant I-Grant I-Grant I-Grant B-Grant I-Grant O O B-Person I-Person O B-Person I-Person O O O O O O O O O O O O O O O O O O B-Person I-Person I-Person O O O O O O O O B-Software B-Citation I-Citation I-Citation I-Citation O B-Software B-Citation I-Citation I-Citation O B-Software B-Citation I-Citation I-Citation I-Citation O B-Software B-Citation I-Citation O O B-Software O B-Software B-Citation I-Citation I-Citation I-Citation O
tokens: ACKNOWLEDGEMENTS The authors wish to acknowledge the DJEI/DES/SFI/HEA Irish Centre for High-End Computing (ICHEC) for the provision of computational facilities and support. This work used the BATS-R-US tools developed at the University of Michigan Center for Space Environment Modeling and made available through the NASA Community Coordinated Modeling Center. DÓF wishes to acknowledge funding received from the Trinity College Postgraduate Award through the School of Physics. AAV acknowledges funding received from the Irish Research Council Laureate Awards 2017/2018. SJ acknowledges the support of the German Science Foundation (DFG) Research Unit FOR2544 ‘Blue Planets around Red Stars’, project JE 701/3-1 and DFG priority program SPP 1992 ‘Exploring the Diversity of Extrasolar Planets’ (RE 1664/18). We thank Jackie Villadsen and Joe Llama for their useful discussion on topics of stellar radio emission. The authors would like to thank our referee, Dr Jorge Zuluaga, for his valuable input on this work. Software: bats-r-us (Powell et al. 1999 ), radiowinds (Ó Fionnagáin 2018 ), scipy (Jones et al. 2001 ), matplotlib (Hunter 2007 ), and tecplot and seaborn (Waskom et al. 2018 ).