ner_tags: O O O O O O B-Person I-Person B-Person I-Person B-Person I-Person B-Person I-Person O B-Person I-Person O O O O O O O O B-Person I-Person O O O O O B-Software O O O O O O O O O O O O B-Person I-Person O O O O O B-Software B-Person O O O O B-Organization I-Organization I-Organization B-Grant I-Grant I-Grant I-Grant O O B-Grant O O O O O B-Organization I-Organization B-Grant I-Grant I-Grant I-Grant B-Person O O O O B-Organization I-Organization I-Organization B-Grant I-Grant I-Grant I-Grant I-Grant I-Grant O O B-Grant O O B-Organization I-Organization I-Organization I-Organization O B-Organization I-Organization I-Organization O O O O O O B-Grant O O O O O O O B-Organization I-Organization I-Organization I-Organization I-Organization I-Organization I-Organization B-Organization O O B-Organization B-Grant I-Grant I-Grant I-Grant I-Grant I-Grant I-Grant I-Grant I-Grant
tokens: The authors would like to thank Marco Castellano, Dijana Vrbanec, Benedetta Ciardi, Darren Croton, and Manodeep Sinha for useful discussions and comments. The authors acknowledge Peter Creasey for permission to use his Python library as a basis for the computation of the power spectra, and Benedetta Ciardi for a collaboration in developing pCRASH. A.H. is supported under the Australian Research Council’s Discovery Project funding scheme (project number DP150102987). P.D. acknowledges support from the European Commission’s CO-FUND Rosalind Franklin program. C.M.T. is supported under the Australian Research Council’s Discovery Early Career Researcher funding scheme (project number DE140100316) and the Centre for All-sky Astrophysics (an Australian Research Council Centre of Excellence funded by grant CE110001020). Finally, this research was supported by the Munich Institute for Astro- and Particle Physics (MIAPP) of the DFG cluster of excellence “Origin and Structure of the Universe.”