Nature research paper: Resolving the H i in damped Lyman α systems that power star formation
This work was supported by a NASA Keck PI Data Award, administered by the NASA Exoplanet Science Institute. Data presented herein were obtained at the W. M. Keck Observatory from telescope time allocated to the National Aeronautics and Space Administration through the agency’s scientific partnership with the California Institute of Technology and the University of California. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation.
Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, Victoria, AustraliaThe Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions , Hawthorn, Victoria, AustraliaMateusz Matuszewski, D. Christopher Martin, Patrick Morrissey & James D. Neill
Research School of Astronomy and Astrophysics, Australian National University, Canberra, Australian Capital Territory, Australia