S. Cunnington. (2022)cite arxiv:2202.13828Comment: 18 pages, 10 figures. See Fig 4 for main forecast of turnover detection for different HI IM surveys. See Fig 7 for constraints possible on turnover scale and Fig 8 for demo of how this can be used for cosmology. Accepted for publication in MNRAS.
S. Gezari, M. Bentz, K. De, K. French, A. Meisner, M. Ntampaka, R. Jedicke, E. Patel, D. Perley, R. Sanderson and 21 other author(s). (2022)cite arxiv:2202.12311Comment: 29 pages, 12 figures, Table of Implementation Recommendations, Appendix of Community Science Pitches, AURA-commissioned whitepaper submitted to the Director of STScI (Ken Sembach) and the Director of NOIRLab (Pat McCarthy).