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HI constraints from the cross-correlation of eBOSS galaxies and Green Bank Telescope intensity maps

, , , , , , , , , , , , , , , , , , , , and . (2021)cite arxiv:2102.04946Comment: 16 pages, 15 figures, 1 table; submitted to MNRAS.

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HI constraints from the cross-correlation of eBOSS galaxies and Green Bank Telescope intensity maps, , , , , , , , , and 11 other author(s). (2021)cite arxiv:2102.04946Comment: 16 pages, 15 figures, 1 table; submitted to MNRAS.Detecting the power spectrum turnover with HI intensity mapping. (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.HI intensity mapping correlation function from UNIT simulations: BAO and observationally induced anisotropy, , , , , , and . (2021)cite arxiv:2105.10454Comment: Comments welcome; 14 pages, 9 figures.Gaussian Process Regression for foreground removal in HI intensity mapping experiments, , , and . (2021)cite arxiv:2105.12665Comment: 19 pages, 1 table, 13 figures, main results in figures 6 and 9, code and data available at https://github.com/paulassoares/gpr4im.