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1/f Noise Analysis for FAST HI Intensity Mapping Drift-Scan Experiment

, , , , , , , , , , and . (2021)cite arxiv:2109.06447Comment: 13 pages,17 figures, MNRAS accepted.

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Measuring the HI mass function below the detection threshold, , , , , , , and . (2019)cite arxiv:1907.10404Comment: 15 pages, 11 figures, submitted to MNRAS.Intensity mapping of H-alpha, H-beta, OII and OIII lines at z<5, , , , , , , and . (2016)cite arxiv:1610.09060Comment: 14 pages, 9 figures, 4 tables.A first detection of neutral hydrogen intensity mapping on Mpc scales at $z0.32$ and $z0.44$, , , and . (2023)cite arxiv:2301.11943Comment: 19 pages, 10 figures, submitted to ApJL.1/f Noise Analysis for FAST HI Intensity Mapping Drift-Scan Experiment, , , , , , , , , and 1 other author(s). (2021)cite arxiv:2109.06447Comment: 13 pages,17 figures, MNRAS accepted.The optically-selected 1.4-GHz quasar luminosity function below 1 mJy, , , , and . (2019)cite arxiv:1908.05316Comment: 20 pages, 14 figures, 5 tables.HI intensity mapping with MeerKAT: 1/f noise analysis, , , , and . (2020)cite arxiv:2007.01767Comment: 14 pages, 12 figures.Improved Constraints on the 21 cm EoR Power Spectrum and the X-Ray Heating of the IGM with HERA Phase I Observations, , , , , , , , , and 84 other author(s). (2022)cite arxiv:2210.04912Comment: 55 pages, 37 figures. Submitted to ApJ. Corresponding author: Joshua S. Dillon.A Real Time Processing system for big data in astronomy: Applications to HERA., , , , , , , , , and 65 other author(s). Astron. Comput., (2021)On the contamination of the global 21~cm signal from polarized foregrounds, , and . (2019)cite arxiv:1908.05303Comment: 9 pages, 10 figures, comments welcome.Prospects for cosmic magnification measurements using HI intensity mapping, , and . (2019)cite arxiv:1907.00755Comment: 7 pages, 7 figures, 1 table.