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O VI Emission Imaging of a Galaxy with the Hubble Space Telescope: a Warm Gas Halo Surrounding the Intense Starburst SDSS J115630.63+500822.1

, , , , , and . (2016)cite arxiv:1606.04536Comment: Accepted by the Astrophysical Journal. 25 pages, 11 figures. Section 7 presents calculated properties of warm halo gas.

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Quenching by gas compression and consumption: A case study of a massive radio galaxy at z = 2.57, , , , and . (2019)cite arxiv:1902.08622Comment: Accepted for publication in Astronomy & Astrophysics. 20 pages, 14 figures, 6 tables.The GLEAMing of the First Supermassive Black Holes, , , , , , , , , and . (2021)cite arxiv:2111.08104Comment: 19 pages, 9 figures, published in PASA.O VI Emission Imaging of a Galaxy with the Hubble Space Telescope: a Warm Gas Halo Surrounding the Intense Starburst SDSS J115630.63+500822.1, , , , , and . (2016)cite arxiv:1606.04536Comment: Accepted by the Astrophysical Journal. 25 pages, 11 figures. Section 7 presents calculated properties of warm halo gas.How robustly can we constrain the low-mass end of the $z\sim6-7$ stellar mass function? -- The limits of lensing models and stellar population assumptions in the Hubble Frontier Fields, , , , and . (2020)cite arxiv:2011.13991Comment: Accepted for publication in MNRAS. 24 pages, 21 figures.