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The abundance of $z 10$ galaxy candidates in the HUDF using deep JWST NIRCam medium-band imaging, , , , , , and . (2022)cite arxiv:2212.10126Comment: 8 pages, 4 figures, submitted to MNRAS.The properties of He II 1640 emitters at z ~ 2.5-5 from the VANDELS survey, , , , , , , , , and 16 other author(s). (2019)cite arxiv:1911.09999Comment: 19 pages, 10 figures (including appendix), submitted to A&A. Comments welcome!.The evolution of the galaxy UV luminosity function at redshifts z ~ 8-15 from deep JWST and ground-based near-infrared imaging, , , , , , , , , and 3 other author(s). (2022)cite arxiv:2207.12356Comment: 28 pages, 4 figures in main manuscript, submitted to MNRAS.Two bright z > 6 quasars from VST ATLAS and a new method of optical plus mid-infra-red colour selection, , , , , , , , and . (2015)cite arxiv:1502.07748Comment: 5 pages, 2 figures, submitted to MNRAS letters.The VANDELS survey: Dust attenuation in star-forming galaxies at $z=3-4$, , , , , , , , , and 7 other author(s). (2017)cite arxiv:1712.01292Comment: 15 pages, 11 figures, submitted to MNRAS.A massive quiescent galaxy at redshift 4.658, , , , , , , , , and 3 other author(s). (2023)cite arxiv:2301.11413Comment: 24 pages, 4 figures, submitted to Nature.