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Photometric IGM Tomography: Efficiently Mapping Quasar Light Echoes with Deep Narrow Band Imaging

, , and . (2022)cite arxiv:2207.08202Comment: 21 pages, 14 figures, accepted for publication in MNRAS.

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Opening Reionization: Quantitative Morphology of the Epoch of Reionization and Its Connection to the Cosmic Density Field, , , and . (2020)cite arxiv:2009.03093Comment: 18 pages, 15 figure, as accepted for publication by MNRAS.Photometric IGM Tomography: Efficiently Mapping Quasar Light Echoes with Deep Narrow Band Imaging, , and . (2022)cite arxiv:2207.08202Comment: 21 pages, 14 figures, accepted for publication in MNRAS.The role of galaxies and AGN in reionising the IGM -- III : IGM-galaxy cross-correlations at z~6 from 8 quasar fields with DEIMOS and MUSE, , , , , , , , and . (2019)cite arxiv:1912.04314Comment: Submitted to MNRAS. 17 pages, 18 figures, 3 tables + appendices. Key results: Figs. 6,13,14.Cosmic Galaxy-IGM HI Relation at $z2-3$ Probed in the COSMOS/UltraVISTA $1.6$ deg$^2$ Field, , , , , , , , , and . (2016)cite arxiv:1605.00379Comment: 9 pages, 8 figures, submitted to ApJ.Observing the redshifted 21 cm signal around a bright QSO at $z10$, , , , , and . (2019)cite arxiv:1911.10880Comment: 11 pages, 10 figures, apj accepted.A new model framework for circumgalactic Ly$\alpha$ radiative transfer constrained by galaxy-Ly$\alpha$ forest clustering, and . (2017)cite arxiv:1710.10053Comment: 20 pages, 14 figures, submitted to MNRAS.Lyman-Alpha Emitting Galaxies as a Probe of Reionization: Large-Scale Bubble Morphology and Small-Scale Absorbers, , , and . (2015)cite arxiv:1510.05647Comment: 23 pages, 20 figures, submitted to MNRAS, Abstract abridged for arXiv submission.Constraining IGM enrichment and metallicity with the C IV forest correlation function, , , and . (2022)cite arxiv:2201.10571Comment: 19 pages, 17 figures, 1 appendix. Submitted to MNRAS.