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Disambiguation of "Haehnelt, Martin G."

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Detection of dark galaxies and circum-galactic filaments fluorescently illuminated by a quasar at z=2.4

, , and . (2012)cite arxiv:1204.5753Comment: 25 pages, 16 figures, submitted to MNRAS.

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Martin G Ruf

Martin G Möhrle

Martin G Mack

Walter G Martin

Martin G Mack

 

Other publications of authors with the same name

A consistent determination of the temperature-density relation of the intergalactic medium at redshift z=2.4, , , and . (2013)cite arxiv:1308.4411Comment: 10 pages, 5 figures, submitted to MNRAS.Lyman-$\alpha$ emitters gone missing: evidence for late reionization?, , , and . (2014)cite arxiv:1412.4790Comment: 17 pages, submitted to MNRAS.The detectability of strong 21 centimetre forest absorbers from the diffuse intergalactic medium in late reionisation models, , , , , , , , and . (2021)cite arxiv:2105.02250Comment: 18 pages, 11 figures, 4 tables. Submitted to MNRAS, comments welcome.The evolution of the low-density HI intergalactic medium from z=3.6 to 0: Data, transmitted flux and HI column density, , , , , , , , , and 1 other author(s). (2020)cite arxiv:2012.05861Comment: 24 pages, 17 figures, 8 tables, accepted for publication to MNRAS, 5 supplementary online-only tables.Large scale opacity fluctuations in the Lyman alpha forest: evidence for QSOs dominating the ionising UV background at z ~ 5.5-6 ?, , and . (2016)cite arxiv:1606.08231Comment: 19 pages, 13 figures.First constraints on fuzzy dark matter from Lyman-$\alpha$ forest data and hydrodynamical simulations, , , , and . (2017)cite arxiv:1703.04683Comment: 7 pages, 3 figures.Extended and Filamentary Lyman Alpha Emission from the Formation of a Protogalactic Halo at z=2.63, , , , and . (2012)cite arxiv:1206.2680Comment: 18 pages, submitted to MNRAS.New Methods for Identifying Lyman Continuum Leakers and Reionization-Epoch Analogues, , , , , , , , , and . (2020)cite arxiv:2005.01734Comment: 16 pages, 11 figures, submitted to MNRAS.Seeding High Redshift QSOs by Collisional Runaway in Primordial Star Clusters, , and . (2015)cite arxiv:1502.03448Comment: 20 pages, 10 figures, submitted to MNRAS.On the rapid demise of Lyman-alpha emitters at z>7 due to the increasing incidence of optically thick absorption systems, and . (2012)cite arxiv:1208.4417Comment: 11 pages, 6 figures, submitted to MNRAS.