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High-precision limit on variation in the fine-structure constant from a single quasar absorption system

, , and . (2016)cite arxiv:1609.03860Comment: 27 pages, 10 figures. Accepted by MNRAS. Quasar spectra and absorption profile fits are available at https://doi.org/10.5281/zenodo.51715.

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High-precision limit on variation in the fine-structure constant from a single quasar absorption system, , and . (2016)cite arxiv:1609.03860Comment: 27 pages, 10 figures. Accepted by MNRAS. Quasar spectra and absorption profile fits are available at https://doi.org/10.5281/zenodo.51715.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.The Magellan Uniform Survey of Damped Lyman alpha Systems II: Paucity of Strong Molecular Hydrogen Absorption, , , and . (2014)cite arxiv:1407.1111Comment: 21 pages, 20 figures, Accepted by MNRAS.Probing the thermal state of the intergalactic medium at $z>5$ with the transmission spikes in high-resolution Ly$\alpha$ forest spectra, , , , , , , , , and 6 other author(s). (2020)cite arxiv:2001.10018Comment: 20 pages (+10 pages appendices), 12 figures (+14 figures appendices); submitted to MNRAS; Main results are summarized in Fig. 10, Fig. 12 and Table 3.Spatial variation in the fine-structure constant -- new results from VLT/UVES, , , , , , , and . (2012)cite arxiv:1202.4758 Comment: 47 pages, 35 figures. Accepted for publication by Monthly Notices of the Royal Astronomical Society. Please see http://astronomy.swin.edu.au/~mmurphy/pub.html for an ASCII version of table A1 and the full set of Voigt profile fits for appendix C.A new Measurement of the Intergalactic Temperature at $z2.55-2.95$, , , , , and . (2017)cite arxiv:1711.00930Comment: Accepted for publication in MNRAS.A high molecular fraction in a sub-damped absorber at z=0.56, , , , , , , , , and 1 other author(s). (2012)cite arxiv:1210.0905Comment: 15 pages, 10 figures, submitted to MNRAS. Comments welcome. The data and code used are available here: https://github.com/nhmc/H2.The evolution of HI and CIV quasar absorption line systems at 1.9 < z < 3.2, , , and . (2013)cite arxiv:1302.6622Comment: 26 pages, 20 figures, accepted for AA, in press.Evidence of bimodal physical properties of intervening, optically-thin CIII absorbers at z ~ 2.5, , and . (2015)cite arxiv:1512.01050Comment: Accepted for publication in MNRAS. For the published paper: 29 pages, 24 figures, 7 tables. For online data, 53 velocity plots (c3_velplot.pdf), profile fitting line parameters (table2.dat, table2.pdf).Iron and alpha-element Production in the First One Billion Years after the Big Bang, , , and . (2011)cite arxiv:1111.4843Comment: Accepted for publication in ApJ.