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Cited article:

Ammonia in the interstellar medium of a starbursting disc at z = 2.6

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Cosmological Constraints on a Temporal Variation of the Proton-to-electron Mass Ratio based on the Red-shifted Lines of Extragalactic Argonium

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Astronomy Reports 65 (12) 1211 (2021)
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ALMA Observations of Molecular Absorption in the Gravitational Lens PMN 0134−0931 at z = 0.7645

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Probing the interstellar dust in galaxies over >10 Gyr of cosmic history

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Planetary and Space Science 133 7 (2016)
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Accurate prediction of the ammonia probes of a variable proton-to-electron mass ratio

A. Owens, S. N. Yurchenko, W. Thiel and V. Špirko
Monthly Notices of the Royal Astronomical Society 450 (3) 3191 (2015)
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The inhomogeneous ISM toward PKS 1830–211 SW: A detailed view of molecular gas at a look-back time of 7.5 Gyr

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Robust Constraint on a Drifting Proton-to-Electron Mass Ratio atz=0.89from Methanol Observation at Three Radio Telescopes

J. Bagdonaite, M. Daprà, P. Jansen, et al.
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ON MEASURING THE COSMIC MICROWAVE BACKGROUND TEMPERATURE AT REDSHIFT 0.89

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INTERSTELLAR SILICATE DUST IN THEz= 0.89 ABSORBER TOWARD PKS 1830-211: CRYSTALLINE SILICATES AT HIGH REDSHIFT?

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From Varying Couplings to Fundamental Physics

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DETECTION OF C I IN ABSORPTION TOWARD PKS 1830 – 211 WITH THE eSMA

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The Astrophysical Journal 690 (2) L130 (2009)
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