Submillimeter water and ammonia absorption by the peculiar z~0.89 interstellar medium in the gravitational lens of the PKS 1830-211 system
K. M. Menten (MPIfR), R. Guesten (MPIfR), S. Leurini (ESO), S., Thorwirth (MPIfR), C. Henkel (MPIfR), B. Klein (MPIfR), C. L. Carilli (NRAO),, and M. J. Reid (CfA)

TL;DR
This study reports the detection of water and ammonia absorption lines in a galaxy at redshift 0.89, providing insights into its interstellar medium and potential for testing fundamental physical constants over cosmic time.
Contribution
First detection of ground-state ammonia and water absorption lines in a galaxy at intermediate redshift using APEX, comparing interstellar medium properties with the Milky Way.
Findings
Detected ortho-ammonia and water lines at z~0.89
Identified differences between extragalactic and Galactic interstellar media
Potential to constrain proton-electron mass ratio variation over 7.2 Gyr
Abstract
Using the Atacama Pathfinder Experiment (APEX) telescope we have detected the rotational ground-state transitions of ortho-ammonia and ortho-water toward the redshift ~0.89 absorbing galaxy in the PKS 1830-211 gravitational lens system. We discuss our observations in the context of recent space-borne data obtained for these lines with the SWAS and Odin satellites toward Galactic sources. We find commonalities, but also significant differences between the interstellar media in a galaxy at intermediate redshift and in the Milky Way. Future high-quality observations of the ground-state ammonia transition in PKS 1830-211, together with inversion line data, will lead to strong constraints on the variation of the proton to electron mass ratio over the past 7.2 Gyr.
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