Cosmo-tomography toward PKS 1830−211: Variability of the quasar and of its foreground molecular absorption monitored with ALMA

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Fig. 6.

Overlay of all ALMA spectra of H₂O (SW and NE lines of sight) and CH (SW only) observed toward PKS 1830−211 between 2012 and 2016. Special profiles showing clear deviations are highlighted with the color code given in the upper box.

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