Abstract
Although a connection between certain classes of QSO absorption line systems and gas associated with galaxies was hypothesized long ago, the first systematic evidence supporting this was provided by Bergeron & Boissé (1991). Observing QSOs with known MgII absorption lines at z abs < z QSO, they identified galaxies near the QSO sightline and spectroscopically confirmed that their redshifts matched those of the MgII absorption doublet.
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References
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Dickinson, M., Steidel, C.C. (1996). Galaxy Evolution from QSO Absorption-Line Selected Samples. In: Bender, R., Davies, R.L. (eds) New Light on Galaxy Evolution. International Astronomical Union / Union Astronomique Internationale, vol 171. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0229-9_44
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DOI: https://doi.org/10.1007/978-94-009-0229-9_44
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