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Q 0420-014
V = 17.0; z = 0.915; exp = 3600 s; coverage = 3810.5-6304.9 A
This QSO was not included in the studies of SSB nor SS92, but was observed by Wills et al.(1980), who first reported the system studied in this work.
z=0.633004 |DATA & VOIGT PROFILES| |EWs & AOD COLUMNS| |VP PARAMETERS|
The overall profile is comprised of two kinematic subfeatures, one broad and complex, separated by ~200 km/s. A total of nine VP components were fit. The Ca II 3934, 3969 doublet was not covered by the HIRES format. The Mn II triplet and all but the Fe II 2600 transition showed no absorption to the EW(rest) limits given in Table 3.15. The spectra are low quality, having signal to noise ranging from two to four, for the Fe II 2344, 2374, and 2382 transitions.
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