Fig. 3

Intervening Fe iλ2719 absorption at zabs = 0.45206 (as marked) towards the quasar HE 0001−2340. This line falls on the blue wing of the quasar Lyα emission line. The spectrum (black curve) is shown together with a fit (see Sect. 3.2.3) of three blended Lyα absorptions, and bluewards, one Si ii absorption at zabs = 1.58643 (red curve). The Fe iλ2719 absorption is unexpectedly very weak (see Fig. 4).
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