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Table 2.

Differential microlensing (B–A) in the BEL wings.

Emission Line Wing Δm (mag) Scatter (mag)
(1) (2) (3) (4)
C IV Blue −0.07 0.00
Red −0.33 0.32

C III] Blue 0.00 0.14
Red +0.09 0.33

Mg II Blue
Red −0.09 0.07

Notes. Col. (1): Emission line core used as a reference for no microlensing. Col. (2): Emission line wing. Cols. (3)–(4): Average differential microlensing and scatter between observational epochs.

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