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Zooming into the broad line region of the gravitationally lensed quasar QSO 2237+0305 equivalent to the Einstein Cross III Determination of the size and structure of the C IV and C III] emitting regions using microlensing

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Academic year: 2020

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Figure

Fig. 1. Comparison of V-band OGLE lightcurves of images A & D (points) of QSO 2237+0305 with the lightcurves derived from our spectra (diamonds; crosses are used for epochs deviating from the OGLE lightcurves)
Table 1. Journal of the observations used in this paper.
Table 2. Decomposition of the C iv and C iii] emission lines (Average value and scatter between epochs when the parameter is fitted).
Table 3. Average values of magnitude difference Δm AD as measured in the blue wing (BE), line core (CE), and red wing (RE) of the C iv and C iii] emission lines.
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