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Table 8
Summary of the main input parameters for the PyCS spline (spl) and dispersion (disp) methods.
| spl: ηintr | 75 days |
| spl: ηextr | 520 days |
| spl: ϵ | 15 days |
| spl: αA | 1.1 |
| spl: βA | 0 |
| spl: αB | 3.1 |
| spl: βB | 0 |
| disp: interpdist | 10 days |
| disp: nparams | 1 |
| tsrand | 5 days |
| truetsr | 0 days |
Notes. Indices A and B refer to the quasar images. (See Tewes et al. 2013, for detailed explanation.)
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