All Tables

Table 1: Equivalent widths of the most intensive emission lines from the local spot model (this paper), measured (i) with respect to the reflected continuum, $EW_{\rm {}refl}$ , and (ii) to the sum of the incident plus reflected continuum, $EW_{\rm {}total}$ . Only lines with EWs higher than 1 eV are listed.
Table 2: Exemplary flare distribution properties for the black hole/disk system seen at a moderate inclination, $i=30{\hbox {$^\circ $ }}$ . Parameters above the double line are assumed while the parameters below the double line are calculated as described in Sect. 2.2.