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Fig. 3


Thermal emission flux maps for three different bolometric albedo values (top: αbol = 0.0, middle: αbol = 0.3, bottom: αbol = 0.5). Thermal emission is stronger for short term period planets around hot stars. For all the plots, we assume RP = 1.0RJ. The white part of the diagram refers to fth < 10-7.

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