Fig. 3.

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Flowchart of the CIRCE data reduction procedure. Because the procedure is complex, we divided it into three steps as explained in detail in the text. Starting from the raw frames provided by the telescope and generating the single images (step 1), and after performing some additional manipulations, we obtain the combined images of each OB (step 2), and finally, the deep NB1257 image (step 3).
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