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Fig. 6


Spectral extraction of a T5 (T ~ 1100 K) model spectrum (black line) for planets at different separations (from top to bottom) and contrast from the star (10-4 on the left, 10-5 on the right). The blue points represent the IFS photometry for each channel (reduced with the SD technique), while the red ones represent the flux measurement in the two IRDIS filters H2 and H3. For IRDIS data, the black horizontal line represents the therotical value of the photometry; each line covers the bandpass of the filters.

This figure is made of several images, please see below:

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