Imaging detection of the inner dust belt and the four exoplanets in the HR 8799 system with JWST’s MIRI coronagraph

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Table 2

Coronagraphic transmission.

Planet	F1065C	F1140C	F1550C
b	0.81/0.82	0.75/0.79	0.77/0.82
c	0.78/0.80	0.75/0.78	0.62/0.65
d	0.61/0.67	0.60/0.65	0.62/0.66
e	0.56/0.58	0.52/0.56	0.40/0.45

Notes. The transmission of the 4QPM coronagraphs at the planet location is calculated for a point source in each filters, either in an aperture region of 1.5 λ/D in radius, or integrated in the whole image.

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