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Table 3
Number of detected planets out of 30, in function of the contrast (columns) and the separation (lines) for IRDIS and IFS subsystems.
10-3 | 3 × 10-4 | 10-4 | 3 × 10-5 | 10-5 | ||||||
|
||||||||||
IRDIS | IFS | IRDIS | IFS | IRDIS | IFS | IRDIS | IFS | IRDIS | IFS | |
0.̋20 | 30 (20) | 30 (70) | 30 (9) | 30 (22) | 6 (7) | 27 (7) | 0 (–) | 1 (6) | 0 (–) | 0 (–) |
0.̋35 | 30 (98) | 30 (347) | 30 (42) | 30 (129) | 30 (15) | 30 (46) | 18 (6) | 30 (14) | 0 (–) | 14 (8) |
0.̋50 | 30 (171) | 30 (238) | 30 (64) | 30 (114) | 30 (22) | 30 (43) | 23 (8) | 30 (12) | 5 (8) | 5 (7) |
0.̋65 | 30 (260) | 30 (281) | 30 (93) | 30 (135) | 30 (31) | 30 (55) | 29 (10) | 30 (17) | 6 (7) | 6 (8) |
0.̋80 | 30 (272) | 30 (285) | 30 (104) | 30 (130) | 30 (36) | 30 (50) | 29 (12) | 26 (17) | 11 (7) | 11 (8) |
Notes. The mean S/N value for the detected planets is given in parenthesis. The definition of the S/N and how it is calculated for our data is described in Sect. 6.1.
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