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Kernel. Application and scientific potentials of full pupil interferometry : Statistical analysis of kernel observables

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Academic year: 2021

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Figure

Fig. 1. Composite image of brown dwarf 2M1207 and its GPCC in H (blue), K s (green) and L ′ (red)
Fig. 3.7 shows the probability mass distribution for a binary at ρ = 74 mas, θ = 315 ◦ and c = 50, in the flux regime shown on the left had side of Fig
Fig. B.1 shows the distributions of the test statistic of T B under H 0 obtained by the AGS, and gradient descent with a random starting point (GDSP)
Fig. 1. Left: entrance pupil for JWST. Centre: discrete model of the pupil. The pupil is modelled by an array of subpupils, enabling the use of the kernel method
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