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Table 2.

Best fit relative fluxes of the T Tau system from an MCMC fit of the kernel phase triple model to the VISIR-NEAR data.

Filter λ [μm] Star Rel. flux σemp Flux [Jy]
ARIII 8.98 N 1.000 0 8.12 ± 0.13
ARIII 8.98 Sa 0.02 4.34 ± 0.11
ARIII 8.98 Sb 0.02 0.10 ± 0.08

SIV_1 9.81 N 1.000 0 9.81 ± 0.16
SIV_1 9.81 Sa 0.02 2.68 ± 0.07
SIV_1 9.81 Sb 0.02 0.02 ± 0.05

SIV_2 10.71 N 1.000 0 10.04 ± 0.19
SIV_2 10.71 Sa 0.02 4.05 ± 0.13
SIV_2 10.71 Sb 0.02 0.66 ± 0.10

NEII 12.80 N 0.03 9.63 ± 0.43
NEII 12.80 Sa 1.000 0 10.64 ± 0.42
NEII 12.80 Sb 0.03 1.23 ± 0.32

Notes. We also report an empirical uncertainty (σemp) for the relative fluxes (see Sect. 4.4) as well as the final photometry of T Tau N, Sa, and Sb in all filters.

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