Open Access

Table B.4

Posterior parameters for the different instruments used in the juliet analysis for TOI-269 b.

Parameter name Posterior estimate Description
Posterior parameters for TESS photometry
MTESS (ppm) Relative flux offset
σw,TESS (ppm) Extra jitter term

Posterior parameters for LCO-CTIO photometry
MLCO (ppm) Relative flux offset
σw,LCO (ppm) Extra jitter term
Parameters of the GP
σGP,LCO (relative flux) Amplitude of the GP
ρGP,LCO (days) Time-scale of the Matern kernel

RV parameters for HARPS
σw,HARPS (m s−1) Extra jitter term

Posterior parameters for ExTrA photometry
Posterior parameters for night 1 of observations
Telescope 2
MExTrA (ppm) Relative flux offset
σw,ExTrA (ppm) Extra jitter term
σGP,ExTrA (relative flux) Amplitude of the GP
ρGP,ExTrA (days) Time-scale of the Matern kernel
Telescope 3
MExTrA (ppm) Relative flux offset
σw,ExTrA (ppm) Extra jitter term
σGP,ExTrA (relative flux) Amplitude of the GP
ρGP,ExTrA (days) Time-scale of the Matern kernel

Posterior parameters for night 2 of observations
Telescope 2
MExTrA (ppm) Relative flux offset
σw,ExTrA (ppm) Extra jitter term
σGP,ExTrA (relative flux) Amplitude of the GP
ρGP,ExTrA (days) Time-scale of the Matern kernel
Telescope 3
MExTrA (ppm) Relative flux offset
σw,ExTrA (ppm) Extra jitter term
σGP,ExTrA (relative flux) Amplitude of the GP
ρGP,ExTrA (days) Time-scale of the Matern kernel

Posterior parameters for night 3 of observations
Telescope 1
MExTrA (ppm) Relative flux offset
σw,ExTrA (ppm) Extra jitter term
σGP,ExTrA (relative flux) Amplitude of the GP
ρGP,ExTrA (days) Time-scale of the Matern kernel
Telescope 2
MExTrA (ppm) Relative flux offset
σw,ExTrA (ppm) Extra jitter term
σGP,ExTrA (relative flux) Amplitude of the GP
ρGP,ExTrA (days) Time-scale of the Matern kernel
Telescope 3
MExTrA (ppm) Relative flux offset
σw,ExTrA (ppm) Extra jitter term
σGP,ExTrA (relative flux) Amplitude of the GP
ρGP,ExTrA (days) Time-scale of the Matern kernel

Notes. The posterior estimate corresponds to the median value. Error bars denote the 68% posterior credibility intervals.

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