Open Access

Table 1

Observational parameters for TOI-5720 b, TOI-6008 b, and TOI-6086 b: date of the observation, filter, telescope, exposure time(s), and FWHM of the point-spread function and photometric aperture.

Planet Date (UT) Filter Telescope Exptime [second] FWHM [arcsec] Aperture [arcsec] Baseline βw βr CF Comment
May 12 2023 zs MuSCAT3 17 3.3 4.5 p(t2) 1.26 1.08 1.36 Full
TOI-5720 b May 12 2023 i′ MuSCAT3 19 3.3 4.5 p(t2 + b1) 1.22 1.04 1.27 Full
May 12 2023 r′ MuSCAT3 25 2.9 4.5 p(t2 + b1) 1.26 1.09 1.37 Full
May 12 2023 g′ MuSCAT3 209 2.6 4.5 p(t2 + a1) 0.92 1.07 0.99 Full

May 07 2023 zs MuSCAT3 20 2.1 3.2 p(t2) 1.13 1.45 1.64 Full
May 07 2023 i′ MuSCAT3 30 2.2 3.2 p(t2) 1.13 1.20 1.36 Full
May 07 2023 r′ MuSCAT3 88 2.3 3.2 p(t2) 1.24 1.22 1.52 Full
May 13 2023 zs MuSCAT3 20 2.9 4.5 p(t2 + b1) 1.17 1.23 1.44 Full
May 13 2023 i′ MuSCAT3 30 3.5 4.8 p(t2) 1.16 1.30 1.51 Full
May 13 2023 r′ MuSCAT3 88 3.5 5.0 p(t2 + a2) 1.11 1.02 1.13 Full
TOI-6008 b May 13 2023 g′ MuSCAT3 500 3.4 5.0 p(t2) 0.85 1.23 1.04 Full
May 31 2023 zs MuSCAT3 20 2.6 4.0 p(x2) 1.15 2.46 2.82 Full
May 31 2023 i′ MuSCAT3 30 2.9 4.2 p(b2) 1.09 1.51 1.64 Full
May 31 2023 r′ MuSCAT3 88 2.7 4.2 p(t2) 1.05 1.19 1.26 Full
July 27 2023 zs MuSCAT2 30 2.1 4.3 p(t2) 1.02 1.31 1.34 Full
July 27 2023 i′ MuSCAT2 30 2.4 4.4 p(t2) 1.01 1.08 1.09 Full
July 27 2023 r′ MuSCAT2 88 2.5 4.5 p(t2) 0.98 1.18 1.18 Full
July 27 2023 g′ MuSCAT2 30 2.7 4.5 p(t2) 1.00 1.04 1.04 Full

July 06 2023 zs MuSCAT3 35 2.4 4.8 p(t2) 0.97 1.00 0.97 Full
July 06 2023 i′ MuSCAT3 43 2.3 4.8 p(t2) 0.95 1.00 0.95 Full
July 06 2023 r′ MuSCAT3 63 2.5 4.8 p(t2 + b1) 1.04 1.00 1.04 Full
July 31 2023 zs MuSCAT3 35 4.1 6.9 p(t2) 1.33 1.22 1.49 Full
July 31 2023 i′ MuSCAT3 43 4.3 6.9 p(t2) 1.16 1.04 1.21 Full
TOI-6086 b July 31 2023 r′ MuSCAT3 63 4.3 6.9 p(t2) 1.01 1.14 1.15 Full
July 29 2023 zs MuSCAT2 20 2.1 10.9 p(t2) 0.95 1.00 0.95 Full
July 29 2023 i′ MuSCAT2 20 2.1 10.9 p(t2) 1.02 1.09 1.011 Full
July 29 2023 r′ MuSCAT2 40 2.5 10.9 p(t2) 1.00 1.09 1.09 Full
July 29 2023 g′ MuSCAT2 25 2.8 10.9 p(t2) 1.00 1.36 1.36 Full

Notes. The analysis parameters are the selected baseline model, red noise βr, white noise βw and CF (Correction Factor). The baseline model is shown as a polynomial p() of systematic parameters, with t is the time, x and y are the positions of the star on the detector, a is the airmass, b is the background, and f is the full with at half maximum of the PSF.

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