Mass determination of the three long-period Neptune- and sub-Neptune-sized planets transiting TOI-282

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Table B.4

Transit times of TOI-282 b from the LCs + RVs MCMCI analysis with TTVs


T_{b, j} (BJD_TDB)	σ_T0 (days)	O–C (minutes)	Telescope
2 458 344.8135	0.024	−2.17	TESS
2 458 390.5660	0.023	−44.79	TESS
2 458 413.4903	0.016	3.09	TESS
2 458 482.1727	0.017	16.44	TESS
2 458 505.0461	0.011	−9.06	TESS
2 458 527.9499	0.024	9.31	TESS
2 458 550.8404	0.013	8.54	TESS
2 458 573.7825	0.024	81.97	TESS
2 458 619.4928	0.019	−21.43	TESS
2 458 665.2832	0.013	−9.45	TESS
2 459 054.4329	0.026	−6.94	TESS
2 459 077.3150	0.029	−19.78	TESS
2 459 123.0878	0.016	−33.13	TESS
2 459 146.0117	0.023	14.10	TESS
2 459 168.9013	0.012	11.99	TESS
2 459 237.5973	0.024	44.89	TESS
2 459 329.1261	0.014	−6.08	TESS
2 459 352.0039	0.037	−25.12	TESS
2 459 970.0749	0.016	−7.16	TESS
2 459 992.9855	0.018	21.04	TESS
2 460 038.7394	0.031	−19.53	TESS
2 460 130.3380	0.014	29.90	TESS
2 460 176.0815	0.017	−25.68	TESS
2 460 702.5884	0.012	−7.43	TESS

Notes. The O–C values (third column) are computed with respect to the linear ephemeris:

T_ref = 2 458 344.8150 ± 0.0053 BJD_TDB

P_lin = 22.89105 ± 0.00011 days.

The transit times are given in the BJD_TDB standard (Eastman et al. 2010); the second column reports the associated 1-σ error.

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