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Table 3

Transit times of K2-24b and K2-24c measured or adopted for our dynamical analysis.

Planet Instrument T0 (BJDTDB) Source
-b K2 2456 905.79529 ± 0.00035 This work
-c K2 2456 915.62477 ± 0.00021 This work
-b K2 2456 926.67909 ± 0.00049 This work
-b K2 2456 947.56565 ± 0.00035 This work
-c K2 2456 957.98825 ± 0.00019 This work
-b K2 2456 968.45070 ± 0.00033 This work
-b Spitzer 2457 323.61610 ± 0.00110 P18
-c Spitzer 2457 339.00020 ± 0.00140 P18
-c Spitzer 2457 550.50740 ± 0.00150 P18
-b Spitzer 2457 553.50490 ± 0.00160 P18
-b HST 2457 574.40950 ± 0.00350 This work
-b CHEOPS 2459 391.82076 ± 0.00064 This work, b1
-b CHEOPS 2459 412.70870 ± 0.00125 This work, b2
-c CHEOPS 2459413.46115 ± 0.00094 This work, c1
-c CHEOPS 2459 667.64590 ± 0.00175 This work, c2
-b CHEOPS 2459 705.07047 ± 0.00082 This work, b3
-c CHEOPS 2459 710.02459 ± 0.00054 This work, c3
-b CHEOPS 2 459 725.94986 ± 0.00062 This work, b4
-b CHEOPS 2459 746.83330 ± 0.00320 This work, b5
-c CHEOPS 2 459 752.39985 ± 0.00093 This work, c4
-c CHEOPS 2460 049.00500 ± 0.00076 This work, c5
-c CHEOPS 2460 091.36711 ± 0.00105 This work, c6
-b CHEOPS 2460 101.84061 ± 0.00066 This work, b6
-b CHEOPS 2460 122.73033 ± 0.00066 This work, b7

Notes. The columns give the following: planet name (K2-24b or K2-24c), instrument used, best-fit transit time T0 in the BJD-TDB standard (Eastman et al. 2010) along with its 1-σ error bar (symmetrized), and the source (plus the light curve ID from Table A.1 for the CHEOPS data). All the T0 values from this work were obtained through the global photometric fit described in Section 3.

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