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Fixed 1102-day timing waves reduce forecast errors for TOI-270 c and d in TESS sectors 97 and 98

We measured 13 transits of TOI-270 c and 6 transits of TOI-270 d in TESS sectors 97 and 98. We tested two forecasts fitted only to published 2018–2020 transit times. One model uses a constant period. The other adds a sine and cosine at a fixed 1102.24-day period. For planet c, the root mean square error falls from 58.55 to 1.65 minutes. For planet d, it falls from 52.60 to 5.46 minutes. The package gives the source light curves, individual times, block-resampling errors, alternate fits, and all analysis code. This test covers a five-year gap between data sets. It tests a simple timing wave with an assumed period. It does not test the published model of planetary motion or determine a new planet mass.

TOI-270 · TESS · transit timing · forecast test · public astronomical data

Admitted 2 citing publications

References

7
  1. usesdoi:10.1093/mnras/stab3483

    Tables A1–A3 supply the early transit times. Table 3 supplies the search periods and transit geometry.

  2. usesdoi:10.17909/t9-nmc8-f686

    Seven SPOC two-minute light curves supply the public observations.

  3. usesdoi:10.1086/683602

    The batman code calculates the transit light curves.

  4. doi:10.1038/s41550-019-0845-5
  5. doi:10.1088/0004-637X/761/2/122
  6. doi:10.1093/mnras/staf334
  7. A sine model gave smaller later timing errors than a linear model for 23 of 26 selected Kepler planet pairs sci:sha256:7cc6a1c1ae9085aad128b73ab10f78f82967c8385e8955219cb2461a5ef0032c

    A prior test compares fixed-period timing waves with clocks for selected Kepler pairs. The present code and TOI-270 measurements are independent.

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