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Symmetric fits to EK Cep SAP data show a decreasing eclipse phase in 2019–2024

We tested the secondary eclipse phase of EK Cep in 12 public 120-second TESS SPOC light curves. Symmetric profile fits to SAP flux give 107 accepted eclipse centers. Twenty-seven secondary events have accepted primary events on both sides. We multiply their local phase by a fixed 4.427794-day period. Equal weights for nine sector means give a slope of -28.53 seconds per year. The approximate HC3 and Student t 95% interval is -31.88 to -25.18 seconds per year. The fitted decrease between endpoint sector means is 146.46 seconds. SAP baseline, window, profile, edge midpoint, and deletion controls retain the decrease. Four annual means also retain it. This result has the direction and scale of known apsidal motion. A PDCSAP fit gives much larger scatter and an interval that includes zero. In sector 78, secondary cycle 613, its fitted center is 490.53 seconds earlier than the SAP center. A flux shape difference is visible in that event. We do not establish a precise slope change between products or a unique physical cause. Independent synthetic shapes recover fixed and imposed phase slopes within 0.05 seconds per year at the accepted timestamps. These tests do not calibrate total uncertainty. The release adds event times through 2024 and flags a specific product difference. It preserves source FITS files, hashes, code, selection records, results, figures, and repeat instructions.

EK Cep · TIC 322262620 · HD 206821 · TESS · eclipse timing · apsidal motion · SAP · PDCSAP · flux processing · reproducible data

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References

5
  1. usesSymmetric profile fits reproduce the V1143 Cyg eclipse drift in 2019–2024 TESS data sci:sha256:7314d3e9fb684fefa04f22fb950122efe2e17ce1418366f3e244de725236ae85

    We use its compact even eclipse profile family and its local phase approach. We wrote new code for EK Cep. We did not reuse its source code, event data, or error calibration.

  2. usesdoi:10.17909/t9-nmc8-f686

    The public TESS light-curve collection supplies 12 single-sector SPOC 120-second files. The release preserves exact files, identifiers, retrieval times, and hashes.

  3. usesdoi:10.1051/0004-6361/202141484

    This study reports known apsidal motion and an EK Cep eclipse-interval slope. It informed target selection, the search offset, and the benchmark slope. Some early TESS data are shared.

  4. usesdoi:10.1093/mnras/stac1712

    We use its EK Cep primary ephemeris to locate eclipse windows. Its eccentricity and inclination also supply context for a conditional orbit conversion.

  5. usesdoi:10.3847/1538-3881/ae0f9e

    We searched the public target and timing tables of CDS J/AJ/170/322 for TIC 322262620. Both searches returned zero rows, so the catalog cannot provide an individual EK Cep timing comparison. The release records the table hashes and search code.

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