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A block test with quoted BAT errors does not reject a common cycle phase for 2S 0114+650 in 2012–2025

We test the phase of the known cycle near 30.8 days in the neutron star binary 2S 0114+650. We use 4,635 accepted daily Swift/BAT rates from 2012 through 2025. The null model has one phase and seven nonnegative amplitudes. Both models fit period, annual means, changing binary profiles, and changing second cycle harmonics. Separate phases improve weighted squared error by 45.72. A restricted residual bootstrap with 128-day sign blocks gives p = 0.311 from 1,999 draws. The common-phase period is 30.72174 days. This test does not reject a common phase at the 5% level. Its calibration assumes approximate sign symmetry of each block's joint errors and independence between blocks. It does not prove a stable physical clock. An added-variance control gives p = 0.048 from 999 draws. This result is near the 5% boundary and limits inference across error rules. All planned controls are reported. A separate MAXI 4–10 keV test gives p = 0.796. Imposed fundamental phase steps from 2020 measure conditional sensitivity for the actual sampling and observed residual noise. We derive calendar intervals from MJD, including 33 BAT rows with following-year labels. Exact source tables, data hashes, selections, code, fitted coefficients, simulations, numerical checks, and figures are preserved.

2S 0114+650 · Swift BAT · MAXI · superorbital cycle · phase coherence · block wild bootstrap · reproducible astronomy

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References

10
  1. usesA BAT point on a notice date reduces conditional cycle prediction gain for 2S 0114+650 in 2023–2026 sci:sha256:fb1d3ce01dee62436198e631e8056b4064374c88f187ab4634e9abfe928a9299

    We exclude two notice dates as described in this earlier BAT analysis. Our question tests phase with period refitted.

  2. 2012–2026 X-ray data do not detect a stable first-order cycle interaction at two fixed periods in 2S 0114+650 sci:sha256:16ac3d4396fe2eec62051442e0f3dbd4f8a484311d90d0750df7deb4d3603d11

    Prior work tested a fixed-period interaction of the binary and long cycles. The present test concerns common fundamental phase.

  3. doi:10.1111/j.1365-2966.2006.10150.x

    Prior discovery of the long cycle.

  4. doi:10.1088/0004-637X/778/1/45

    Prior measurement of the BAT cycle period.

  5. doi:10.3847/1538-4357/aa79a3

    Prior measurements of changing cycle strength and shape.

  6. doi:10.1093/mnras/stad3878

    Phase-resolved spectral study and the binary period used here.

  7. doi:10.1088/0067-0049/209/1/14

    Swift/BAT transient monitor data and method.

  8. doi:10.1093/pasj/61.5.999

    MAXI instrument.

  9. doi:10.1214/aos/1176350142

    Residual resampling in regression is prior methodology.

  10. doi:10.1111/jtsa.12118

    Block wild resampling for serially correlated regression errors is prior methodology. Its results do not prove calibration for this specific test.

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