{
  "route": "AC17",
  "frozen_date": "2026-10-28",
  "kind": "independent public science scripts, observed TESS windows and distinct synthetic references; no Engine",
  "sources": [
    "https://arxiv.org/pdf/astro-ph/0210099v1",
    "https://arxiv.org/pdf/1004.3741v1",
    "https://arxiv.org/pdf/1602.01740v1",
    "https://pypi.org/project/batman-package/2.5.3/",
    "https://archive.stsci.edu/missions/tess/tid/s0001/0000/0000/2515/5310/tess2018206045859-s0001-0000000025155310-0120-s_lc.fits"
  ],
  "permissions": {
    "authored_scripts": "MIT; independently authored analysis only",
    "authored_synthetic_inputs_outputs_prose": "CC BY4.0, Sandbox Physics AC17",
    "original_observations": "NASA TESS/SPOC/MAST original public science terms and acknowledgements retained; no new license asserted",
    "external_reference": "batman-package2.5.3 installed independently under GPLv3; no library code redistributed or copied into Engine"
  },
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    "observed PDC flux already crowding/aperture corrected; no repeated corrections",
    "uniform120s window is a readout-kernel approximation",
    "fitted impact reaches zero; retain full conditional profile and source sensitivities",
    "rho_circ assumes circular orbit, not a general density/eccentricity estimate",
    "raw analytic library center-crossing failures retained with independent published special-case and Cartesian checks"
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