{
  "annotation_id": "32c19b03-44d2-4e7d-888c-cf2d581eea71",
  "date_created": "2026-03-02T18:00:49.903000Z",
  "date_modified": "2026-03-02T18:00:49.903000Z",
  "file_hash": "56b0e24f0aa72ce2d982d981bd19feab0264ccbde751991bf07fd715658b40ed",
  "private": false,
  "record": {
    "abstract": "We propose a numerical method for compensating dispersion effects in optical\ncoherence tomography that does not require a priori knowledge of dispersive\nproperties of the sample. The method is based on the generalized\nautoconvolution function, and its principle of operation can be intuitively\nvisualized using the Wigner distribution function formalism.",
    "arxiv_id": "physics/0404054",
    "authors": [
      "Konrad Banaszek",
      "Aleksandr S. Radunsky",
      "Ian A. Walmsley"
    ],
    "categories": [
      "physics.optics",
      "physics.med-ph",
      "quant-ph"
    ],
    "title": "Blind dispersion compensation for optical coherence tomography",
    "url": "https://arxiv.org/abs/physics/0404054"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "b28a3d79-be36-459a-98be-4bbb0e940312",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}