{
  "id": "2308.15759",
  "version": "v1",
  "published": "2023-08-30T04:58:17.000Z",
  "updated": "2023-08-30T04:58:17.000Z",
  "title": "Chi-square test of the relativistic precession model through the neutron star IGR J17511-3057",
  "authors": [
    "Ivan Z. Stefanov"
  ],
  "comment": "13 pages, 3 figures",
  "categories": [
    "astro-ph.HE",
    "gr-qc"
  ],
  "abstract": "The aim of the current paper is to apply the method of Bambi (Bambi, 2015) to a source which contains two or more simultaneous triads of variability components. The joint chi-square variable that can be composed in this case, unlike some previous studies, allows the goodness of the fit to be tested. It appears that a good fit requires one of the observation groups to be disregarded. Even then, the model prediction for the mass of the neutron star in the accreting millisecond pulsar IGR J17511-3057 is way too high to be accepted.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2023-08-30T04:58:17.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "relativistic precession model",
      "neutron star igr",
      "chi-square test",
      "accreting millisecond pulsar igr",
      "current paper"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 13,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}