{
  "id": "2407.01285",
  "version": "v1",
  "published": "2024-07-01T13:39:33.000Z",
  "updated": "2024-07-01T13:39:33.000Z",
  "title": "Search for rotating radio transients in monitoring data for three years",
  "authors": [
    "S. A. Tyul'bashev",
    "M. A. Kitaeva",
    "D. V. Pervoukhin",
    "G. E. Tyul'basheva",
    "E. A. Brylyakova",
    "A. V. Chernosov",
    "I. L. Ovchinnikov"
  ],
  "comment": "A&A, in press, 6 pages, 2 figures, 1 table",
  "categories": [
    "astro-ph.HE"
  ],
  "abstract": "The search for rotating radio transients (RRAT) was done at a frequency of 111 MHz, in daily observations carried out on the radio telescope, a Large Phased Array (LPA) at declinations -9o < decj < +42o. 19 new RRATs were discovered for dispersion measures (DM) from 2.5 to 72.6 pc cm^{-3}. Estimates of the periods were obtained for three RRATs. Two of them (J0408+28; J0440+35) are located at distances of 134 and 136 pc from Sun and are among the closest of all known RRATs.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2024-07-01T13:39:33.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "rotating radio transients",
      "monitoring data",
      "radio telescope",
      "large phased array",
      "dispersion measures"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 6,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}