{
  "id": "2010.02077",
  "version": "v1",
  "published": "2020-10-05T15:15:50.000Z",
  "updated": "2020-10-05T15:15:50.000Z",
  "title": "Study of the Dependence of the Plateau Shape for Type II Supernovae on Metallicity",
  "authors": [
    "A. A. Goldshtein",
    "S. I. Blinnikov"
  ],
  "comment": "14 pages, 10 figures",
  "journal": "Astronomy Letters 46(5) (2020) 312-318; Pis'ma v Astron.Zh 46(5) (2020) 333-339",
  "doi": "10.1134/S1063773720050047 10.31857/S0320010820050046",
  "categories": [
    "astro-ph.HE"
  ],
  "abstract": "We consider the effect of a change in the rate of flux decline in the U band for type II-P supernovae (SNe IIP) as a function of metallicity $Z$. Based on this effect, we propose a new method to determine the photometric redshift from the SN IIP light curve in the U band. Using the STELLA code, we have constructed model light curves in different bands for different redshifts $z = 0.0, 0.1$, and $0.3$ as the metallicity in the models decreases from $Z \\sim 10^{-3}$ to $\\sim 10^{-6}$. The flux in the U band is shown to reach a plateau at the lowest metallicities. We consider the influence of other parameters as well: the presupernova mass and the mass of radioactive nickel-56.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2020-10-05T15:15:50.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "plateau shape",
      "metallicity",
      "sn iip light curve",
      "dependence",
      "constructed model light curves"
    ],
    "tags": [
      "journal article"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 14,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}