{
  "id": "1807.08121",
  "version": "v1",
  "published": "2018-07-21T10:11:28.000Z",
  "updated": "2018-07-21T10:11:28.000Z",
  "title": "Low resolution spectroscopic investigation of Am stars using Automated method",
  "authors": [
    "Kaushal Sharma",
    "Santosh Joshi",
    "H. P. Singh"
  ],
  "comment": "4 pages, 2 figures, Proceeding for \"First Belgo-Indian Network for Astronomy & Astrophysics (BINA) workshop\", held in Nainital (India), November 15-18, 2016. Published in Bulletin of Li\\`ege Royal Society of Sciences Vol. 87, p. 121-124",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "Automated method of full spectrum fitting gives reliable estimates of stellar atmospheric parameters (Teff, logg and [Fe/H]) for late A, F, G and early K type stars. Recently, the technique was further improved in the cooler regime and the validity range was extended up to M6 - M7 spectral type( Teff $\\sim\\,2900$ K). The present study aims to explore the application of this method on the low-resolution spectra of Am stars, a class of chemically peculiar (CP) stars, to examine its robustness for these objects. We use ULySS with MILES (Medium-resolution INT Library of Empirical Spectra) V2 spectral interpolator for parameter determination. Determined Teff and logg are found to be in good agreement with those obtained from high-resolution spectroscopy.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2018-07-21T10:11:28.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "low resolution spectroscopic investigation",
      "automated method",
      "stellar atmospheric parameters",
      "m7 spectral type",
      "medium-resolution int library"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 4,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}