Medium-resolution isaac newton telescope library of empirical spectra

  • P. Sanchez-Blazquez*
  • , R. F. Peletier
  • , J. Jimenez-Vicente
  • , N. Cardiel
  • , A. J. Cenarro
  • , J. Falcon-Barroso
  • , J. Gorgas
  • , S. Selam
  • , A. Vazdekis
  • *Corresponding author for this work

Research output: Contribution to journalArticleAcademicpeer-review

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Abstract

A new stellar library developed for stellar population synthesis modelling is presented. The library consists of 985 stars spanning a large range in atmospheric parameters. The spectra were obtained at the 2.5-m Isaac Newton Telescope and cover the range lambda lambda 3525-7500 angstrom at 2.3 angstrom (full width at half-maximum) spectral resolution. The spectral resolution, spectral-type coverage, flux-calibration accuracy and number of stars represent a substantial improvement over previous libraries used in population-synthesis models.

Original languageEnglish
Pages (from-to)703-718
Number of pages16
JournalMonthly Notices of the Royal Astronomical Society
Volume371
Issue number2
DOIs
Publication statusPublished - 11-Sept-2006

Keywords

  • atlases
  • stars : fundamental parameters
  • galaxies : stellar content
  • OLD STELLAR POPULATIONS
  • EARLY-TYPE GALAXIES
  • ABSORPTION-LINE SPECTRA
  • INFRARED CAII TRIPLET
  • METAL-RICH STARS
  • GLOBULAR-CLUSTERS
  • K-STARS
  • SPECTROPHOTOMETRIC ATLAS
  • INTERSTELLAR EXTINCTION
  • ABUNDANCE ANALYSIS

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