ZASpE: A code to measure stellar atmospheric parameters and their covariance from spectra

Rafael Brahm, Andrés Jordán, Joel Hartman, Gáspár Bakos

Research output: Contribution to journalArticle

29 Scopus citations

Abstract

We describe the Zonal Atmospheric Stellar Parameters Estimator (ZASPE), a new algorithm, and its associated code, for determining precise stellar atmospheric parameters and their uncertainties from high-resolution echelle spectra of FGK-type stars. ZASPE estimates stellar atmospheric parameters by comparing the observed spectrum against a grid of synthetic spectra only in the most sensitive spectral zones to changes in the atmospheric parameters. Realistic uncertainties in the parameters are computed from the data itself, by taking into account the systematic mismatches between the observed spectrum and the best-fitting synthetic one. The covariances between the parameters are also estimated in the process. ZASPE can in principle use any pre-calculated grid of synthetic spectra, but unbiased grids are required to obtain accurate parameters. We tested the performance of two existing libraries, and we concluded that neither is suitable for computing precise atmospheric parameters. We describe a process to synthesize a new library of synthetic spectra that was found to generate consistent results when compared with parameters obtained with different methods (interferometry, asteroseismology, equivalent widths).

Original languageEnglish (US)
Pages (from-to)971-984
Number of pages14
JournalMonthly Notices of the Royal Astronomical Society
Volume467
Issue number1
DOIs
StatePublished - May 1 2017

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Keywords

  • Methods: data analysis
  • Planetary systems
  • Stars: fundamental parameters
  • Techniques: spectroscopic

Fingerprint Dive into the research topics of 'ZASpE: A code to measure stellar atmospheric parameters and their covariance from spectra'. Together they form a unique fingerprint.

  • Cite this