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The Near-IR Calcium Triplet: Empirical Calibration and Stellar Populations Models

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The Evolution of Galaxies

Abstract

We present a new stellar library at the near-IR spectral range(λ 8350–9020Å, FWHM ~ 1.5 Å) devoted to the empirical calibration of the Ca II triplet (λλ 8498, 8542 and 8662 Å) which consists of 706 stars spanning a wide range in atmospheric parameters (2747 K < Teff < 38367 K, 0.00 < log g < 5.12, and −3.45 < [Fe/H] < +0.60). The atmospheric parameters were determined by bootstrapping literature data against a fix reference system (Soubiran, Katz and Cayrel, 1998), constituting then a highly homogeneous set.

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References

  • Soubiran C., Katz D. and Cayrel R.: 1998, A&AS 133, 221.

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  • Vazdekis, A., Casuso, E., Peletier, R.F. and Beckman, J.E.: 1996, ApJS 106, 307. Vazdekis, A.: 1999, ApJ 513, 224.

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© 2001 Springer Science+Business Media Dordrecht

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Cenarro, A.J., Gorgas, J., Cardiel, N., Pedraz, S., Vazdekis, A., Peletier, R.F. (2001). The Near-IR Calcium Triplet: Empirical Calibration and Stellar Populations Models. In: Vílchez, J.M., Stasińska, G., Pérez, E. (eds) The Evolution of Galaxies. Springer, Dordrecht. https://doi.org/10.1007/978-94-017-3313-7_71

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  • DOI: https://doi.org/10.1007/978-94-017-3313-7_71

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-90-481-5821-8

  • Online ISBN: 978-94-017-3313-7

  • eBook Packages: Springer Book Archive

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