Empirical calibration of the near-infrared Ca II triplet - III. Fitting functions
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Spain. | Instituto de Astrof'isica de Canarias | UK. | U. Nottingham | N. Cardiel | A. Cenarro | A. Vazdekis | J. Gorgas | R. G. D. U. A. D. Madrid
[1] Spain.,et al. Empirical calibration of the near-infrared Ca ii triplet — II. The stellar atmospheric parameters , 2001, astro-ph/0109158.
[2] Spain.,et al. Empirical calibration of the near-infrared Ca ii triplet — I. The stellar library and index definition , 2001, astro-ph/0109157.
[3] R. Schiavon,et al. Near-Infrared Spectral Features in Single-aged Stellar Populations , 1999, astro-ph/9910274.
[4] S. Pedraz,et al. Empirical calibration of the \lambda 4000 \AA break , 1999, astro-ph/9905264.
[5] Denis Foo Kune,et al. Starburst99: Synthesis Models for Galaxies with Active Star Formation , 1999, astro-ph/9902334.
[6] A. Vazdekis,et al. Evolutionary Stellar Population Synthesis at 2 Å Spectral Resolution , 1999, astro-ph/9901181.
[7] C. Soubiran,et al. On-line determination of stellar atmospheric parameters $T_{\mathrm{eff}}$, $\log g$, [Fe/H] from ELODIE echelle spectra - II. The library of F5 to K7 stars , 1998, astro-ph/9806234.
[8] A. Bressan,et al. Calcium triplet synthesis , 1998, astro-ph/9802143.
[9] S. Mallik. The Ca II triplet lines as diagnostics of luminosity, metallicity and chromospheric activity in cool stars , 1997 .
[10] D. Ottaviani,et al. Hγ and Hδ Absorption Features in Stars and Stellar Populations , 1997 .
[11] Y. Mayya. Use of Red Supergiant Spectral Features as Age Indicators in Starburst Regions , 1997, astro-ph/9704068.
[12] F. Thévenin,et al. The Infrared CA II Triplet as a Metallicity Indicator of Stellar Populations , 1997 .
[13] R. G. Gratton,et al. Abundances for globular cluster giants: I. homogeneous metallicities for 24 clusters , 1996, astro-ph/9607078.
[14] R. Peletier,et al. A new chemo-evolutionary population synthesis model for early-type galaxies .1. Theoretical basis , 1996, astro-ph/9605112.
[15] C. Sneden,et al. Sodium Abundances in Field Metal-Poor Stars , 1996 .
[16] G. Worthey. Comprehensive stellar population models and the disentanglement of age and metallicity effects , 1994 .
[17] David Burstein,et al. Old stellar populations. 5: Absorption feature indices for the complete LICK/IDS sample of stars , 1994 .
[18] R. Doyon,et al. A NEAR-INFRARED SPECTROSCOPIC STUDY OF THE LUMINOUS MERGER NGC 3256. I: CONSTRAINTS ON THE INITIAL MASS FUNCTION OF THE STARBURST , 1994 .
[19] S. Faber,et al. Old Stellar Populations. IV. Empirical Fitting Functions for Features in the Spectra of G and K Stars , 1993 .
[20] Kenneth R. Lang,et al. Astrophysical Data : Planets and Stars , 1992 .
[21] R. Terlevich,et al. Near-IR features in late type stars: their relation with stellar atmosphere parameters , 1989 .
[22] A. Pickles,et al. THE DWARF STAR CONTENT OF ELLIPTIC AND LENTICULAR GALAXIES , 1986 .
[23] D. Alloin,et al. The infrared CA II triplet - A luminosity indicator for stellar population synthesis. , 1984 .
[24] Michael J. West,et al. The globular cluster system of the Galaxy. III: measurements of radial velocity and metallicity for 60 clusters and a compilation of metallicities for 121 clusters , 1984 .
[25] J. Cohen. Near-infrared luminosity-sensitive features in M dwarfs and giants, and in M31 and M32. , 1978 .