{ "id": "1406.6127", "version": "v2", "published": "2014-06-24T02:54:06.000Z", "updated": "2014-07-11T18:58:37.000Z", "title": "Metallicity of M dwarfs IV. A high-precision [Fe/H] and Teff technique from high-resolution optical spectra for M dwarfs", "authors": [ "V. Neves", "X. Bonfils", "N. C. Santos", "X. Delfosse", "T. Forveille", "F. Allard", "S. Udry" ], "comment": "Accepted in Astronomy and Astrophysics. Updated one important reference in the introduction. Some typos corrected", "categories": [ "astro-ph.SR" ], "abstract": "Aims. In this work we develop a technique to obtain high precision determinations of both metallicity and effective temperature of M dwarfs in the optical. Methods. A new method is presented that makes use of the information of 4104 lines in the 530-690 nm spectral region. It consists in the measurement of pseudo equivalent widths and their correlation with established scales of [Fe/H] and $T_{eff}$. Results. Our technique achieves a $rms$ of 0.08$\\pm$0.01 for [Fe/H], 91$\\pm$13 K for $T_{eff}$, and is valid in the (-0.85, 0.26 dex), (2800, 4100 K), and (M0.0, M5.0) intervals for [Fe/H], $T_{eff}$ and spectral type respectively. We also calculated the RMSE$_{V}$ which estimates uncertainties of the order of 0.12 dex for the metallicity and of 293 K for the effective temperature. The technique has an activity limit and should only be used for stars with $\\log{L_{H_{\\alpha}}/L_{bol}} < -4.0$. Our method is available online at \\url{http://www.astro.up.pt/resources/mcal}.", "revisions": [ { "version": "v2", "updated": "2014-07-11T18:58:37.000Z" } ], "analyses": { "keywords": [ "high-resolution optical spectra", "teff technique", "metallicity", "high-precision", "pseudo equivalent widths" ], "tags": [ "journal article" ], "publication": { "doi": "10.1051/0004-6361/201424139", "journal": "Astronomy and Astrophysics", "year": 2014, "month": "Aug", "volume": 568 }, "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "adsabs": "2014A&A...568A.121N" } } }