ivo://org.gavo.dc/sp_ace/q/distThe GAVO DC teamBoeche, C.Demleitner, M.Heinl, H.2015-11-302016-02-042016-07-282017-06-212017-12-042019-08-122020-07-17GAVO Data Centre Team

Mönchhofstrasse 12-14, D-69120 Heidelberg

gavo@ari.uni-heidelberg.de+49 6221 54 1837stellar-abundancesspectroscopystellar-atmospheresastronomy-data-analysis SP_ACE computes stellar parameters (gravity, temperature) and element abundances from optical stellar spectra (`sample spectrum`_). It employs 1D stellar atmosphere models in Local Thermodynamic Equilibrium (LTE). The present service does not offer all the options available for SP_Ace as documented in `the tutorial`_. All options are available if running SP_Ace locally (cf. `download page`_). This service exposes an updated version containing some bug fixes with respect to the one described in the paper. .. _the tutorial: http://dc.g-vo.org/sp_ace/q/dist/static/tutorial.pdf .. _download page: http://dc.g-vo.org/sp_ace/q/dist/static .. _sample spectrum: http://dc.g-vo.org/sp_ace/q/c/static/fast_spectrum.txt2016A&A...587A...2Bhttps://dc.g-vo.org/sp_ace/q/dist/info If you use results obtained by this service, please cite the original publication (see source meta) and acknowlege: This work has made use of the sp_ace spectral analysis tool version 1.4.