SP_ACE spectral analysis tool

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.zah.uni-heidelberg.de/sp_ace/q/dist/static/tutorial.pdf .. _download page: http://dc.zah.uni-heidelberg.de/sp_ace/q/dist/static .. _sample spectrum: http://dc.zah.uni-heidelberg.de/sp_ace/q/c/static/fast_spectrum.txt

Identifier
Source https://dc.g-vo.org/rr/q/lp/custom/org.gavo.dc/sp_ace/q/c
Related Identifier http://dc.zah.uni-heidelberg.de/sp_ace/q/c/info
Related Identifier http://dc.zah.uni-heidelberg.de/SP_ACE
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://org.gavo.dc/sp_ace/q/c
Provenance
Creator Boeche, C.; Demleitner, M.; Heinl, H.
Publisher The GAVO DC team
Publication Year 2014
Rights 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.
OpenAccess true
Contact GAVO Data Center Team <gavo(at)ari.uni-heidelberg.de>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Interdisciplinary Astronomy; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy