ARESv2 is an upgraded version of ARES that includes new interesting features:

The features are described in some detail in the paper Sousa et al. (2015 A&A in press.) where the user can see some tests performed using the new features.

This simple code TMCalc is a C code developed as an extension to ARES. Using the line list given it uses the calibration derived for several line-rations to estimate the spectroscopic temperature for FGK dwarf stars and the use the iron lines strenght calibration to derive the metallicity [Fe/H]. The calibration for the metallicity is described in a work (Sousa et al. 2012, A&A, 544, 122) .

ARES is a C code developed for the measurement of Equivalent Width of absortion lines in stellar spectra.
The code reads a 1D FITS spectra and fits the requested lines in order to calculate the Equivalent width.
The Code is described in the paper by Sousa et al. 2007, A&A, 469, 783, where the user can see the results of tests of this code for several types of spectra.

The LineSearcher code, is a derivation from the ARES code. You can use this code to search all the absortion lines in a given wavelength interval. This code returns the center wavelength and estimated depth for each line found in the interval.

This simple code Teff_LR is a C code developed as an extension to ARES. Using the line list given it uses the calibration derived for several line-rations to estimate the spectroscopic temperature for FGK dwarf stars. The line-ratio calibration are described in Sousa et al. 2010, A&A, 512, 13

Please fill the form in order to acess the download page for ARESv2.

Please fill the form in order to acess the download page for ARESv1.

Please fill the form in order to acess the download page for LineSearcher.

Please fill the form in order to acess the download page for Teff_LR_Code.

Please fill the form in order to acess the download page for TMCalc.

For help/support on ARES or other codes please contact Sérgio G. Sousa.