ARES: Automatic Routine for line Equivalent widths in stella

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ARES: Automatic Routine for line Equivalent widths in stellar Spectra

Post by owlice » Sat May 26, 2012 10:09 am

[c]ARES: Automatic Routine for line Equivalent widths in stellar Spectra[/c][/b]
Abstract: ARES was developed for the measurement of Equivalent Width of absortion lines in stellar spectra; it can also be used to determine fundamental spectroscopic stellar parameters.The code reads a 1D FITS spectra and fits the requested lines in order to calculate the Equivalent width. The code is written in C++ based on the standard method of determining EWs. It automates the manual procedure that one normally carries out when using interactive routines such as the splot routine implemented in IRAF.

Credit: Sousa, Sérgio G.

Site: http://www.astro.up.pt/~sousasag/ares/
http://adsabs.harvard.edu/abs/2007A%26A...469..783S

Bibcode: 2012ascl.soft05009S

ID: ascl:1205.009
Last edited by Ada Coda on Tue Dec 18, 2018 11:17 pm, edited 1 time in total.
Reason: Updated code entry.
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