Automatic Routine for line Equivalent widths in stellar Spectra

Details Automatic Routine for line Equivalent widths in stellar Spectra Automatic Routine for line Equivalent widths in stellar Spectra

Jun 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007asd..soft...31s&link_type=abstract

Astrophysics Software Database, CAU Kiel, Germany (http://www1.astrophysik.uni-kiel.de/asd/).

Astronomy and Astrophysics

Astrophysics

C/C++

Scientific paper

ARES is a C++ code developed for the measurement of Equivalent Width of absorption 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 S. G. Sousa, N. C. Santos, G. Israelian, M. Mayor, M. J.P.F.G. Monteiro (2007, A&A - accepted for publication), where the user can see the results of tests of this code for several types of spectra.

Affiliated with

Also associated with

No associations

Rating

Automatic Routine for line Equivalent widths in stellar Spectra does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Automatic Routine for line Equivalent widths in stellar Spectra, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Automatic Routine for line Equivalent widths in stellar Spectra will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-875020