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[ascl:1108.008] PÉGASE-HR: Stellar Population Synthesis at High Resolution Spectra

PÉGASE-HR is a code aimed at computing synthetic evolutive optical spectra of galaxies with a very high resolution (R=10 000, or dlambda=0.55) in the range Lambda=[4000, 6800] Angstroms. PÉGASE-HR is the result of combining the code PÉGASE.2 with the high-resolution stellar library ÉLODIE. This code can also be used at low resolution (R=200) over the range covered by the BaSeL library (from far UV to the near IR), and then produces the same results as PÉGASE.2. In PEGASE-HR, the BaSeL library is replaced by a grid of spectra interpolated from the high-resolution ÉLODIE library of stellar spectra. The ÉLODIE library is a stellar database of 1959 spectra for 1503 stars, observed with the echelle spectrograph ÉLODIE on the 193 cm telescope at the Observatoire de Haute Provence.

Code site:
http://www2.iap.fr/pegase/pegasehr/
Used in:
https://ui.adsabs.harvard.edu/abs/2004A%26A...425..881L
Bibcode:
2011ascl.soft08008L

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ascl:1108.008
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