Abstract
We report on GalevNB (Galev for N-body simulations), an integrated software solution that provides N-body users direct access to the software package GALEV (GALaxy EVolutionary synthesis models). GalevNB is developed for the purpose of a direct comparison between N-body simulations and observations. It converts the fundamental stellar properties of N-body simulations, i.e., stellar mass, temperature, stellar luminosity and metallicity, into observational magnitudes for a variety of filters of widely used instruments/telescopes (HST, ESO, SDSS, 2MASS), and into spectra that span from far-UV (90 Å) to near-IR (160 μm).
| Original language | English |
|---|---|
| Pages (from-to) | 258-259 |
| Number of pages | 2 |
| Journal | Proceedings of the International Astronomical Union |
| Volume | 10 |
| DOIs | |
| Publication status | Published - 2016 |
| Externally published | Yes |
Keywords
- N-body
- magnitude
- spectra
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