GalevNB: GALEV for N-body simulations
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).
- Publication:
-
Star Clusters and Black Holes in Galaxies across Cosmic Time
- Pub Date:
- February 2016
- DOI:
- 10.1017/S1743921315007978
- arXiv:
- arXiv:1504.03282
- Bibcode:
- 2016IAUS..312..258P
- Keywords:
-
- N-body;
- magnitude;
- spectra;
- Astrophysics - Astrophysics of Galaxies;
- Astrophysics - Instrumentation and Methods for Astrophysics
- E-Print:
- IAU 312 proceeding