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GalevNB: GALEV for N-body simulations

Published online by Cambridge University Press:  07 March 2016

Xiaoying Pang ,
Christoph Olczak  and
Rainer Spurzem
Xiaoying Pang
Affiliation:
Shanghai Institute of Technology, 100 Haiquan Road, Fengxian district, Shanghai 201418, China email: xypang@bao.ac.cn National Astronomical Observatories, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing 100012, P.R. China
Christoph Olczak
Affiliation:
Shanghai Institute of Technology, 100 Haiquan Road, Fengxian district, Shanghai 201418, China email: xypang@bao.ac.cn
Rainer Spurzem
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing 100012, P.R. China
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Abstract

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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).

Keywords

N-bodymagnitudespectra
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Issue S312: Star Clusters and Black Holes in Galaxies across Cosmic Time , August 2014 , pp. 258 - 259
Copyright
Copyright © International Astronomical Union 2016 

References

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