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GalevNB: from simulations to observations

Published online by Cambridge University Press:  31 March 2017

Xiaoying Pang ,
Christoph Olczak  and
Rainer Spurzem
Xiaoying Pang
Affiliation:
Shanghai Institute of Technology, 100 Haiquan Road, Fengxian district, Shanghai 201418, P.R. 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:
National Astronomical Observatories, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing 100012, P.R. China
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 present GalevNB (Galev for N-body simulations), an utility that converts fundamental stellar properties of N-body simulations into observational properties using the GALEV (GAlaxy EVolutionary synthesis models) package, and thus allowing direct comparisons between observations and N-body simulations. 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 12 , Symposium S316: Formation, evolution, and survival of massive star clusters , August 2015 , pp. 259 - 260
Copyright
Copyright © International Astronomical Union 2017 

References

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