TY - JOUR
T1 - GalevNB
T2 - From simulations to observations
AU - Pang, Xiaoying
AU - Olczak, Christoph
AU - Spurzem, Rainer
AU - Charbonnel, Corinne
AU - Nota, Antonella
N1 - Publisher Copyright:
Copyright © International Astronomical Union 2017.
PY - 2015
Y1 - 2015
N2 - 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 â) to near-IR (160 μm).
AB - 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 â) to near-IR (160 μm).
KW - N-body
KW - magnitude
KW - spectra
UR - http://www.scopus.com/inward/record.url?scp=85016649339&partnerID=8YFLogxK
U2 - 10.1017/S174392131500887X
DO - 10.1017/S174392131500887X
M3 - Article
AN - SCOPUS:85016649339
SN - 1743-9213
VL - 12
SP - 259
EP - 260
JO - Proceedings of the International Astronomical Union
JF - Proceedings of the International Astronomical Union
ER -
