GalevNB: From simulations to observations

Xiaoying Pang; Christoph Olczak; Rainer Spurzem; Corinne Charbonnel; Antonella Nota

doi:10.1017/S174392131500887X

GalevNB: From simulations to observations

Xiaoying Pang
, Christoph Olczak
, Rainer Spurzem
, Corinne Charbonnel
, Antonella Nota

Research output: Contribution to journal › Article › peer-review

Abstract

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).

Original language	English
Pages (from-to)	259-260
Number of pages	2
Journal	Proceedings of the International Astronomical Union
Volume	12
DOIs	https://doi.org/10.1017/S174392131500887X
Publication status	Published - 2015
Externally published	Yes

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This output contributes to the following UN Sustainable Development Goals (SDGs)

SDG 3 Good Health and Well-being

Keywords

N-body
magnitude
spectra

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10.1017/S174392131500887X

Cite this

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title = "GalevNB: From simulations to observations",

abstract = "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 {\^a}) to near-IR (160 μm).",

keywords = "N-body, magnitude, spectra",

author = "Xiaoying Pang and Christoph Olczak and Rainer Spurzem and Corinne Charbonnel and Antonella Nota",

note = "Publisher Copyright: Copyright {\textcopyright} International Astronomical Union 2017.",

year = "2015",

doi = "10.1017/S174392131500887X",

language = "English",

volume = "12",

pages = "259--260",

journal = "Proceedings of the International Astronomical Union",

issn = "1743-9213",

}

TY - JOUR

T1 - GalevNB

T2 - From simulations to observations

AU - Pang, Xiaoying

AU - Olczak, Christoph

AU - Spurzem, Rainer

AU - Charbonnel, Corinne

AU - Nota, Antonella

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 - https://www.scopus.com/pages/publications/85016649339

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 -

GalevNB: From simulations to observations

Abstract

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Keywords

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