Comparing six evolutionary population synthesis models by performing spectral synthesis for galaxies

X. Y. Chen; Y. C. Liang; F. Hammer; Ph. Prugniel; G. H. Zhong; M. Rodrigues; Y. H. Zhao; H. Flores

doi:10.1051/0004-6361/200913894

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Volume 515 (June 2010)

A&A, 515 (2010) A101

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Table 2:

Selections of ages and metallicities for SSPs from each model, which we use below.
Models	Ages (Gyr)												Metallicities ( $Z_{\odot}$ )
	Young (<0.2 Gyr)				Intermediate (0.2-2 Gyr)				Old (>2 Gyr)
	Y1	Y2	Y3	Y4	I1	I2	I3	I4	O1	O2	O3	O4	Z1	Z2	Z3
BC03, CB07	0.004	0.010	0.064	0.102	0.286	0.509	0.905	1.434	3.00	6.00	10.00	13.00	0.2	1.0	2.5
Ma05	0.004	0.010	0.065	0.100	0.300	0.500	0.900	1.500	3.00	6.00	10.00	13.00	0.5	1.0	2.0
GALEV	0.004	0.012	0.064	0.100	0.280	0.500	0.900	1.432	3.00	6.00	10.00	13.00	0.2	1.0	2.5
GRASIL	0.004	0.010	0.060	0.100	0.300	0.500	0.900	1.500	3.00	6.00	10.00	13.00	0.2	1.0	2.5
Vazdekis/Miles			0.063	0.100	0.280	0.500	0.890	1.410	3.16	6.31	10.00	12.59	0.2	1.0	1.5

Notes. BC03 and CB07 are shown in the same line. See more details in Sect. 4.2.

Source LaTeX | All tables | In the text

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