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Appendix A: Zoom in to individual bands

In this section, we present the spectral energy distribution of our single stellar population models over the J, H and K-bands. Figures A.1 to A.3 present the SEDs at solar metallicity and different ages. Figures A.4 to A.6 present the SEDs at solar metallicity and different ages.

	Fig. A.1 Same as Fig. 7 except over the J-band (1.04−1.44 μm).
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	Fig. A.2 Same as Fig. 7 expect over the H-band (1.46−1.84 μm).
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	Fig. A.3 Same as Fig. 7 expect over the K-band (1.90−2.48 μm).
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	Fig. A.4 Same as Fig. 8 expect over the J-band (1.04−1.44 μm).
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	Fig. A.5 Same as Fig. 8 expect over the H-band (1.46−1.84 μm).
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	Fig. A.6 Same as Fig. 8 expect over the K-band (1.90−2.48 μm).
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Appendix B: Integrated colours and line-strength indices from our models

These are the integrated colours and the line strength indices from the spectral energy distributions of the our single stellar population. The SEDs were convolved to a velocity dispersion of 350 km s^-1 before calculating indices.

© ESO, 2015