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Table 1

Details of the parameters used for our SED fitting.


Photometry NUV, FUV, u,g,r,i,z,Y,J,H,K U,B,V,R,I,z,J,H,K
IRAC (3.6 μm, 4.5 μm) IRAC (3.6 μm, 4.5 μm)

Ages 51 ages (in the range 0.1 Gyr to 14.5 Gyr)

IMF Chabrier (2003)

Metallicities Z = 1, 0.4, 0.2 Z

Dust extinction law Calzetti et al. (2000), SMC-like law (Arnouts et al. 2013)

E(BV) 0, 0.05, 0.1, 0.15, 0.2, 0.25, 0.3, 0.4, 0.5, 0.6, 0.7

Star formation histories Exponential (τ = 0.1,0.3,1,3,5,10,30 Gyr) and delayed exponential (1, 3 Gyr delay)

Notes. We use the publicly available photometry in the COSMOS field: GALEX – Zamojski et al. (2007); Subaru – Capak et al. (2007); Ultra-Vista – McCracken et al. (2012); Spitzer-IRAC – Sanders et al. (2007). For the ECDFS we use the photometry compilation by Cardamone et al. (2010).

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