Table 4: Near-IR and optical-UV fluxes.

Object		 $\lambda$(Å) Flux1 $\log(L^2$) Refs.

NGC 4235		 $3.5~{\mu}$m $2.21\times10^{-16}$ 42.13 1
  $2.1~{\mu}$m $\mbox{<}4.49\times10^{-16}$ <42.21 1
  $1.6~{\mu}$m $4.33\times10^{-16}$ 42.08 1
  6030 Å $2.33\times10^{-16}$ 41.62 2
NGC 4639 5487 Å $3.32\times10^{-17}$ 39.87 2
  4316 Å $4.50\times10^{-17}$ 39.90 2
  3004 Å $2.32\times10^{-16}$ 40.45 2
NGC 5033 $3.5~{\mu}$m $2.11\times10^{-16}$ 41.31 1
  $2.1~{\mu}$m $\mbox{<}5.45\times10^{-16}$ <41.50 1
  $1.6~{\mu}$m $3.78\times10^{-16}$ 41.22 1
  $1.1~{\mu}$m $1.51\times10^{-16}$ 40.66 1
  6030 Å $1.04\times10^{-16}$ 40.24 2
  5487 Å $1.08\times10^{-15}$ 41.21 2
  4316 Å $1.51\times10^{-15}$ 41.26 2
NGC 5273 $3.5~{\mu}$m $7.35\times10^{-17}$ 40.97 1
  $1.6~{\mu}$m $1.96\times10^{-16}$ 41.06 1
  $1.1~{\mu}$m $1.69\times10^{-16}$ 40.83 1
  7898 Å $1.44\times10^{-16}$ 40.62 2
  6030 Å $2.86\times10^{-16}$ 40.80 2
  5487 Å $3.60\times10^{-16}$ 40.87 2
  4316 Å $5.43\times10^{-16}$ 40.93 2
  3004 Å $6.73\times10^{-16}$ 40.87 2

1 In erg cm-2 s-1 Å-1; 2 in erg s-1. References: (1) Alonso-Herrero et al. (2003); (2) this work.


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