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Table 2:

Values plotted in Fig. 8.
Filter $\lambda$ $\nu$(1+z) mag $F_\nu$
  (Å) (1015 Hz)   ($\mu$Jy)
$R_{\rm C}$ 6588 2.17 $18.83\pm0.04$ $90.40 \pm3.33$
v 5402 2.65 $20.03\pm0.2$ $35.38 \pm6.52$
b 4329 3.31 $21.28\pm0.3$ $13.09 \pm3.62$
u 3501 4.09 >22.13 <2.54
uvw1 2634 5.43 >21.33 <2.56
uvm2 2231 6.41 >23.33 <0.41
uvw2 2030 7.05 >21.33 <2.82
The u, uvw1, uvm2 and uvw2 data are upper limits. For all filters except $R_{\rm C}$, $\lambda$ is from Poole et al. (2008). Data refer to t=0.27 days. A redshift of z=3.773 was assumed. The values have been corrected for Galactic extinction. The fluxes have been calculated assuming the conversion factors from Bessell (1979) and Poole et al. (2008).

Source LaTeX | All tables | In the text

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