GRB 060605: multi-wavelength analysis of the first GRB observed using integral field spectroscopy

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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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