Table 1:

Multi-wavelength data. All fluxes are given in mJy.
$\lambda_{\rm obs}$ SDSS J1148+5251 Refs BR 1202-0725 Refs
in $\mu $m z=6.42   z = 4.69  
0.1450a 0.0887 1 $0.23\pm0.02$ 11
1.2 $0.080\pm0.004$b 1 $0.32\pm0.04$b 12
1.6 $0.092\pm0.004$b 2 $0.50\pm0.06$b 12
2.2 $0.11\pm0.005$b 2 $0.41\pm0.08$b 12
3.6 $0.124\pm0.002$ 3 $0.461\pm0.001$ 4
4.5 $0.140\pm0.003$ 3 $0.375\pm0.001$ 4
5.8 $0.133\pm0.010$ 3 $0.410\pm0.001$ 4
8.0 $0.241\pm0.016$ 3 $0.657\pm0.002$ 4
16.0 0.84 3 - -
24.0 $1.520\pm0.130$ 4 $5.1\pm0.6$c 5
70.0 - - $15.0\pm2.0$c 5
100.0 $4.1 \pm 1.0$ 5 - -
160.0 $6.3 \pm 2.0$ 5 $39.8\pm3.7$c 5
350.0 $21\pm6$ 6 $106\pm7$c 13
450.0 $24.7\pm7.4$ 7 $92\pm38$c 14
800.0 - - $50\pm7$c 14
850.0 $7.9\pm0.7$ 7 - -
900.0 - - $59\pm11$c 15
1100.0 - - $21\pm5$c 14
1200.0 $5.0\pm0.6$ 8 - -
1330.0 $3.9\pm0.8$ 9 - -
1350.0 - - $16.0\pm2.2$c 16
2750.0 $0.28\pm0.07$ 9 - -
1.4 GHz $0.055\pm0.8$ 10 $0.315\pm0.080$c 17

Notes. (a) Refers to the 1450 Å flux in the rest frame of the source. (b) Calculated using the zero points presented in Cohen et al. (2003). (c) Total flux including the companion.

References. (1) Fan et al. (2003); (2) Iwamuro et al. (2004); (3) Jiang et al. (2006); (4) Hines et al. (2006); (5) this work; (6) Beelen et al. (2006); (7) Robson et al. (2004); (8) Bertoldi et al. (2003); (9) Riechers et al. (2009); (10) Carilli et al. (2004); (11) Storrie-Lombardi et al. (1996); (12) Skrutskie et al. (2006); (13) Benford et al. (1999); (14) Isaak et al. (1994); (15) Iono et al. (2006); (16) Omont et al. (1996a); (17) Yun et al. (2000).


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