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Table A.1.

Data for the SEDs of the sources presented in Fig. A.1.

Name pa W1 S/NW1 W2 S/NW2 W3 S/NW3 W4 S/NW4 1.4 GHz LFIRe
(Vega)b (Vega) (Vega) (Vega) (mJy) (1012nL⊙)
MAM-850.7 0.052 16.955 ± 0.086 12.6 17.071 ± 0.300 3.6 < 12.839c 0.2 < 8.853c 1.3 < 0.94d 15.4
MAM-850.8 0.017 17.746 ± 0.162 6.7 16.608 ± 0.207 5.3 < 12.933c 0.0 < 9.315c 0.2 < 0.96d 8.68
MAM-850.10 0.055 17.502 ± 0.134 8.1 16.008 ± 0.127 8.6 < 13.069c −1.2 < 9.379c 0.2 < 0.94d 7.89
MAM-850.16 0.091 18.232 ± 0.244 4.4 16.691 ± 0.210 5.2 12.898 ± 0.495 2.2 < 9.12c 0.4 < 0.94d 7.04
MAM-850.18 0.041 16.834 ± 0.073 15.0 16.988 ± 0.287 3.8 < 12.704c 0.5 < 9.565c −0.5 < 0.91d 6.75
MAM-850.26 0.012 18.017 ± 0.202 5.4 < 17.008c 2.0 < 13.130c −0.6 < 9.437c −1.1 < 0.91d 6.05
MAM-850.27 0.014 17.51 ± 0.134 8.1 17.106 ± 0.309 3.5 < 13.017c −0.5 < 8.877c 1.5 < 0.94d 4.83

Notes.

(a)

p-value estimated following Downes et al. (1986).

(b)

We converted the Vega magnitude in the AllWise Source Catalog to mJy following Wright et al. (2010) and a source with Fν ∝ ν−2 (see their Table 2).

(c)

This value is the 95% confidence brightness upper limit from the AllWise Source Catalog.

(d)

Detection limit of the FIRST catalog at source position.

(e)

Far-infrared luminosity measured by integrating the fitted average ALESS SED (Fig. A.1) in the rest-frame range 8–1000 μm.

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