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Table 11

Tcold and Twarm obtained from fitting a black-body model to FIR+mm and NIR peak emission, respectively.

Source Tcold Twarm Tbol Lbol Lbol /Lsubmm Mdisk /Menv Inc. αIR βmm αIR (*) Tbol (*)
[K] [K] [K] [10−2L] [deg] [K]
AzTEC-lup1-2 8.3 ± 0.2 ... 10 ± 1 1.0 ± 0.3 1.7 0 ... ... ... ... ...
AzTEC-lup3-5 10.9 ± 0.3 1000 ± 200 164 ± 53 0.6 ± 0.2 1.0 0 ... 0.78 ... ... ...
IRAS 16059-3857 30.3 ± 0.6 900 ± 300 42 ± 5 17 ± 2 0.8 3.6 53 ± 2 0.26 0.2 1.10 – 1.14 39 – 39
IRAS 15398-3359 33.1 ± 0.9 700 ± 300 68 ± 27 110 ± 48 2.6 0.4 66 ± 14 0.60 0.1 ... 48
J160115-41523 29.3 ± 0.6 1150 ± 40 90 ± 13 15.3 ± 0.7 18.9 0.3 66 ± 3 −0.73 0.8 −0.19 – −0.26 130 – 150
Sz 102 144 ± 6 4300 ± 300 460 ± 140 7 ± 2 135 58 ± 3 0.76 0.1 0.72 – 0.63 810 – 3100
Merin 28 270 ± 20 750 ± 70 529 ± 1 7.8 ± 0.1 155 68 ± 1 0.16 0.4 0.22 – 0.71 560 – 640

Notes. Tbol and Lbol values were obtained applying two different integration methods and averaging between them (Simpson and Trapezoidal rules). The Mdisk /Menv values were calculated as the ratio between the emission measured with the 12m and the 7m-12m array (this ratio diverges for Sz 102 and Merin 28). (*)The last two columns include values for IR spectral index (measured between 2 and 24 μm) and Tbol extracted from Dunham et al. (2015) (uncorrected-corrected by extinction). IRAS 15398-3359 was not reported in that paper. IRAS 15398-3359 Tbol from Evans et al. (2009).

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