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Table 1

Spitzer mid-IR, submillimeter, and radio data of the selected sample.

IDa IAU name S 24   μm b S 24   μm,spectra c S 350   μm d S 1.2mm a S 20   cm e α f
(μJy) (mJy) (μJy)

L1 SWIRE4_J104351.17+590058.1 664  ±  18 674  ±  38 30.0  ±  10.5 2.95  ±  0.66 76.3  ±  9.0 –0.84
L3 SWIRE4_J104410.00+584056.0 589  ±  12 495  ±  80 ... 1.04  ±  1.11 105.5  ±  35.0 +0.86
L5 SWIRE4_J104427.52+584309.6 542  ±  11 645  ±  26 ... 2.75  ±  0.76 71.0  ±  20.0 –1.03
L7 SWIRE4_J104430.60+585518.6 825  ±  13 871  ±  105 ... 1.39  ±  0.79 101.7  ±  13.3 –0.81
L9 SWIRE4_J104440.25+585928.3 653  ±  14 586  ±  109 55.1  ±  17.1 4.00  ±  0.55 116.5  ±  9.2 –0.54
L10 SWIRE4_J104549.77+591904.0 626  ±  12 605  ±  76 ... 1.39  ±  0.81 67.2  ±  11.7 –0.40
L11 SWIRE4_J104556.90+585318.8 661  ±  13 825  ±  55 38.9  ±  5.8 3.08  ±  0.58 314.8  ±  4.1 –0.45
L14 SWIRE4_J104638.68+585612.5 631  ±  13 661  ±  48 29.7  ±  4.9 2.13  ±  0.71 159.5  ±  6.0 –0.73
L15 SWIRE4_J104656.46+590235.5 579  ±  14 695  ±  41 25.7  ±  5.9 2.36  ±  0.62 68.6  ±  3.7 –1.03
L17 SWIRE4_J104704.97+592332.3 644  ±  14 629  ±  83 45.3  ±  12.4 2.24  ±  0.64 341.0  ±  33.0 –0.76
L19 SWIRE4_J104708.78+590627.2 556  ±  14 618  ±  42 ... 0.89  ±  0.97 102.2  ±  12.0 –0.44
L20 SWIRE4_J104717.96+590231.7 692  ±  15 558  ±  107 51.6  ±  7.2 2.66  ±  0.78 51.1  ±  4.7 –1.25
L25 SWIRE4_J104738.32+591010.0 704  ±  13 667  ±  74 36.1  ±  7.1 2.56  ±  0.74 69.0  ±  9.0 –1.09
L27 SWIRE4_J104744.60+591413.5 533  ±  13 591  ±  50 27.4  ±  7.9 2.48  ±  0.73 77.2  ±  13.7 –0.38
L31 SWIRE4_J104830.70+585659.3 640  ±  16 640  ±  101 ... 1.62  ±  0.60 121.0  ±  39.0 –0.31
L33 SWIRE4_J104848.23+585059.3 536  ±  15 487  ±  61 ... –0.28  ±  1.09 109.0  ±  33.0 +0.27

Notes.

(a)

IDs and S1.2   mm are the same as F09. The bold values are  >3σ detections;

(b)

S24   μm comes from the internal SWIRE catalogue;

(c)

S24   μm,spectra is calculated by convolution of the 24 μm MIPS filter and our spectra;

(d)

S350   μm comes from Kovács et al. (2010);

(e)

S20   cm comes from Owen & Morrison (2008);

(f)

The radio spectral index α is calculated using the best power law fit, Sν ∝ να, between S20   cm, S50   cm, and S90   cm as reported in F09.

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