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Table 9

DGS and KINGFISH dust parameters.

Name Log[Mdust] [Gr] Log[Mdust] [Ac] Log[LTIR] f PAH U σU T dust U min ΔU α T MIR,BB
Log[M] Log[M] Log[L] [fPAH] [U] [U] [K] [U] [U] [K]
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11)

DGS
Haro11 35.5 10.75 3.86 × 105 1.95
Haro2 27.9 3.02 8.35 × 105 2.10
Haro3 26.0 1.95 6.60 × 105 2.10
He2-10 26.7 2.14 3.77 × 105 2.03
HS0017+1055 ≤ 0.05 30.3 4.19 2.39 × 106 1.96
HS0052+2536 25.4 1.79 2.01 × 105 2.15
HS0822+3542 ≤ 0.00 c 25.6 1.90 9.97 × 104 2.16
HS1222+3741 ≤ 0.17 27.3 2.56 1.03 × 106 2.06
HS1236+3937
HS1304+3529 ≤ 0.00 c 30.3 5.74 2.44 × 105 2.28
HS1319+3224 ≤ 0.00 c 27.3 2.65 3.67 × 105 2.11
HS1330+3651 ≤ 0.13 24.1 1.38 8.57 × 103 2.21
HS1442+4250 ≤ 0.20 25.3 0.25 5.35 × 102 1.29
HS2352+2733 ≥ 4.00 a b 51.6 a
IZw18 ≤ 0.03 48.6 204.65 4.31 × 101 1.00 100.
IC 10 21.2 0.65 9.52 × 105 2.21
IIZw40 28.2 2.59 5.67 × 103 1.91 113.
Mrk 1089 24.3 1.38 4.57 × 104 2.14
Mrk 1450 29.4 2.35 1.16 × 103 1.66 100.
Mrk 153 ≤ 0.00 36.6 17.48 1.37 × 105 2.26
Mrk 209 ≤ 0.03 31.0 5.73 2.68 × 105 2.10
Mrk 930 20.4 0.28 1.21 × 103 1.75 105.
NGC 1140 22.8 0.96 7.97 × 104 2.17
NGC 1569 28.4 3.22 3.05 × 103 2.05 100.
NGC 1705 17.7 0.12 3.16 × 102 1.74
NGC 2366 18.9 0.19 4.43 × 103 1.80
NGC 4214 17.6 0.17 3.75 × 103 1.99
NGC 4449 22.4 0.92 1.60 × 104 2.26
NGC 4861 19.5 0.30 7.13 × 104 1.97
NGC 5253 25.2 1.48 3.71 × 105 2.01
NGC 625 20.0 0.41 4.31 × 105 2.10
NGC 6822 ≤ 0.21 11.9 0.01 7.72 × 101 1.71
Pox186 ≤ 0.00 c 16.7 0.12 9.99 × 104 1.99 147.
SBS0335-052 ≤ 0.24 64.4 1088.17 1.00 1.00 123., 273
SBS1159+545 ≤ 0.12 25.0 1.38 1.01 × 106 1.98 150.
SBS1211+540 ≤ 0.18 34.9 13.38 4.86 × 106 2.27
SBS1249+493 ≤ 0.00 25.7 1.95 3.91 × 105 2.15
SBS1415+437 ≤ 0.64 35.3 13.83 5.87 × 105 2.23
SBS1533+574 27.2 2.99 5.51 × 103 2.26 100.
Tol0618-402 b
Tol1214-277 ≤ 0.98 20.0 0.01 4.45 × 101 1.00 102.
UGC 4483 ≤ 0.00 c 36.3 18.90 2.37 × 105 2.45
UGCA 20
UM133 ≤ 0.00 c 30.5 6.31 1.46 × 105 2.35
UM311 14.4 0.01 9.36 1.27
UM448 30.9 6.05 7.26 × 105 2.19
UM461 ≤ 0.04 27.7 2.68 1.53 × 105 2.03 150.
VIIZw403 ≤ 0.00 c 25.8 1.94 8.28 × 103 2.13

KINGFISH
NGC 0337 22.2 0.89 2.54 × 104 2.28
NGC 0584
NGC 0628 19.5 0.46 7.40 × 101 2.50
NGC 0855 17.1 0.12 4.72 × 102 1.85
NGC 0925 12.6 0.01 7.87 1.51
NGC 1097 21.0 0.64 1.87 × 106 2.26
NGC 1266 29.6 5.02 6.17 × 106 2.29
NGC 1291 ≤ 0.00 c 17.5 0.24 1.04 × 102 2.50
NGC 1316
NGC 1377 26.1 1.33 7.28 × 103 1.79
NGC 1404
IC 0342 21.1 0.74 6.18 × 105 2.50
NGC 1482 26.7 2.67 2.14 × 106 2.27
NGC 1512 13.9 0.03 4.13 × 101 1.85
NGC 2146 29.1 4.80 3.89 × 105 2.37
HoII ≤ 0.00 c 21.8 0.75 3.83 × 105 2.20
DDO053 24.4 1.57 5.23 × 105 2.30
NGC 2798 28.0 3.37 6.04 × 106 2.19
NGC 2841 19.2 0.58 1.00 2.50
NGC 2915 12.5 0.01 6.00 × 101 1.58
HoI 11.5 0.01 3.85 × 102 1.80
NGC 2976 21.0 0.72 7.60 × 101 2.50
NGC 3049 16.5 0.11 6.99 × 103 1.95
NGC 3077 14.8 0.01 2.98 × 101 1.30
M81dwB ≤ 0.21 12.0 0.01 2.90 × 101 1.67
NGC 3190 21.3 0.79 4.86 × 101 2.50
NGC 3184 19.8 0.53 7.56 2.50
NGC 3198 14.1 0.01 5.62 1.25
IC 2574 ≤ 0.06 13.2 0.03 2.75 × 102 1.88
NGC 3265 22.2 0.71 1.49 × 104 2.03
NGC 3351 20.9 0.71 1.26 × 106 2.50
NGC 3521 21.7 0.94 1.38 × 101 2.50
NGC 3621 17.1 0.02 6.64 1.00
NGC 3627 22.9 1.22 7.64 × 106 2.50
NGC 3773 21.4 0.66 3.97 × 104 2.17
NGC 3938 20.5 0.63 6.19 × 101 2.50
NGC 4236 ≤ 0.17 11.9 0.01 2.48 × 101 1.68
NGC 4254 22.2 1.01 2.33 × 106 2.50
NGC 4321 21.9 1.09 5.73 2.50
NGC 4536 20.8 0.53 1.35 × 104 2.14
NGC 4559 13.7 0.01 1.06 × 101 1.36
NGC 4569 20.4 0.61 1.51 × 106 2.50
NGC 4579 19.6 0.49 2.20 × 106 2.50
NGC 4594 19.5 0.48 1.27 1.00
NGC 4625 15.4 0.01 4.76 1.07
NGC 4631 22.3 1.05 8.47 × 103 2.50
NGC 4725
NGC 4736
DDO154
NGC 4826 26.1 3.95 4.53 2.42
DDO165
NGC 5055 21.2 0.98 2.77 2.50
NGC 5398 12.1 0.01 6.34 × 101 1.66
NGC 5408 13.0 0.01 1.93 × 103 1.55
NGC 5457 15.9 0.01 5.40 1.04
NGC 5474 14.2 0.04 2.52 × 102 1.96
NGC 5713 24.6 1.61 9.18 × 105 2.26
NGC 5866 25.6 4.00 1.84 2.37
NGC 6946 21.6 0.85 1.65 × 106 2.50
NGC 7331 21.5 0.87 2.10 × 101 2.50
NGC 7793 14.2 0.01 7.65 1.27

Notes. (1) Dust masses derived using graphite for the carbonaceous component, in M; (2) dust masses derived using amorphous carbons for the carbonaceous component, in M; (3) total infrared luminosity, from the best-fit model and integrated between 1 and 1000 μm, in L; (4) PAH mass fraction, normalised to the Galactic value fPAH = 4.57%; (5) mass-averaged starlight intensity, computed with Eq. (1), normalised to the Galactic value U = 2.2 × 10-5 W m-2; (6) standard deviation of the starlight intensity distribution, computed with Eq. (2), normalised to the Galactic value U; (7) average dust temperature, in Kelvins, computed by integrating Eq. (1) over T = TMW × U1/(4+β), with β = 2.0, and TMW = 19.7 K from Planck Collaboration XI (2014); (8) minimum value of the starlight intensity, normalised to the Galactic value U; (9) difference between the maximum and minimum values of the starlight intensity distribution, normalised to the Galactic value U; (10) index of the power law describing the starlight intensity distribution; (11) temperature of the additional MIR modBB, in Kelvins.

(a)

Dust mass and temperature obtained from a modBB fit (see Sect. 3.2.2).

(b)

LTIR obtained from Galametz et al. (2013b) calibrations as no SED fit was possible for this galaxy.

(c)

In these galaxies the fit converges towards 0: no PAH are detected and it is not possible to give an upper limit with the method described in Sect. 4.3.

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