Free Access

Table 8

2MASS and IRAS flux densities from the literature for the DGS sample.

2MASS IRAS
Source J H K Ref. F 12 F 25 F 60 F 100 Ref.
[mJy] [mJy] [mJy] [Jy] [Jy] [Jy] [Jy]

Haro11 13.0 ± 0.4 13.0 ± 0.6 14.1 ± 0.7 1 0.42 ± 0.05 2.49 ± 0.16 6.48 ± 0.57 5.01 ± 0.61 6
Haro2 43.6 ± 1.4 53.5 ± 2.3 44.9 ± 2.3 2 0.21 ± 0.03 0.95 ± 0.06 4.68 ± 0.41 5.32 ± 0.62 6
Haro3 44.7 ± 1.4 53.2 ± 2.3 37.9 ± 1.9 1 0.21 ± 0.03 0.94 ± 0.06 4.95 ± 0.51 6.75 ± 0.79 6
He2-10 178. ± 6. 201. ± 9. 167. ± 8. 1 1.18 ± 0.14 6.78 ± 0.84 23.4 ± 3.2 26.3 ± 4.7 7
HS0017+1055 0.38 ± 0.01 0.59 ± 0.03 0.36 ± 0.02 3
HS0052+2536 0.54 ± 0.02 0.55 ± 0.02 0.40 ± 0.02 3 0.108 ± 0.005b 0.148 ± 0.009b 0.25 ± 0.02b 0.71 ± 0.07b 6
HS0822+3542 0.15 ± 0.02 0.34 ± 0.04 0.16 ± 0.03 4
HS1222+3741 0.90 ± 0.03 1.18 ± 0.05 0.83 ± 0.04 3
HS1236+3937
HS1304+3529 0.315 ± 0.010 0.27 ± 0.01 0.38 3
HS1319+3224
HS1330+3651
HS1442+4250
HS2352+2733
IZw18 0.75 ± 0.08 0.64 ± 0.07 0.52 ± 0.06 3
IC 10 2051.6 ± 63.9 2972. ± 129. 2632. ± 133. 2
IIZw40 15.1 ± 1.5 21.0 ± 2.2 20.3 ± 2.1 4 0.41 ± 0.04 1.88 ± 0.12 6.02 ± 0.57 1.97 6
Mrk 1089 12.2 ± 0.4 13.9 ± 0.6 12.2 ± 0.6 1 0.25 ± 0.01b 0.70 ± 0.04 4.06 ± 0.26 5.64 ± 0.56 8
Mrk 1450 1.05 ± 0.03 0.90 ± 0.04 0.66 ± 0.03 3 0.06 0.10 0.28 ± 0.04 0.57 6
Mrk 153 4.64 ± 0.56 4.27 ± 0.59 3.63 ± 0.51 4 0.08 0.09 0.28 ± 0.04 0.05 6
Mrk 209 7. ± 1. 8. ± 2. 7. ± 2. 5
Mrk 930 3.52 ± 0.36 4.64 ± 0.48 3.53 ± 0.36 4 0.08 0.23 ± 0.02 1.25 ± 0.12 2.15 6
NGC 1140 48.9 ± 1.5 57.2 ± 2.5 41.8 ± 2.1 2 0.10 ± 0.03 0.49 ± 0.06 3.34 ± 0.38 4.92 ± 0.81 7
NGC 1569 473. ± 49. 547. ± 57. 479. ± 50. 2 0.87 ± 0.08 7.73 ± 0.80 44.0 ± 4.5 47.1 ± 7.5 7
NGC 1705 52.1 ± 1.6 50.9 ± 2.2 41.1 ± 2.1 2 0.05 0.11 0.87 1.82 6
NGC 2366 145. ± 10. 147. ± 13. 110. ± 14. 5 0.12 0.70 ± 0.08 3.51 ± 0.29b 4.67 ± 0.54b 6
NGC 4214 521. ± 16. 614. ± 27. 458. ± 23. 2 0.65 ± 0.07 2.58 ± 0.25 17.9 ± 1.7 29.0 ± 4.3 7
NGC 4449 916. ± 29. 1068.3 ± 46.3 839. ± 42. 2 2.14 ± 0.25b 5.15 ± 0.73 36.6 ± 4.6 73.0 ± 13.5 7
NGC 4861a 16.9 ± 0.5 14.0 ± 0.6 13.1 ± 0.7 2 0.25 ± 0.03b 0.41 ± 0.09b 1.82 ± 0.40b 2.39 ± 0.60b 7
NGC 5253 380. ± 12. 414. ± 18. 334. ± 17. 2 2.81 ± 0.24b 12.3 ± 1.3 29.0 ± 3.0 29.1 ± 4.7 7
NGC 625 218. ± 7. 236. ± 10. 184. ± 9. 2 0.20 ± 0.04 1.30 ± 0.09 5.73 ± 0.37 8.63 ± 0.87 9
NGC 6822a 1619.2 ± 50.4 1753.5 ± 76.0 1362.5 ± 69.0 2 0.25 ± 0.04b 2.46 ± 0.40b 47.6 ± 7.8b 95.4 ± 17.2b 10
Pox186
SBS0335-052 0.303 ± 0.009 0.28 ± 0.01 0.38 3
SBS1159+545
SBS1211+540
SBS1249+493
SBS1415+437
SBS1533+574 1.95 ± 0.06 2.14 ± 0.09 1.54 ± 0.08 3 0.06 0.07 0.26 ± 0.03b 0.4 ± 0.1b 6
Tol0618-402 4.32 ± 0.13 5.84 ± 0.25 4.04 ± 0.20 4
Tol1214-277
UGC 4483 2.20 ± 0.23 0.9 ± 0.1 3.11 ± 0.39 4 0.09 0.09 0.12 0.57 7
UGCA 20
UM133
UM311
UM448 19.3 ± 0.6 22.2 ± 1.0 19.4 ± 1.0 2 0.15 ± 0.04b 0.8 ± 0.1 4.01 ± 0.47 4.30 ± 0.75 7
UM461 2.03 ± 0.21 1.49 ± 0.16 1.27 ± 0.14 4 0.09 0.09 0.12 b 0.57 7
VIIZw403 4.31 ± 0.44 3.89 ± 0.40 2.97 ± 0.31 4 0.07 ± 0.01b 0.06 ± 0.01 0.39 ± 0.05 0.9 ± 0.2b 7

Notes.

(a)

The aperture used does not cover the total emission from the galaxy and the 2MASS magnitudes reported in the database are not consistent with the rest of the IR photometry. Thus we do not consider them for the modelling.

(b)

This IRAS flux density is not consistent with the rest of the IR photometry. Thus we do not consider it for the modelling.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.