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Table 3

Flux densities of NGC 4214 for an aperture of 5′ radius centred at RA  =  12h15m39.1s Dec  =  +36°19′345 (J2000) (see Fig. 2).

Band λ0 (μm) (Jy) C color FDISK (Jy) FDIFF (Jy)

IRAC8 7.872 0.678 0.590 1.149  ±  0.115 0.695
MIPS24 23.680 2.050 0.986 2.080  ±  0.208 0.625
MIPS70 71.440 23.945 0.893 26.814  ±  5.363 13.417
PACS70 70.000 24.209 0.982 24.652  ±  2.466 11.703
PACS100 100.000 35.309 0.985 35.847  ±  3.585 21.128
PACS160 160.000 34.097 1.010 33.759  ±  3.376 22.967
MIPS160 155.900 39.016 0.971 38.574  ±  7.715 27.287
SPIRE250 250.000 18.888 0.992 19.033  ±  2.855 14.594
Planck350 350.000 9.546 0.986 9.682  ±  0.988 7.933
SPIRE350 363.000 10.059 0.999 10.068  ±  1.510 8.453
SPIRE500 517.000 4.497 1.025 4.387  ±  0.659 3.848
Planck550 550.000 3.635 0.921 3.947  ±  1.318 3.510
Planck850 850.000 0.946 0.887 1.066  ±  0.264 0.958
MAMBO* 1200.000 0.350 1.000 0.350  ±  0.106 0.288

Notes.  is the measured, background-subtracted flux, FDISK is the final flux of the entire galaxy, after applying colour correction, and FDIFF is the flux of the diffuse emission obtained as FDISK − (FNW + FSE). The lower error of FDIFF includes the contribution of smaller and less intense SF regions in the disk (see Sect. 6).

(*)

The contribution from thermal radio emission was not subtracted.

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