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Table 6.

Properties of the radio emission of the disk and halo of NGC 4217 at three frequencies.

Exponential fits
Integrated flux density
Flux density Flux density disk + halo
(mJy beam−1) (″) (kpc) (mJy) disk + halo (mJy) (mJy)
C-band
Disk 3.2 ± 0.1 2.6 ± 0.2 0.26 ± 0.02 14.2 ± 1.2
Halo 1.0 ± 0.1 11.0 ± 0.4 1.10 ± 0.04 18.8 ± 2.0 33.0 ± 2.3 33 ± 2
Ratio 3.2 ± 0.3 0.24 ± 0.02 (1) 0.75 ± 0.10

L-band
Disk 5.2 ± 0.2 4.6 ± 0.4 0.46 ± 0.04 41.4 ± 3.9
Halo 2.7 ± 0.2 14.3 ± 0.8 1.43 ± 0.09 66.7 ± 6.2 108.1 ± 7.3 108 ± 5
Ratio 1.9 ± 0.2 0.32 ± 0.03 0.62 ± 0.08

LOFAR
Disk 10.3 ± 1.1 4.9 (2) ± 1.4 0.49 ± 0.15 87.3 ± 8.4
Halo 14.7 ± 1.1 15.5 (3) ± 0.36 1.55 ± 0.04 394.2 ± 18.7 481.5 ± 20 470 ± 40
Ratio 0.70 ± 0.09 0.32 ± 0.09 0.22 ± 0.07

Notes. as the mean amplitudes and the mean scale heights of the exponential fits. The column “flux density” lists the integrated flux densities of the disk and halo calculated from the exponential fits. The last column displays the integrated flux densities from Table 4.

(1)

Lower limit if only the synchrotron emission is considered.

(2)

Strip no. 2 not included.

(3)

Strip no. 1 not included.

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