Table 4.
Integrated flux densities of NGC 4217.
| # | Freq. | Flux dens. | log(Freq.) | log(Flux dens.) |
|---|---|---|---|---|
| (GHz) | (Jy) | |||
| I | 0.0575 | 0.30 ± 0.20 | 7.76 | −0.52 ± 0.69 |
| II | 0.150 | 0.47 ± 0.04 | 8.18 | −0.33 ± 0.04 |
| III | 0.151 | 0.44 ± 0.05 | 8.18 | −0.36 ± 0.09 |
| IV | 0.408 | 0.22 ± 0.02 | 8.61 | −0.66 ± 0.07 |
| V | 1.40 | 0.123 ± 0.044 | 9.15 | −0.91 ± 0.32 |
| VI | 1.58 | 0.108 ± 0.005 | 9.20 | −0.96 ± 0.02 |
| VII | 4.85 | 0.040 ± 0.007 | 9.69 | −1.40 ± 0.15 |
| VIII | 5.0 | 0.050 ± 0.011 | 9.70 | −1.30 ± 0.19 |
| IX | 6.00 | 0.033 ± 0.002 | 9.78 | −1.48 ± 0.05 |
Notes. I: Low-frequency radio continuum evidence for cool ionized gas in normal spiral galaxies (Israel & Mahoney 1990). II: LOTSS (this work). III: The 6C survey of radio Sources (6C, Hales et al. 1988). IV: A new Bologna sky survey at 408 MHz (Ficarra et al. 1985). V: The NRAO VLA Sky Survey (NVSS, Condon et al. 1998). VI: CHANG-ES L-band (this work). VII: The 87 GB Catalog of radio sources (Gregory & Condon 1991). VIII: The 5 GHz survey of bright sources (Sramek 1975). IX: CHANG-ES C-band (this work).
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