Table 2.
Astrophysical properties of the sample.
NGC | log10M* | log10L144 | LLS | ![]() |
Beq |
---|---|---|---|---|---|
[M⊙] | [W/Hz] | [kpc] | [μG] | ||
4262 | 10.20 | 19.54 ± 0.12 | < 0.68 | ||
4374 | 11.18 | 23.93 ± 0.09 | 13.14 | −0.69 ± 0.10 | 9.20 |
4406 | 11.22 | 20.61 ± 0.09 | < 1.37 | −0.94 ± 0.15 | |
4435 | 10.30 | 20.57 ± 0.10 | < 0.73 | −0.51 ± 0.12 | |
4459 | 10.78 | 20.09 ± 0.10 | < 0.98 | −0.27 ± 0.11 | |
4472 | 11.59 | 23.08 ± 0.09 | 149.4 | −1.21 ± 0.10 | 4.13 |
4486 | 11.36 | 25.61 ± 0.09 | 65.97 | −0.82 ± 0.10 | 7.80 |
4526 | 10.96 | 21.03 ± 0.12 | < 1.47 | −0.47 ± 0.10 | |
4552 | 10.80 | 21.66 ± 0.09 | 15.58 | −0.40 ± 0.10 | 3.27 |
4621 | 10.28 | 19.60 ± 0.10 | < 0.65 | −0.95 ± 0.15 | |
4649 | 11.34 | 21.81 ± 0.09 | 33.21 | −0.82 ± 0.10 | 2.82 |
4660 | 10.05 | 19.79 ± 0.21 | < 0.65 | −0.86 ± 0.14 |
Notes. Column description: (1) NGC; (2) total stellar mass of the host galaxy in stellar units; (3) total 144 MHz luminosity; (4) LLS of the radio emission with upper limits for point and point-like sources; (5) radio spectral index between 144 MHz and 1.28 GHz defined by Fν ∝ να; (6) Equipartition magnetic field strength for the extended sources
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