Table 3.
Radio luminosities and spectral index of the VLA sample of AGN dwarf galaxy candidates.
| MaNGA plateifu | Lν, thermal (1026 erg s−1 Hz−1) | LSNR − SNe (1026 erg s−1 Hz−1) | Lpop (1026 erg s−1 Hz−1) | Regions | L6 GHz (1026 erg s−1 Hz−1) | α |
|---|---|---|---|---|---|---|
| 8441-1901 | 23.6 | 1.1 | 9.9 | A | 80.0 ± 3.2 | –0.35 ± 0.03 |
| 8255-12701 | 11.4 | 0.4 | 3.8 | A | 7.0 ± 0.03 | –0.5 ± 0.1 |
| 8465-9101 | 2.9 | 0.1 | 1.0 | A | 3.8 ± 0.5 | –0.5 ± 0.1 |
| B | 2.9 ± 0.2 | –0.6 ± 0.1 | ||||
| C | 3.4 ± 0.2 | –0.5 ± 0.1 | ||||
| D | 4.3 ± 0.3 | –0.5 ± 0.1 | ||||
| 8932-9102 | 23.4 | 0.9 | 8.2 | A | 4.5 ± 0.4 | –0.4 ± 0.1 |
| B | 1.9 ± 0.1 | –0.4 ± 0.1 | ||||
| C | 1.9 ± 0.3 | –0.6 ± 0.1 |
Notes. The expected luminosity radio frequencies of star-forming regions, individual SNR-SNe, and SNRs-SNee populations are Lν, thermal, LSNR − SNe, and Lpop, respectively. The radio luminosity density for each region selected is L6 GHz. The computed spectral index for each source is α.
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