MaNGA AGN dwarf galaxies (MAD) - IV. Revealing hidden AGN in dwarf galaxies with radio observations

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Table 2.

Results of the Gaussian fitting.

MaNGA plateifu	Clean beam size (arcsec × arcsec)	RMS noise (μJy beam⁻¹)	Region	S/N	Peak flux (μJy beam⁻¹)	Integrated flux (μJy)	Size (arcsec × arcsec)
8442-1901	0.42 × 0.37	3.6	A	81.0 ± 8.0	291.0 ± 12.0	500 ± 29	0.36 × 0.31
8255-12704	0.65 × 0.35	4.0	A	13.1 ± 0.5	52.7 ± 0.2	161.7 ± 0.9	0.86 × 0.52
8465-9101	0.53 × 0.35	4.1	A	7.5 ± 1.0	30.8 ± 4.0	51.3 ± 9.9	0.61 × 0.51
			B	5.8 ± 0.5	23.9 ± 2.0	58.2 ± 6.6	1.0 × 0.46
			C	6.7 ± 0.4	27.8 ± 1.7	81.7 ± 6.7	1.2 × 0.47
			D	8.4 ± 0.6	34.7 ± 2.4	90.1 ± 8.3	0.94 × 0.51
8932-9102	0.52 × 0.36	4.0	A	12.2 ± 1.1	48.6 ± 4.1	168.0 ± 18.0	0.95 × 0.37
			B	5.3 ± 0.4	21.0 ± 1.6	20.1 ± 2.7	0.49 × 0.36
			C	5.3 ± 0.7	53.0 ± 10.0	53.0 ± 10.0	0.90 × 0.17

Notes. Size corresponds to that deconvolved from the beam. Only emission regions with an S/N > 5 were considered. Each region has been marked with a letter and can be identified in Figures 1, A.1, A.2, and A.3.

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