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Table 3.

Parameters of the point and extended sources fitted to the continuum emission of the MSR and HSR datasets.

Name α2000(a) δ2000(a) Ipoint(b) IGauss(c) IGauss/Ipoint(d) FWHMx(e) FWHMy(e) PAGauss(e) iGauss(e)
hms ° ′ ″ mJy mJy ″ ″ ° °
(MSR, HSR) (MSR, HSR) (MSR, HSR) (MSR, HSR) (MSR, HSR) (MSR, HSR) (MSR, HSR)
NGC 6300 17:16:59.543 −62:49:14.04 (0.37 ± 0.04, 0.22 ± 0.05) (10.52 ± 0.17, 11.95 ± 0.26) (30, 55)±7 (0.65, 0.64) ± 0.02 (0.47, 0.46) ± 0.02 (85, 85) ± 2 (> 44, > 44)
NGC 5643 14:32:40.699 −44:10:27.93 (0.69 ± 0.03, 0.67 ± 0.04) (3.95 ± 0.08, 4.27 ± 0.12) (6, 10)±1 (0.32, 0.32) ± 0.02 (0.25, 0.23) ± 0.02 (4, 5) ± 2 (> 39, > 44)
NGC 7314 22:35:46.201 −26:03:01.58 (0.29 ± 0.03, 0.29 ± 0.03) (1.43 ± 0.06, 1.53 ± 0.09) (5, 5)±1 (0.57, 0.59) ± 0.01 (0.29, 0.31) ± 0.01 (21, 30) ± 3 (> 59, > 58)
NGC 4388 12:25:46.781 +12:39:43.75 (1.86 ± 0.04, 1.79 ± 0.05) (1.75 ± 0.07, 1.92 ± 0.11) (1, 1)±0.1 (0.27, 0.26) ± 0.01 (0.25, 0.23) ± 0.01 (−43, −7) ± 5 (> 22, > 28)
NGC 4941 13:04:13.103 −05:33:05.73 (0.19 ± 0.03, 0.16 ± 0.03) (1.13 ± 0.10, 1.34 ± 0.16) (6, 9)±1 (0.77, 0.73) ± 0.02 (0.29, 0.28) ± 0.02 (−27, −29) ± 5 (> 68, > 67)
NGC 7213 22:09:16.209 −47:10:00.12 (36.5 ± 0.05, 36.10 ± 0.06) (39.59 ± 0.10, 19.10 ± 0.10) (1, 0.5)±0.1 (0.15, 0.14) ± 0.01 (0.13, 0.09) ± 0.01 (71, 44) ± 8 (> 30, > 50)
NGC 7582 23:18:23.643 −42:22:13.54 (0.55 ± 0.04, 0.52 ± 0.05) (3.32 ± 0.16, 3.55 ± 0.21) (6, 7)±1 (0.83, 0.74) ± 0.02 (0.43, 0.40) ± 0.01 (−18, −20) ± 2 (> 59, > 57)
NGC 6814 19:42:40.587 −10:19:25.10 (0.42 ± 0.02, 0.43 ± 0.03) (0.63 ± 0.06, 0.49 ± 0.07) (1.5, 1)±0.1 (0.31, 0.35) ± 0.02 (0.21, 0.12) ± 0.02 (90, 61) ± 10 (> 47, > 70)
NGC 5506 14:13:14.878 −03:12:27.66 (5.07 ± 0.03, 4.73 ± 0.04) (4.06 ± 0.09, 3.96 ± 0.11) (1, 1)±0.1 (0.67, 0.52) ± 0.01 (0.38, 0.31) ± 0.01 (87, 88) ± 2 (> 55, > 53)
NGC 7465 23:02:00.961 +15:57:53.21 (0.08 ± 0.02, < 0.09) (1.19 ± 0.09, 1.13 ± 0.13) (14, 22)±4 (0.50, 0.42) ± 0.02 (0.30, 0.24) ± 0.01 (4, 4) ± 4 (> 53, > 55)
NGC 1365 03:33:36.369 −36:08:25.50 0.15 ± 0.04 2.76 ± 0.11 19 ± 5 0.21 ± 0.03 0.14 ± 0.03 50 ± 10 > 48
NGC 3227 10:23:30.577 +19:51:54.28 0.36 ± 0.03 2.17 ± 0.11 6 ± 1 0.37 ± 0.01 0.24 ± 0.01 166 ± 2 > 50

Notes.

(a)

Positions of the unresolved (point-like) components fitted to the continuum emission derived from the MSR and HSR datasets of the GATOS core sample (listed first); we also include new fits to the data of NGC 1365 (Combes et al. 2019), and NGC 3227 (Alonso-Herrero et al. 2019).

(b)

Intensity of the fitted point sources.

(c)

Spatially-integrated intensity of the elliptical Gaussians that fit the extended emission.

(d)

Flux ratios between the extended components and the points sources.

(e)

Extent (major and minor FWHM: FWHMx, y) and orientation (PAGauss) of the Gaussians. We also list the lower limit to the inclinations of the extended components derived assuming axisymmetry and a negligible thickness-to-radius (H/R) ratio for these features: iGauss = acos(FWHMy/FWHMx).

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