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Table 1.

Sample properties.

Name RA Dec D D25 i SFR 12 + log(O/H) fAGN
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11)
CGCG 381-051 23h48m41.29s +02d14m21.01s 135 1.848 34 10.43 ± 0.08 8.11 ± 0.09 13.26 ± 0.07 8.92 ± 0.14 0.01 ± 0.42
ESO 033-G002 04h55m59.59s −75d32m26.99s 79 1.971 30 10.60 ± 0.08 8.36 ± 0.08 2.86 ± 0.02 9.19 ± 0.21 0.61 ± 0.02
IC 5063 20h52m1.99s −57d4m9.01s 49 2.429 51 10.69 ± 0.09 7.09 ± 0.07 5.28 ± 0.63 8.89 ± 0.13 0.46 ± 0.05
IRAS F01475-0740 01h50m2.69s −07d25m48.0s 77 1.595 43 9.05 ± 0.06 6.62 ± 0.08 3.49 ± 0.42 8.96 ± 0.15 0.25 ± 0.6
IRAS F04385-0828 04h40m54.91s −08d22m22.01s 65 1.838 82 10.27 ± 0.10 8.03 ± 0.08 3.36 ± 0.28 9.26 ± 0.23 0.71 ± 0.03
IRAS F15480-0344 15h50m41.50s −03d53m17.99s 133 1.647 53 10.75 ± 0.09 7.78 ± 0.07 10.16 ± 1.34 8.97 ± 0.15 0.52 ± 0.1
MCG-03-34-064 13h22m24.38s −16d43m43.0s 72 2.129 57 10.65 ± 0.09 7.25 ± 0.08 5.65 ± 0.56 9.60 ± 0.30 0.72 ± 0.07
MCG-03-58-007 22h49m36.91s −19d16m23.99s 138 1.914 44 10.95 ± 0.11 8.82 ± 0.10 20.15 ± 0.88 9.38 ± 0.25 0.48 ± 0.07
MCG+00-29-023 11h21m12.20s −02d59m3.01s 109 1.92 42 10.95 ± 0.11 8.82 ± 0.09 18.71 ± 0.55 9.05 ± 0.17 0.34 ± 0.13
Mrk 0273 13h44m42.11s +55d53m12.65s 167 1.822 67 11.04 ± 0.08 8.03 ± 0.10 66.85 ± 8.02 9.39 ± 0.25 0.39 ± 0.02
Mrk 0463 13h56m2.90s +18d22m18.98s 224 2.035 59 11.22 ± 0.07 7.45 ± 0.11 15.4 ± 2.03 8.81 ± 0.10 0.87 ± 0.02
Mrk 0897 21h7m45.80s +03d52m40.01s 115 1.838 0 10.91 ± 0.10 9.39 ± 0.07 28.23 ± 3.39 9.50 ± 0.27 0.08 ± 0.02
NGC 0034 00h11m06.55s −12d06m26.33s 85 2.062 90 10.58 ± 0.08 7.66 ± 0.08 24.44 ± 1.79 9.53 ± 0.29 0.19 ± 0.1
NGC 0424 01h11m27.49s −38d5m1.0s 51 2.219 78 10.49 ± 0.08 6.65 ± 0.06 1.26 ± 0.05 9.10 ± 0.19 0.8 ± 0.03
NGC 0513 01h24m26.85s +33d47m58.01s 85 1.791 62 10.78 ± 0.09 8.35 ± 0.09 6.64 ± 0.44 9.14 ± 0.21 0.08 ± 0.3
NGC 1125 02h51m40.39s −16d39m1.98s 47 2.178 75 9.52 ± 0.08 6.98 ± 0.08 2.23 ± 0.06 9.15 ± 0.21 0.28 ± 0.13
NGC 1320 03h24m48.71s −03d2m33.0s 38 2.27 81 10.43 ± 0.08 6.56 ± 0.07 0.92 ± 0.01 9.10 ± 0.20 0.56 ± 0.01
NGC 2992 09h45m42.01s −14d19m35.0s 33 2.465 90 9.19 ± 0.07 7.98 ± 0.09 3.61 ± 0.26 9.23 ± 0.22 0.35 ± 0.03
NGC 3079 10h01m57.80s +55d40m47.24s 16 2.913 90 9.76 ± 0.07 7.15 ± 0.10 3.81 ± 0.04 9.81 ± 0.32 0.2 ± 0.1
NGC 4388 12h25m46.75s +12d39m43.51s 36 2.731 90 9.31 ± 0.09 6.97 ± 0.09 3.7 ± 0.11 8.84 ± 0.11 0.4 ± 0.1
NGC 4602 12h40m36.52s −5d7m54.98s 37 2.11 54 9.42 ± 0.10 8.08 ± 0.07 2.99 ± 0.07 8.97 ± 0.16 0.12 ± 0.31
NGC 5135 13h25m44.06s −29d50m01.2s 59 2.379 25 10.71 ± 0.10 7.91 ± 0.10 15.61 ± 1.87 9.60 ± 0.30 0.25 ± 0.04
NGC 5256 13h38m17.50s +48d16m37.0s 122 2.08 (a) 10.42 ± 0.08 8.26 ± 0.07 31.72 ± 1.39 9.16 ± 0.2 0.14 ± 0.17
NGC 5347 13h53m17.83s +33d29m26.98s 34 2.21 45 10.11 ± 0.11 7.52 ± 0.11 0.71 ± 0.01 9.24 ± 0.22 0.53 ± 0.04
NGC 5506 14h13m14.81s −03d12m27.0s 27 2.457 90 10.41 ± 0.10 8.05 ± 0.08 1.96 ± 0.08 9.06 ± 0.18 0.65 ± 0.07
NGC 5953 15h34m32.30s +15d11m42.0s 28 2.168 44 9.99 ± 0.06 7.40 ± 0.09 2.56 ± 0.1 9.06 ± 0.17 0.02 ± 0.6
NGC 5995 15h48m24.91s −13d45m28.01s 110 2.008 42 10.87 ± 0.08 8.98 ± 0.07 19.19 ± 2.3 9.38 ± 0.25 0.34 ± 0.05
NGC 6890 20h18m18.11s −44d48m23.0s 35 2.201 38 9.86 ± 0.08 6.85 ± 0.12 2.05 ± 0.25 9.37 ± 0.26 0.13 ± 0.69
NGC 7130 21h48m19.52s −34d57m04.48s 70 2.194 34 10.49 ± 0.09 7.74 ± 0.05 20.93 ± 0.05 9.17 ± 0.22 0 ± 0
NGC 7496 23h9m47.20s −43d25m40.01s 24 2.525 53 9.46 ± 0.10 7.03 ± 0.06 1.55 ± 0.19 8.89 ± 0.14 0 ± 0
NGC 7674 23h27m56.70s +08d46m45.01s 127 2.049 27 11.11 ± 0.10 8.00 ± 0.07 23.58 ± 2.83 9.30 ± 0.22 0.58 ± 0.6
TOLOLO 1238-364 12h40m52.90s −36d45m22.0s 47 2.095 22 9.66 ± 0.09 7.53 ± 0.11 5.76 ± 0.17 9.14 ± 0.21 0.32 ± 0.6
UGC 05101 09h35m51.60s +61d21m11.45s 174 2.08 0 10.92 ± 0.08 8.25 ± 0.09 55.21 ± 6.63 9.59 ± 0.29 0.65 ± 0.03

Notes. Column descriptions: (1) name; (2) right ascension; (3) declination; (4) distance, in units of Mpc; (5) and (6) logarithm of the 25 mag arcsec−2 isophotal diameter and inclination angle in degrees, respectively, both from the Hyperleda catalog (Makarov et al. 2014); (7) logarithm of the stellar mass from G16; (8) logarithm of the dust mass from G16; (9) SFRs, in units of M yr−1, from G16; (10) oxygen abundances derived through the empirical N2 relation taken from Pérez-Montero & Contini (2009); and (11) the relative contribution of the AGN to the 5–40 μm band luminosity.

(a)

For NGC 5256 we used the D25 measurement from the 3RC catalog (de Vaucouleurs et al. 1991). Since this object is a major merger, the authors did not provide any estimate for the inclination. To provide an aperture correction factor for NGC 5256 consistent with the remaining part of the sample, we estimated the aperture correction assuming ten evenly spaced inclination angles between face-on (i = 0°) and edge-on (i = 90°) configurations. We then adopted a mass correction factor fap = 1.9 ± 0.2, which is the mean of the estimated values and the standard deviation as uncertainty.

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