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Table 3.

Photometric parameters extracted with Photutils.

Name RA ΔRA Dec ΔDec PA i iBellocchi+13 i2MASS
(mas) (mas) (deg) (deg) (deg) (deg)
(1) (2) (3) (4) (5) (6) (7) (8) (9)
NGC 2369 07h16m37.68s 59 −62° 20′37.02″ 127 170 ± 1 67 ± 3 75 ± 3 63
NGC 3110 10h04m02.09s 85 −06° 28′29.82″ 86 189 ± 6 50 ± 4 65 ± 3 55
NGC 3256 10h27m51.25s 232 −43° 54′14.53″ 322 170 ± 7 46 ± 10 45 ± 10 47
ESO 320-G030 11h53m11.72s 145 −39° 07′49.07″ 60 118 ± 10 46 ± 5 37 ± 3 (†) 61
IRAS F12115-4656 12h14m12.82s 33 −47° 13′42.79″ 49 119 ± 4 56 ± 5 42 ± 3 (†) 50
NGC 5135 13h25m44.02s 149 −29° 50′01.20″ 172 56 ± 15 31 ± 3 37 ± 3 61
IRAS F17138-1017 17h16m35.82s 121 −10° 20′39.12″ 123 198 ± 5 62 ± 6 52 ± 8 ...
IC 4687 18h13m39.74s 253 −57° 43′30.84″ 165 20 ± 32 27 ± 7 47 ± 3 (†) 50
NGC 7130 21h48m19.51s 103 −34° 57′04.48″ 126 161 ± 13 34 ± 6 51 ± 2 28
IC 5179 22h16m09.16s 278 −36° 50′37.07″ 348 29 ± 6 59 ± 5 56 ± 4 (†) 68

Notes. All the parameters were measured using elliptical Rr apertures whereas their associated uncertainties were computed using Monte Carlo simulations. Columns (2)–(5): coordinates and errors of the photometric centre determination, assuming ALMA astrometry (see Sect. 2.4). Column (6): position angle, defined as the anti-clockwise angle from the north to the semi-major axis. Column (7): inclination, defined as cos i = b/a where b/a is the axial ratio of the elliptical aperture. Column (8): inclination extracted from the same HST/NICMOS images in Bellocchi et al. (2013). (†)Values extracted using Hα maps. Column (9): inclination measured with the 2MASS/Ks image (Skrutskie et al. 2006), obtained from the NASA/IPAC Extragalactic Database (NED).

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