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Table 1.

Physical properties of galaxies in our sample, from H11 and Heald et al. (2012).

UGC Other name Type Dist. INCH11 INCBB PABB D25 MB vrot SFR
(Mpc) (°) (°) (°) (′) (mag) (km s−1) (M yr−1)
1256 NGC 0672 SBcd 7.6 70 67.6 64.2 6.4 −18.65 130.7 0.23
1913 NGC 0925 SABd 9.1 54 57.9 284.7 11.3 −19.66 102.4 0.77
1983 NGC 0949 SAd 11.3 52 52.5 160.8 3.5 −17.85 90.9 0.31
2137 NGC 1003 SAcd 11.6 67 70.4 276.3 6.3 −18.61 95.5 0.40
3918 NGC 2403 SAcd 3.2 62 62.5 124.6 23.8 −19.68 121.9 0.6
4284 NGC 2541 SAcd 12.0 67 63.8 171.8 7.2 −18.37 92.1 0.55 (a)
5572 NGC 3198 SBc 14.5 71 70.0 214.3 8.8 −19.62 148.2 1.1
7045 NGC 4062 SAc 16.9 68 67.1 100.1 4.5 −18.27 140.5 0.67
7353 NGC 4258 SABbc 7.6 71 74.0 331.9 17.1 −20.59 208.0 1.7
7377 NGC 4274 SBab 19.4 72 71.3 279.8 6.5 −19.22 239.9 1.2
7539 NGC 4414 SAc 17.8 50 53.9 159.7 4.5 −19.12 224.7 4.2
7591b NGC 4448 SBab 9.7 71 73.5 94.4 3.8 −18.43 221.6 0.056
7766 NGC 4559 SABcd 7.9 69 68.0 323.1 11.3 −20.07 113.4 0.69
8334 NGC 5055 SAbc 8.5 55 65.2 99.4 13.0 −20.14 215.5 2.1
9179 NGC 5585 SABd 8.7 51 50.4 48.2 5.5 −17.96 79.1 0.41

Notes.

(a)

We also list the median kinematical inclination (INCBB) and position angle (PABB) found with 3DBAROLO and used in our EPG modelling. Based on TIR+UV measurements from Thilker et al. (2007) and re-scaled to the distance used in this work. Heald et al. (2012) report only an upper limit based on a non-detection with IRAS 25 μm.

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