Table I.1.
Summary of multi-component decomposition models.
FDS ID | FCC ID | Alias | RA [deg] | Dec [deg] | log10(M*/M⊙) | Multi-comp model | B/T | Bar/T | Re [arcsec] | S4G overlap |
---|---|---|---|---|---|---|---|---|---|---|
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) |
FDS11_0003 | FCC213 | NGC1399 | 54.6209 | −35.4504 | 11.37 | BD | 0.39 | – | 297.01 | Yes |
FDS26_0001 | FCC021 | NGC1316 | 50.6823 | −37.1931 | 11.37 | BD | 0.66 | – | 281.50 | No |
FDS11_0166 | FCC219 | NGC1404 | 54.7164 | −35.5933 | 11.01 | BD | 0.60 | – | 125.12 | No |
FDS17_0365 | FCC121 | NGC1365 | 53.4015 | −36.1408 | 11.00 | NblbarD | – | 0.15 | 167.79 | Yes |
FDS11_0006 | FCC167 | NGC1380 | 54.1150 | −34.9760 | 10.91 | BblbarDD | 0.09 | 0.10 | 210.57 | Yes |
FDS14_0133 | FCC088 | NGC1350 | 52.7835 | −33.6284 | 10.72 | BblbarDD | 0.06 | 0.07 | 132.72 | Yes |
FDS11_0001 | FCC184 | NGC1387 | 54.2376 | −35.5066 | 10.66 | BbarD | 0.31 | 0.06 | 49.82 | Yes |
FDS25_0000 | FCC029 | NGC1326 | 50.9848 | −36.4644 | 10.63 | NblbarD | – | 0.19 | 63.82 | Yes |
FDS26_0254 | FCC022 | NGC1317 | 50.6889 | −37.1051 | 10.48 | BbarbarD | 0.29 | 0.08 | 55.69 | No |
FDS6_0001 | FCC276 | NGC1427 | 55.5810 | −35.3925 | 10.47 | BDD | 0.30 | – | 99.26 | Yes |
FDS11_0002 | FCC161 | NGC1379 | 54.0165 | −35.4412 | 10.39 | BDD | 0.48 | – | 51.44 | Yes |
FDS16_0001 | FCC147 | NGC1374 | 53.8191 | −35.2263 | 10.33 | BDD | 0.24 | – | 60.67 | Yes |
FDS12_0003 | FCC179 | NGC1386 | 54.1925 | −35.9993 | 10.33 | BD | 0.20 | – | 38.09 | Yes |
FDS19_0000 | FCC083 | NGC1351 | 52.6457 | −34.8539 | 10.31 | BDD | 0.61 | – | 99.22 | Yes |
FDS11_0004 | FCC170 | NGC1381 | 54.1318 | −35.2952 | 10.23 | BZZ | 0.40 | – | 47.38 | Yes |
FDS11_0000 | FCC193 | NGC1389 | 54.2989 | −35.7461 | 10.22 | BbarD | 0.74 | 0.09 | 75.14 | Yes |
FDS6_0000 | FCC290 | NGC1436 | 55.9045 | −35.8531 | 10.08 | BbarDD | 0.04 | 0.05 | 54.29 | Yes |
FDS1_0000 | FCC312 | ESO358-063 | 56.5797 | −34.9418 | 10.02 | DD | – | – | 172.84 | Yes |
FDS15_0002 | FCC153 | IC0335 | 53.8794 | −34.4470 | 9.97 | NZZ | – | – | 32.04 | Yes |
FDS13_0000 | FCC249 | NGC1419 | 55.1754 | −37.5108 | 9.91 | BD | 0.73 | – | 144.44 | Yes |
FDS10_0000 | FCC177 | NGC1380A | 54.1978 | −34.7397 | 9.79 | BbarZZ | 0.07 | 0.09 | 43.26 | Yes |
FDS7_0737 | FCC310 | NGC1460 | 56.5571 | −36.6964 | 9.78 | NblbarD | – | 0.19 | 35.28 | Yes |
FDS20_0000 | FCC047 | NGC1336 | 51.6339 | −35.7136 | 9.75 | NBD | 0.51 | – | 43.03 | Yes |
FDS16_0000 | FCC148 | NGC1375 | 53.8200 | −35.2656 | 9.68 | BblD | 0.14 | – | 71.52 | Yes |
FDS12_0002 | FCC176 | NGC1369 | 54.1886 | −36.2562 | 9.68 | NblbarD | – | 0.05 | 30.53 | No |
FDS11_0005 | FCC190 | NGC1380B | 54.2873 | −35.1951 | 9.66 | BblbarD | 0.09 | 0.03 | 37.68 | Yes |
FDS28_0420 | FCC013 | NGC1310 | 50.2646 | −37.0979 | 9.60 | barD | – | 0.02 | 27.02 | Yes |
FDS22_0000 | FCC062 | NGC1341 | 51.9933 | −37.1495 | 9.59 | barD | – | 0.12 | 19.60 | Yes |
FDS6_0002 | FCC277 | NGC1428 | 55.5949 | −35.1541 | 9.57 | BD | 0.80 | – | 37.62 | Yes |
FDS4_0001 | FCC255 | ESO358-050 | 55.2650 | −33.7791 | 9.50 | NbarDD | – | 0.05 | 30.39 | Yes |
FDS7_0736 | FCC308 | NGC1437B | 56.4785 | −36.3569 | 9.47 | D | – | – | 37.12 | Yes |
FDS7_0000 | FCC301 | ESO358-059 | 56.2649 | −35.9727 | 9.45 | barDD | – | 0.17 | 20.41 | Yes |
FDS19_0001 | FCC055 | ESO358-006 | 51.8251 | −34.5265 | 9.42 | ND | – | – | 13.73 | Yes |
FDS16_0002 | FCC143 | NGC1373 | 53.7467 | −35.1711 | 9.36 | BbarD | 0.51 | 0.04 | 17.35 | Yes |
FDS26_0003 | FCC033 | NGC1316C | 51.2432 | −37.0096 | 9.30 | NbarD | – | 0.17 | 17.96 | Yes |
FDS2_0000 | FCC335 | ESO359-002 | 57.6530 | −35.9094 | 9.28 | NDD | – | – | 38.46 | Yes |
Notes. We include identifications (1) of our galaxy sample as outlined in Sect. 2.2, as well as any FCC (2) and alias (3) i.e. designations based on cross-match with HyperLeda (Makarov et al. 2014, http://leda.univ-lyon1.fr/), if one exists. We also include the J2000 right ascension (4) and declination (5) and the parameters from decompositions such as the stellar mass (6), multi-component models (7), bulge-to-total (8), bar-to-total (9), effective radius (10), and whether the galaxies overlap with the S4G (11). The effective radius was calculated from the outermost disk component from the multi-component model. The galaxies are ordered by their stellar masses, in descending order. For brevity only a short extract is shown. The full table can be found at the CDS.
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