Table 1.
Basic data for the newly observed or processed group-dominant galaxies.
Galaxy | z | DL (Mpc) | Beama (kpc) | log LBb (L⊙) | D25b (kpc) | log Mdustd (L⊙) | log M(HI)c (M⊙) | log LFIRd (L⊙) | log M*e (M⊙) | M(H2)f (108 M⊙) | F1.4 GHzg (mJy) |
IRAM 30 m CLoGS survey observations | |||||||||||
NGC 128 | 0.014146 | 58.54 | 6.22 | 10.66 | 53.73 | 6.48 | 8.65 | 9.84 ± 0.03 | 11.09 | 1.76 ± 0.18h | 1.5 |
NGC 252 | 0.016471 | 71.65 | 7.63 | 10.56 | 33.72 | 6.97 | 9.56 | 9.84 ± 0.05 | 11.06 | 6.29 ± 0.79 | 2.5 |
NGC 410 | 0.017659 | 76.67 | 8.17 | 10.95 | 52.77 | – | – | – | 11.37 | <1.17 | 5.8 |
NGC 584 | 0.006011 | 18.71 | 1.97 | 10.20 | 20.60 | 6.06 | 8.08 | 8.15 ± 0.06 | 10.62 | <0.11 | 0.6 |
NGC 924 | 0.014880 | 63.61 | 6.76 | 10.30 | 37.61 | 7.30 | 9.96 | 9.50 ± 0.23 | 10.76 | 0.52 ± 0.10 | 0.9 |
NGC 978 | 0.015794 | 68.66 | 7.30 | 10.56 | 36.60 | 5.49 | – | 8.96 ± 0.08 | 11.08 | <0.70 | 0.7 |
NGC 1106 | 0.014467 | 63.26 | 6.72 | 10.33 | 33.56 | 6.19 | – | 10.03 ± 0.06 | 10.87 | 6.81 ± 0.33 | 132 |
NGC 1453 | 0.012962 | 53.54 | 5.68 | 10.61 | 38.32 | 7.15 | 9.01 | 9.10 ± 0.06 | 11.16 | <0.78 | 28 |
NGC 1550 | 0.012389 | 52.13 | 5.53 | 10.36 | 26.17 | – | – | – | 10.88 | <0.47 | 17 |
NGC 2563 | 0.014944 | 64.39 | 6.84 | 10.47 | 37.89 | – | <8.73 | – | 11.02 | <0.93 | 0.7 |
NGC 2911 | 0.010617 | 45.84 | 4.85 | 10.43 | 46.13 | 5.13 | 9.31 | 8.83 ± 0.07 | 10.82 | 2.66 ± 0.31 | 56 |
NGC 3325 | 0.018873 | 79.67 | 8.50 | 10.40 | 29.24 | – | 9.18 | 4.10 ± 0.01 | 10.88 | <1.57 | – |
NGC 4008 | 0.012075 | 53.96 | 5.72 | 10.47 | 32.57 | 4.62 | <8.49 | 8.87 ± 0.20 | 10.90 | <0.73 | 11 |
NGC 4169 | 0.012622 | 56.67 | 6.01 | 10.44 | 27.04 | 7.48 | 10.03 | 10.46 ± 0.01 | 10.89 | 1.44 ± 0.34 | 1.1 |
NGC 4261 | 0.007378 | 29.38 | 3.10 | 10.65 | 36.29 | 5.04 | <8.69 | 8.30 ± 0.11 | 11.05 | <0.37 | 19700 |
NGC 4956 | 0.015844 | 70.90 | 7.54 | 10.58 | 32.16 | 5.87 | 9.05 | 9.54 ± 0.09 | 10.91 | <0.75 | – |
NGC 5353 | 0.007755 | 35.43 | 3.74 | 10.49 | 24.44 | 3.91 | 9.72 | 8.74 ± 0.04 | 11.05 | 1.90 ± 0.25 | 40 |
NGC 5444 | 0.013169 | 60.46 | 6.42 | 10.64 | 43.67 | – | <8.79 | – | 11.04 | <0.64 | 660 |
NGC 5490 | 0.016195 | 71.94 | 7.66 | 10.68 | 34.73 | – | – | – | 11.15 | <0.64 | 1300 |
NGC 5629 | 0.015004 | 67.73 | 7.20 | 10.58 | 33.61 | – | – | – | 10.95 | <0.91 | 4.6 |
NGC 6658 | 0.014243 | 63.97 | 6.79 | 10.66 | 27.84 | – | – | – | 10.76 | <0.71 | – |
IRAM 30 m deep observations | |||||||||||
NGC 4636 | 0.003129 | 13.61 | 1.43 | 10.44 | 24.98 | 5.07 | 8.84i | 7.94 ± 0.03 | 10.51 | 0.010 ± 0.003 | 78 |
NGC 5813 | 0.006525 | 29.92 | 3.15 | 10.53 | 36.28 | 4.55 | <7.94 | 8.09 ± 0.06 | 10.89 | <0.11 | 15 |
NGC 5846 | 0.005711 | 23.12 | 2.44 | 10.48 | 28.69 | 3.99 | 8.48i | 8.05 ± 0.06 | 10.83 | 0.14 ± 0.06 | 21 |
NGC 7619 | 0.012549 | 54.30 | 5.76 | 10.82 | 39.68 | 6.98 | 7.41i | 9.17 ± 0.12 | 11.21 | <0.29 | 20 |
APEX CLoGS survey observations | |||||||||||
ESO 507-25 | 0.010788 | 45.21 | 6.00 | 10.45 | 34.67 | 6.50 | 10.50 | 9.46 ± 0.05 | 10.95 | 4.23 ± 0.56 | 24 |
NGC 1779 | 0.011051 | 44.44 | 5.90 | 10.27 | 34.47 | 6.53 | 9.26 | 9.73 ± 0.08 | 10.75 | 4.57 ± 0.60 | 5.4 |
NGC 2292 | 0.006791 | 29.57 | 3.91 | 10.40 | 37.29 | 6.84 | 9.35 | 9.26 ± 0.03 | 10.79 | <0.47 | – |
NGC 3923 | 0.005801 | 21.28 | 2.81 | 10.54 | 42.63 | 3.63 | <8.41 | 7.38 ± 0.08 | 11.03 | <0.29 | 1.0 |
NGC 5061 | 0.006945 | 28.26 | 3.73 | 10.61 | 30.82 | 2.65 | <8.66 | 7.40 ± 0.10 | 10.96 | <0.43 | <1.0 |
NGC 5153 | 0.014413 | 60.54 | 8.06 | 10.59 | 43.03 | – | – | – | 10.89 | <1.75 | – |
NGC 5903 | 0.008556 | 31.48 | 4.17 | 10.30 | 27.46 | – | 9.48 | – | 10.73 | <0.58 | 320 |
NGC 7377 | 0.011138 | 46.73 | 6.20 | 10.69 | 53.25 | 6.70 | – | 9.47 ± 0.05 | 11.04 | 4.74 ± 0.44 | 3.1 |
APEX archival observations | |||||||||||
NGC 1395 | 0.005727 | 22.39 | 2.95 | 10.65 | 31.39 | 5.64 | <8.45 | 8.12 ± 0.08 | 10.91 | <0.27 | 1.1 |
NGC 3078 | 0.008606 | 32.66 | 4.32 | 10.39 | 28.89 | – | <8.78 | – | 10.84 | <0.23 | 310 |
NGC 5084 | 0.005741 | 24.09 | 3.18 | 10.31 | 69.59 | 5.74 | 10.18 | 8.87 ± 0.05 | 10.91 | <0.16 | 46 |
Computed from HYPERLEDA (http://leda.univ-lyon1.fr/).
H I masses are drawn from NED (http://nedwww.ipac.caltech.edu/), the extragalactic distance database all-digital H I catalog (Courtois et al. 2009), Serra & Oosterloo (2010), Serra et al. (2012, 2008), Appleton et al. (1990), Huchtmeier (1994), Barnes (1999), Chung et al. (2012), Haynes et al. (2018).
The derivation of LFIR and dust masses Mdust is described in Sect. 5.2.
Molecular gas masses and upper limits either derived from our data or drawn from previous observations (see Sect. 3). Where CO(1-0) and CO(2-1) estimates are available, the larger mass or upper limit is reported here.
1.4 GHz continuum fluxes are drawn from the NRAO VLA Sky Survey (NVSS, Condon et al. 1998, 2002), the Faint Images of the Radio Sky at Twenty Centimeters survey (FIRST, Becker et al. 1995), or from Brown et al. (2011) except in the cases of NGC 924, NGC 978 and NGC 2563, where we extrapolate from the 610 MHz flux (Kolokythas et al. 2018) assuming a spectral index α = 0.8, and NGC 5903 where use the measured flux from O’Sullivan et al. (2018).
Mass estimated from offset pointing, see NGC 128-HI in Table 2.
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