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Table 1.

Median values of the concentration indices for the cold and hot molecular gas and hot-to-cold ratios.

log10LX bin [CO] Number of galaxies Median CCI

erg s−1 log units
bin-1: [42.85–43.50] 9 0.10 ± 0.04
bin-2: [42.65–42.85] 8 –0.05 ± 0.07
bin-3: [42.20–42.65] 8 0.13 ± 0.27
bin-4: [41.73–42.20] 8 0.56 ± 0.13
bin-5: [40.40–41.73] 8 0.58 ± 0.23
bin-6: [39.00–40.40] 8 0.45 ± 0.20
bin-7: [37.80–39.00] 8 0.36 ± 0.11
nonAGN bin 19 0.27 ± 0.13

log10LX bin [NIR] Number of galaxies Median HCI

erg s−1 log units

bin-1: [42.84–43.50] 8 0.16 ± 0.18
bin-2: [42.37–42.82] 6 0.24 ± 0.05
bin-3: [41.73–42.24] 6 0.62 ± 0.25
bin-4: [39.68–41.42] 6 0.56 ± 0.17
bin-5: [37.78–39.60] 6 0.46 ± 0.07
nonAGN bin 3

log10LX bin [hot/cold] Number of galaxies Hot/cold ratio concentration

erg s−1 log units
bin-1: [42.98–43.50] 7 0.35 ± 0.14
bin-2: [42.80–42.86] 7 0.21 ± 0.10
bin-3: [42.37–42.67] 7 0.34 ± 0.05
bin-4: [41.73–42.24] 7 0.06 ± 0.16
bin-5: [39.60–41.42] 7 –0.08 ± 0.08
bin-6: [37.78–39.30] 7 –0.09 ± 0.19

Notes. Column (1) identifies the range of LX luminosities (in log units) used to define the different bins that group the CO and NIR data sets of the galaxies of the sample. Column (2) lists the number of independent data sets in each LX bin. Column (3) lists the median values and the median absolute deviations of the concentration indices (CCI and HCI) and the concentration of the hot-to-cold ratio (shown in Fig. 14) for each LX bin.

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