Model parameters for the cstat analysis. The redshifts for each galaxy are as given in Table 2. |$kT$| is the temperature of the apec model component; Z is the abundance relative to solar abundance. Where |$\mathrm{CFrac}$| was fitted as 1, there is no upper error, so only a lower bounds on the error is given. The errors represent the 90 per cent confidence intervals using |$\chi ^2$|.
| Target . | |$N_\text{H}^{\prime }$| . | |$kT$| . | Z . | |$\mathrm{ Norm}$| . | |$\mathrm{CFrac}$| . | |$N_\text{H}$| . | |$\dot{M}$| . | |$\dot{M}_\text{u}$| . |
|---|---|---|---|---|---|---|---|---|
| . | |$10^{22}$| cm|$-$|2 . | (keV) . | (|$Z_{\odot }$|) . | |$10^{-4}$| . | . | |$10^{22}$| cm|$-$|2 . | (|$\mathrm{ M}_\odot$| yr|$-$|1) . | (|$\mathrm{ M}_\odot$| yr|$-$|1) . |
| NGC 1316 | 0.0199 | |$1.00^{+0.05}_{-0.12}$| | |$0.21^{+0.03}_{-0.04}$| | 7.8e−3 | |$0.90^{+0.06}_{-0.01}$| | 3.8 | |$4.4^{+3.1}_{-2.2}$| | |$0.52 \pm 0.04$| |
| NGC 1332 | 0.0214 | |$0.67^{+0.04}_{-0.05}$| | |$0.11^{+0.03}_{-0.02}$| | 2.4 | |$1_{-0.04}$| | 4.7 | |$7.9^{+2.8}_{-0.4}$| | |$0.27^{+0.06}_{-0.05}$| |
| NGC 1404 | 0.0138 | |$0.69 \pm 0.01$| | |$0.21\pm 0.01$| | 20 | |$0.97^{+0.02}_{-0.03}$| | 2.2 | |$8.0\pm 0.3$| | |$0.62\pm 0.14$| |
| NGC 4552 | 0.0266 | |$0.70\pm 0.02$| | |$0.072^{+0.007}_{-0.006}$| | 7.3 | |$0.97^{+0.03}_{-0.15}$| | 4.6 | |$0.72^{+0.6}_{-0.1}$| | |$0.036^{+0.004}_{-0.006}$| |
| NGC 4636 | 0.0182 | |$0.76\pm 0.02$| | |$0.26\pm 0.02$| | 33 | |$1_{-0.24}$| | 0.33 | |$0.91^{0.23}_{-0.22}$| | |$0.32^{+0.06}_{-0.05}$| |
| NGC 4649 | 0.0202 | |$0.91\pm 0.01$| | |$0.32\pm 0.02$| | 23 | |$1_{-0.01}$| | 9.9 | |$4.0^{+1.5}_{-1.9}$| | negligible |
| IC 1459 | 0.009 67 | |$0.73^{+0.16}_{0.07}$| | |$0.09^{+0.03}_{-0.02}$| | 1.6 | |$0.91^{+0.06}_{-0.39}$| | 6.2 | |$3.2^{+2.9}_{-2.5}$| | |$0.33^{+0.05}_{-0.06}$| |
| Target . | |$N_\text{H}^{\prime }$| . | |$kT$| . | Z . | |$\mathrm{ Norm}$| . | |$\mathrm{CFrac}$| . | |$N_\text{H}$| . | |$\dot{M}$| . | |$\dot{M}_\text{u}$| . |
|---|---|---|---|---|---|---|---|---|
| . | |$10^{22}$| cm|$-$|2 . | (keV) . | (|$Z_{\odot }$|) . | |$10^{-4}$| . | . | |$10^{22}$| cm|$-$|2 . | (|$\mathrm{ M}_\odot$| yr|$-$|1) . | (|$\mathrm{ M}_\odot$| yr|$-$|1) . |
| NGC 1316 | 0.0199 | |$1.00^{+0.05}_{-0.12}$| | |$0.21^{+0.03}_{-0.04}$| | 7.8e−3 | |$0.90^{+0.06}_{-0.01}$| | 3.8 | |$4.4^{+3.1}_{-2.2}$| | |$0.52 \pm 0.04$| |
| NGC 1332 | 0.0214 | |$0.67^{+0.04}_{-0.05}$| | |$0.11^{+0.03}_{-0.02}$| | 2.4 | |$1_{-0.04}$| | 4.7 | |$7.9^{+2.8}_{-0.4}$| | |$0.27^{+0.06}_{-0.05}$| |
| NGC 1404 | 0.0138 | |$0.69 \pm 0.01$| | |$0.21\pm 0.01$| | 20 | |$0.97^{+0.02}_{-0.03}$| | 2.2 | |$8.0\pm 0.3$| | |$0.62\pm 0.14$| |
| NGC 4552 | 0.0266 | |$0.70\pm 0.02$| | |$0.072^{+0.007}_{-0.006}$| | 7.3 | |$0.97^{+0.03}_{-0.15}$| | 4.6 | |$0.72^{+0.6}_{-0.1}$| | |$0.036^{+0.004}_{-0.006}$| |
| NGC 4636 | 0.0182 | |$0.76\pm 0.02$| | |$0.26\pm 0.02$| | 33 | |$1_{-0.24}$| | 0.33 | |$0.91^{0.23}_{-0.22}$| | |$0.32^{+0.06}_{-0.05}$| |
| NGC 4649 | 0.0202 | |$0.91\pm 0.01$| | |$0.32\pm 0.02$| | 23 | |$1_{-0.01}$| | 9.9 | |$4.0^{+1.5}_{-1.9}$| | negligible |
| IC 1459 | 0.009 67 | |$0.73^{+0.16}_{0.07}$| | |$0.09^{+0.03}_{-0.02}$| | 1.6 | |$0.91^{+0.06}_{-0.39}$| | 6.2 | |$3.2^{+2.9}_{-2.5}$| | |$0.33^{+0.05}_{-0.06}$| |
Model parameters for the cstat analysis. The redshifts for each galaxy are as given in Table 2. |$kT$| is the temperature of the apec model component; Z is the abundance relative to solar abundance. Where |$\mathrm{CFrac}$| was fitted as 1, there is no upper error, so only a lower bounds on the error is given. The errors represent the 90 per cent confidence intervals using |$\chi ^2$|.
| Target . | |$N_\text{H}^{\prime }$| . | |$kT$| . | Z . | |$\mathrm{ Norm}$| . | |$\mathrm{CFrac}$| . | |$N_\text{H}$| . | |$\dot{M}$| . | |$\dot{M}_\text{u}$| . |
|---|---|---|---|---|---|---|---|---|
| . | |$10^{22}$| cm|$-$|2 . | (keV) . | (|$Z_{\odot }$|) . | |$10^{-4}$| . | . | |$10^{22}$| cm|$-$|2 . | (|$\mathrm{ M}_\odot$| yr|$-$|1) . | (|$\mathrm{ M}_\odot$| yr|$-$|1) . |
| NGC 1316 | 0.0199 | |$1.00^{+0.05}_{-0.12}$| | |$0.21^{+0.03}_{-0.04}$| | 7.8e−3 | |$0.90^{+0.06}_{-0.01}$| | 3.8 | |$4.4^{+3.1}_{-2.2}$| | |$0.52 \pm 0.04$| |
| NGC 1332 | 0.0214 | |$0.67^{+0.04}_{-0.05}$| | |$0.11^{+0.03}_{-0.02}$| | 2.4 | |$1_{-0.04}$| | 4.7 | |$7.9^{+2.8}_{-0.4}$| | |$0.27^{+0.06}_{-0.05}$| |
| NGC 1404 | 0.0138 | |$0.69 \pm 0.01$| | |$0.21\pm 0.01$| | 20 | |$0.97^{+0.02}_{-0.03}$| | 2.2 | |$8.0\pm 0.3$| | |$0.62\pm 0.14$| |
| NGC 4552 | 0.0266 | |$0.70\pm 0.02$| | |$0.072^{+0.007}_{-0.006}$| | 7.3 | |$0.97^{+0.03}_{-0.15}$| | 4.6 | |$0.72^{+0.6}_{-0.1}$| | |$0.036^{+0.004}_{-0.006}$| |
| NGC 4636 | 0.0182 | |$0.76\pm 0.02$| | |$0.26\pm 0.02$| | 33 | |$1_{-0.24}$| | 0.33 | |$0.91^{0.23}_{-0.22}$| | |$0.32^{+0.06}_{-0.05}$| |
| NGC 4649 | 0.0202 | |$0.91\pm 0.01$| | |$0.32\pm 0.02$| | 23 | |$1_{-0.01}$| | 9.9 | |$4.0^{+1.5}_{-1.9}$| | negligible |
| IC 1459 | 0.009 67 | |$0.73^{+0.16}_{0.07}$| | |$0.09^{+0.03}_{-0.02}$| | 1.6 | |$0.91^{+0.06}_{-0.39}$| | 6.2 | |$3.2^{+2.9}_{-2.5}$| | |$0.33^{+0.05}_{-0.06}$| |
| Target . | |$N_\text{H}^{\prime }$| . | |$kT$| . | Z . | |$\mathrm{ Norm}$| . | |$\mathrm{CFrac}$| . | |$N_\text{H}$| . | |$\dot{M}$| . | |$\dot{M}_\text{u}$| . |
|---|---|---|---|---|---|---|---|---|
| . | |$10^{22}$| cm|$-$|2 . | (keV) . | (|$Z_{\odot }$|) . | |$10^{-4}$| . | . | |$10^{22}$| cm|$-$|2 . | (|$\mathrm{ M}_\odot$| yr|$-$|1) . | (|$\mathrm{ M}_\odot$| yr|$-$|1) . |
| NGC 1316 | 0.0199 | |$1.00^{+0.05}_{-0.12}$| | |$0.21^{+0.03}_{-0.04}$| | 7.8e−3 | |$0.90^{+0.06}_{-0.01}$| | 3.8 | |$4.4^{+3.1}_{-2.2}$| | |$0.52 \pm 0.04$| |
| NGC 1332 | 0.0214 | |$0.67^{+0.04}_{-0.05}$| | |$0.11^{+0.03}_{-0.02}$| | 2.4 | |$1_{-0.04}$| | 4.7 | |$7.9^{+2.8}_{-0.4}$| | |$0.27^{+0.06}_{-0.05}$| |
| NGC 1404 | 0.0138 | |$0.69 \pm 0.01$| | |$0.21\pm 0.01$| | 20 | |$0.97^{+0.02}_{-0.03}$| | 2.2 | |$8.0\pm 0.3$| | |$0.62\pm 0.14$| |
| NGC 4552 | 0.0266 | |$0.70\pm 0.02$| | |$0.072^{+0.007}_{-0.006}$| | 7.3 | |$0.97^{+0.03}_{-0.15}$| | 4.6 | |$0.72^{+0.6}_{-0.1}$| | |$0.036^{+0.004}_{-0.006}$| |
| NGC 4636 | 0.0182 | |$0.76\pm 0.02$| | |$0.26\pm 0.02$| | 33 | |$1_{-0.24}$| | 0.33 | |$0.91^{0.23}_{-0.22}$| | |$0.32^{+0.06}_{-0.05}$| |
| NGC 4649 | 0.0202 | |$0.91\pm 0.01$| | |$0.32\pm 0.02$| | 23 | |$1_{-0.01}$| | 9.9 | |$4.0^{+1.5}_{-1.9}$| | negligible |
| IC 1459 | 0.009 67 | |$0.73^{+0.16}_{0.07}$| | |$0.09^{+0.03}_{-0.02}$| | 1.6 | |$0.91^{+0.06}_{-0.39}$| | 6.2 | |$3.2^{+2.9}_{-2.5}$| | |$0.33^{+0.05}_{-0.06}$| |
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