Table 4.
Open in new tab

Model parameters for the 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. |$N_\text{H}$| is the column density of intrinsic absorption, while |$H_\text{H}^{\prime }$| is the column density associated with absorption in our Galaxy. Where |$\mathrm{CFrac}$| was fitted as 1, there is no upper error, so only lower bounds on error are given. The errors represent 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|$-$|2keV|$Z_{\odot }$||$10^{-4}$||$10^{22}$| cm|$-$|2|$\mathrm{ M}_\odot$| yr|$-$|1|$\mathrm{ M}_\odot$| yr|$-$|1
NGC 13160.0199|$0.98_{-0.10}^{+0.07}$||$0.22\pm 0.04$|0.47|$0.91_{-0.13}^{+0.04}$|3.6|$4.2_{-2.5}^{+3.1}$||$0.49^{+0.01}_{-0.04}$|
NGC 13320.0214|$0.68_{-0.05}^{+0.04}$||$0.11_{-0.03}^{+0.04}$|2.43|$1_{-0.03}$|4.0|$5.8^{+3.6}_{-3.4}$||$0.23\pm 0.05$|
NGC 14040.0138|$0.69\pm 0.02$||$0.21\pm 0.01$|19|$0.97\pm 0.03$|2.3|$7.7^{+0.9}_{-1.0}$||$0.55^{+0.11}_{-0.12}$|
NGC 45520.0266|$0.70_{-0.10}^{+0.03}$||$0.07^{+0.02}_{-0.01}$|6.6|$0.97^{+0.16}_{-0.03}$|4.4|$0.65\pm 0.12$||$0.034^{+0.004}_{-0.005}$|
NGC 46360.0182|$0.75\pm 0.01$||$0.27\pm 0.02$|31|$1_{-0.18}$|0.4|$0.89_{-0.11}^{+0.25}$||$0.28\pm 0.05$|
NGC 46490.0202|$0.90\pm 0.01$||$0.33\pm 0.02$|22|$1_{-0.01}$|10.06|$3.4_{-2.4}^{+1.3}$|negligible
IC 14590.009 67|$0.73_{-0.08}^{+0.16}$||$0.11_{-0.02}^{+0.04}$|1.3|$0.91_{-0.51}^{+0.09}$|6.5|$2.7_{-2.3}^{+3.3}$||$0.30_{-0.05}^{+0.06}$|
Target|$N_\text{H}^{\prime }$||$kT$|Z|$\mathrm{ Norm}$||$\mathrm{CFrac}$||$N_\text{H}$||$\dot{M}$||$\dot{M}_\text{u}$|
|$10^{22}$| cm|$-$|2keV|$Z_{\odot }$||$10^{-4}$||$10^{22}$| cm|$-$|2|$\mathrm{ M}_\odot$| yr|$-$|1|$\mathrm{ M}_\odot$| yr|$-$|1
NGC 13160.0199|$0.98_{-0.10}^{+0.07}$||$0.22\pm 0.04$|0.47|$0.91_{-0.13}^{+0.04}$|3.6|$4.2_{-2.5}^{+3.1}$||$0.49^{+0.01}_{-0.04}$|
NGC 13320.0214|$0.68_{-0.05}^{+0.04}$||$0.11_{-0.03}^{+0.04}$|2.43|$1_{-0.03}$|4.0|$5.8^{+3.6}_{-3.4}$||$0.23\pm 0.05$|
NGC 14040.0138|$0.69\pm 0.02$||$0.21\pm 0.01$|19|$0.97\pm 0.03$|2.3|$7.7^{+0.9}_{-1.0}$||$0.55^{+0.11}_{-0.12}$|
NGC 45520.0266|$0.70_{-0.10}^{+0.03}$||$0.07^{+0.02}_{-0.01}$|6.6|$0.97^{+0.16}_{-0.03}$|4.4|$0.65\pm 0.12$||$0.034^{+0.004}_{-0.005}$|
NGC 46360.0182|$0.75\pm 0.01$||$0.27\pm 0.02$|31|$1_{-0.18}$|0.4|$0.89_{-0.11}^{+0.25}$||$0.28\pm 0.05$|
NGC 46490.0202|$0.90\pm 0.01$||$0.33\pm 0.02$|22|$1_{-0.01}$|10.06|$3.4_{-2.4}^{+1.3}$|negligible
IC 14590.009 67|$0.73_{-0.08}^{+0.16}$||$0.11_{-0.02}^{+0.04}$|1.3|$0.91_{-0.51}^{+0.09}$|6.5|$2.7_{-2.3}^{+3.3}$||$0.30_{-0.05}^{+0.06}$|
Table 4.
Open in new tab

Model parameters for the 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. |$N_\text{H}$| is the column density of intrinsic absorption, while |$H_\text{H}^{\prime }$| is the column density associated with absorption in our Galaxy. Where |$\mathrm{CFrac}$| was fitted as 1, there is no upper error, so only lower bounds on error are given. The errors represent 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|$-$|2keV|$Z_{\odot }$||$10^{-4}$||$10^{22}$| cm|$-$|2|$\mathrm{ M}_\odot$| yr|$-$|1|$\mathrm{ M}_\odot$| yr|$-$|1
NGC 13160.0199|$0.98_{-0.10}^{+0.07}$||$0.22\pm 0.04$|0.47|$0.91_{-0.13}^{+0.04}$|3.6|$4.2_{-2.5}^{+3.1}$||$0.49^{+0.01}_{-0.04}$|
NGC 13320.0214|$0.68_{-0.05}^{+0.04}$||$0.11_{-0.03}^{+0.04}$|2.43|$1_{-0.03}$|4.0|$5.8^{+3.6}_{-3.4}$||$0.23\pm 0.05$|
NGC 14040.0138|$0.69\pm 0.02$||$0.21\pm 0.01$|19|$0.97\pm 0.03$|2.3|$7.7^{+0.9}_{-1.0}$||$0.55^{+0.11}_{-0.12}$|
NGC 45520.0266|$0.70_{-0.10}^{+0.03}$||$0.07^{+0.02}_{-0.01}$|6.6|$0.97^{+0.16}_{-0.03}$|4.4|$0.65\pm 0.12$||$0.034^{+0.004}_{-0.005}$|
NGC 46360.0182|$0.75\pm 0.01$||$0.27\pm 0.02$|31|$1_{-0.18}$|0.4|$0.89_{-0.11}^{+0.25}$||$0.28\pm 0.05$|
NGC 46490.0202|$0.90\pm 0.01$||$0.33\pm 0.02$|22|$1_{-0.01}$|10.06|$3.4_{-2.4}^{+1.3}$|negligible
IC 14590.009 67|$0.73_{-0.08}^{+0.16}$||$0.11_{-0.02}^{+0.04}$|1.3|$0.91_{-0.51}^{+0.09}$|6.5|$2.7_{-2.3}^{+3.3}$||$0.30_{-0.05}^{+0.06}$|
Target|$N_\text{H}^{\prime }$||$kT$|Z|$\mathrm{ Norm}$||$\mathrm{CFrac}$||$N_\text{H}$||$\dot{M}$||$\dot{M}_\text{u}$|
|$10^{22}$| cm|$-$|2keV|$Z_{\odot }$||$10^{-4}$||$10^{22}$| cm|$-$|2|$\mathrm{ M}_\odot$| yr|$-$|1|$\mathrm{ M}_\odot$| yr|$-$|1
NGC 13160.0199|$0.98_{-0.10}^{+0.07}$||$0.22\pm 0.04$|0.47|$0.91_{-0.13}^{+0.04}$|3.6|$4.2_{-2.5}^{+3.1}$||$0.49^{+0.01}_{-0.04}$|
NGC 13320.0214|$0.68_{-0.05}^{+0.04}$||$0.11_{-0.03}^{+0.04}$|2.43|$1_{-0.03}$|4.0|$5.8^{+3.6}_{-3.4}$||$0.23\pm 0.05$|
NGC 14040.0138|$0.69\pm 0.02$||$0.21\pm 0.01$|19|$0.97\pm 0.03$|2.3|$7.7^{+0.9}_{-1.0}$||$0.55^{+0.11}_{-0.12}$|
NGC 45520.0266|$0.70_{-0.10}^{+0.03}$||$0.07^{+0.02}_{-0.01}$|6.6|$0.97^{+0.16}_{-0.03}$|4.4|$0.65\pm 0.12$||$0.034^{+0.004}_{-0.005}$|
NGC 46360.0182|$0.75\pm 0.01$||$0.27\pm 0.02$|31|$1_{-0.18}$|0.4|$0.89_{-0.11}^{+0.25}$||$0.28\pm 0.05$|
NGC 46490.0202|$0.90\pm 0.01$||$0.33\pm 0.02$|22|$1_{-0.01}$|10.06|$3.4_{-2.4}^{+1.3}$|negligible
IC 14590.009 67|$0.73_{-0.08}^{+0.16}$||$0.11_{-0.02}^{+0.04}$|1.3|$0.91_{-0.51}^{+0.09}$|6.5|$2.7_{-2.3}^{+3.3}$||$0.30_{-0.05}^{+0.06}$|
Close
This Feature Is Available To Subscribers Only

Sign In or Create an Account

Close

This PDF is available to Subscribers Only

View Article Abstract & Purchase Options

For full access to this pdf, sign in to an existing account, or purchase an annual subscription.

Close