XMM–Newton, 0.3–10 keV and 0.16–13 keV, and Swift sub-sample IGM column density results. For each blazar, the columns give Blazar name, redshift, fitted IGM |$\mathit {N}\small {\rm HXIGM}$| for Swift, XMM−Newton 0.3–10 keV and 0.16–13 keV, respectively.
| . | . | Swift 0.3–10 keV . | XMM−Newton 0.3–10 keV . | XMM−Newton 0.16–13 keV . |
|---|---|---|---|---|
| Blazar . | z . | log|$\big(\frac{\mathit {N}\small {\rm HXIGM}}{\textrm {cm}^{-2}}\big)$| . | log|$\big(\frac{\mathit {N}\small {\rm HXIGM}}{\textrm {cm}^{-2}}\big)$| . | log|$\big(\frac{\mathit {N}\small {\rm HXIGM}}{\textrm {cm}^{-2}}\big)$| . |
| 3C 454.3 | 0.86 | |$21.67^{+0.41}_{-1.19}$| | |$21.18^{+0.95}_{-0.57}$| | |$21.52^{+0.04}_{-0.12}$| |
| PKS2149−306 | 2.35 | |$21.90^{+0.28}_{-1.12}$| | |$22.18^{+0.05}_{-0.68}$| | |$22.09^{+0.19}_{-0.91}$| |
| PKS2126−158 | 3.26 | |$22.30^{+0.08}_{-1.38}$| | |$22.10^{+0.13}_{-1.40}$| | |$22.11^{+0.11}_{-1.62}$| |
| PKS0537−286 | 3.10 | |$22.21^{+0.07}_{-1.02}$| | |$22.35^{+0.02}_{-0.37}$| | |$22.26^{+0.09}_{-0.39}$| |
| 1ES0836+710 | 2.17 | |$21.85^{+0.36}_{-0.98}$| | |$22.23^{+0.17}_{-1.19}$| | |$21.64^{+0.37}_{-0.87}$| |
| TXS0222+185 | 2.69 | |$22.28^{+0.13}_{-0.96}$| | |$22.44^{+0.04}_{-0.08}$| | |$22.18^{+0.04}_{-0.09}$| |
| PKS0528+134 | 2.06 | |$22.23^{+0.14}_{-0.86}$| | |$22.34^{+0.07}_{-0.12}$| | |$22.31^{+0.08}_{-0.14}$| |
| . | . | Swift 0.3–10 keV . | XMM−Newton 0.3–10 keV . | XMM−Newton 0.16–13 keV . |
|---|---|---|---|---|
| Blazar . | z . | log|$\big(\frac{\mathit {N}\small {\rm HXIGM}}{\textrm {cm}^{-2}}\big)$| . | log|$\big(\frac{\mathit {N}\small {\rm HXIGM}}{\textrm {cm}^{-2}}\big)$| . | log|$\big(\frac{\mathit {N}\small {\rm HXIGM}}{\textrm {cm}^{-2}}\big)$| . |
| 3C 454.3 | 0.86 | |$21.67^{+0.41}_{-1.19}$| | |$21.18^{+0.95}_{-0.57}$| | |$21.52^{+0.04}_{-0.12}$| |
| PKS2149−306 | 2.35 | |$21.90^{+0.28}_{-1.12}$| | |$22.18^{+0.05}_{-0.68}$| | |$22.09^{+0.19}_{-0.91}$| |
| PKS2126−158 | 3.26 | |$22.30^{+0.08}_{-1.38}$| | |$22.10^{+0.13}_{-1.40}$| | |$22.11^{+0.11}_{-1.62}$| |
| PKS0537−286 | 3.10 | |$22.21^{+0.07}_{-1.02}$| | |$22.35^{+0.02}_{-0.37}$| | |$22.26^{+0.09}_{-0.39}$| |
| 1ES0836+710 | 2.17 | |$21.85^{+0.36}_{-0.98}$| | |$22.23^{+0.17}_{-1.19}$| | |$21.64^{+0.37}_{-0.87}$| |
| TXS0222+185 | 2.69 | |$22.28^{+0.13}_{-0.96}$| | |$22.44^{+0.04}_{-0.08}$| | |$22.18^{+0.04}_{-0.09}$| |
| PKS0528+134 | 2.06 | |$22.23^{+0.14}_{-0.86}$| | |$22.34^{+0.07}_{-0.12}$| | |$22.31^{+0.08}_{-0.14}$| |
XMM–Newton, 0.3–10 keV and 0.16–13 keV, and Swift sub-sample IGM column density results. For each blazar, the columns give Blazar name, redshift, fitted IGM |$\mathit {N}\small {\rm HXIGM}$| for Swift, XMM−Newton 0.3–10 keV and 0.16–13 keV, respectively.
| . | . | Swift 0.3–10 keV . | XMM−Newton 0.3–10 keV . | XMM−Newton 0.16–13 keV . |
|---|---|---|---|---|
| Blazar . | z . | log|$\big(\frac{\mathit {N}\small {\rm HXIGM}}{\textrm {cm}^{-2}}\big)$| . | log|$\big(\frac{\mathit {N}\small {\rm HXIGM}}{\textrm {cm}^{-2}}\big)$| . | log|$\big(\frac{\mathit {N}\small {\rm HXIGM}}{\textrm {cm}^{-2}}\big)$| . |
| 3C 454.3 | 0.86 | |$21.67^{+0.41}_{-1.19}$| | |$21.18^{+0.95}_{-0.57}$| | |$21.52^{+0.04}_{-0.12}$| |
| PKS2149−306 | 2.35 | |$21.90^{+0.28}_{-1.12}$| | |$22.18^{+0.05}_{-0.68}$| | |$22.09^{+0.19}_{-0.91}$| |
| PKS2126−158 | 3.26 | |$22.30^{+0.08}_{-1.38}$| | |$22.10^{+0.13}_{-1.40}$| | |$22.11^{+0.11}_{-1.62}$| |
| PKS0537−286 | 3.10 | |$22.21^{+0.07}_{-1.02}$| | |$22.35^{+0.02}_{-0.37}$| | |$22.26^{+0.09}_{-0.39}$| |
| 1ES0836+710 | 2.17 | |$21.85^{+0.36}_{-0.98}$| | |$22.23^{+0.17}_{-1.19}$| | |$21.64^{+0.37}_{-0.87}$| |
| TXS0222+185 | 2.69 | |$22.28^{+0.13}_{-0.96}$| | |$22.44^{+0.04}_{-0.08}$| | |$22.18^{+0.04}_{-0.09}$| |
| PKS0528+134 | 2.06 | |$22.23^{+0.14}_{-0.86}$| | |$22.34^{+0.07}_{-0.12}$| | |$22.31^{+0.08}_{-0.14}$| |
| . | . | Swift 0.3–10 keV . | XMM−Newton 0.3–10 keV . | XMM−Newton 0.16–13 keV . |
|---|---|---|---|---|
| Blazar . | z . | log|$\big(\frac{\mathit {N}\small {\rm HXIGM}}{\textrm {cm}^{-2}}\big)$| . | log|$\big(\frac{\mathit {N}\small {\rm HXIGM}}{\textrm {cm}^{-2}}\big)$| . | log|$\big(\frac{\mathit {N}\small {\rm HXIGM}}{\textrm {cm}^{-2}}\big)$| . |
| 3C 454.3 | 0.86 | |$21.67^{+0.41}_{-1.19}$| | |$21.18^{+0.95}_{-0.57}$| | |$21.52^{+0.04}_{-0.12}$| |
| PKS2149−306 | 2.35 | |$21.90^{+0.28}_{-1.12}$| | |$22.18^{+0.05}_{-0.68}$| | |$22.09^{+0.19}_{-0.91}$| |
| PKS2126−158 | 3.26 | |$22.30^{+0.08}_{-1.38}$| | |$22.10^{+0.13}_{-1.40}$| | |$22.11^{+0.11}_{-1.62}$| |
| PKS0537−286 | 3.10 | |$22.21^{+0.07}_{-1.02}$| | |$22.35^{+0.02}_{-0.37}$| | |$22.26^{+0.09}_{-0.39}$| |
| 1ES0836+710 | 2.17 | |$21.85^{+0.36}_{-0.98}$| | |$22.23^{+0.17}_{-1.19}$| | |$21.64^{+0.37}_{-0.87}$| |
| TXS0222+185 | 2.69 | |$22.28^{+0.13}_{-0.96}$| | |$22.44^{+0.04}_{-0.08}$| | |$22.18^{+0.04}_{-0.09}$| |
| PKS0528+134 | 2.06 | |$22.23^{+0.14}_{-0.86}$| | |$22.34^{+0.07}_{-0.12}$| | |$22.31^{+0.08}_{-0.14}$| |
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