Table 11
Temperature, absorption and metallicity.
| No. | Galaxy | kT | NH | ZSNII | ZSi |
| keV | 1021 cm-2 | Z⊙ | Z⊙ | ||
|
|
|||||
| Cycle 8 targets | |||||
| 3 | VII Zw 31 |
|
— | 4-2 |
|
| 5 | ESO 255-IG7 N |
|
— |
|
— |
| 9 | 09022-3615 |
|
— |
|
|
| 10 | F09111-1007 E |
|
— |
|
|
| 13 | ESO 374-IG32 |
|
— |
|
|
| 19 | 13120-5453 |
|
— |
|
— |
| 20 | VV 250 |
|
— |
|
|
| 21 | UGC 8387 |
|
— |
|
|
| 25 | VV 340 N |
|
— |
|
|
| 29 | ESO 69-IG6 N |
|
— |
|
|
| 31 | F17132+5313 |
|
— | 0.7-0.4 | — |
| 33 | F18293-3413 |
|
|
|
— |
| 34 | ESO 593-IG8 |
|
— |
|
|
| 35 | F19297-0406 |
|
— | 5-4 | — |
| 37 | CGCG 448-020 |
|
|
|
— |
| 40 | ESO 239-IG2 |
|
— |
|
|
| Archival data | |||||
| 12 | UGC 5101 |
|
— |
|
|
| 15 | F10565+2448 |
|
— |
|
|
| 16 | NGC 3690 |
|
|
|
|
| 18 | UGC 8058 neb |
|
— |
|
|
| 22 | UGC 8696 |
|
— |
|
|
| 22 | UGC 8696 neb |
|
— |
|
|
| 23 | F14348–1447 |
|
— |
|
— |
| 26 | VV 705 N |
|
— |
|
|
| 28 | UGC 9913 |
|
|
|
|
| 30 | NGC 6240 |
|
|
|
|
| 32 | F17207–0014 |
|
|
|
|
| 38 | ESO 286-IG19 |
|
— |
|
|
| 42 | ESO 148-IG2 N |
|
— |
|
|
| 42 | ESO 148-IG2 S |
|
— |
|
|
Notes. The 0.4–2 keV data are fitted with a thermal emission spectrum assuming the metal abundance pattern of core-collapse supernovae (see text for details). When excess absorption above the Galactic value is required, the best-fit column density (NH) is listed. ZSNII is the metallicity for oxygen, which is tied to the other elements with the assumed abundance pattern of Type II SNe. This value is mainly driven by the Fe metallicity, which is assumed to be 0.27 times that of the oxygen metallicity, and which fits the Fe L hump around 1 keV. When excess metallicity for Si (and Mg) is required, the Silicon metallicity is fitted independently (ZSi).
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