Table C.1.
Sources not selected as SNRs.
| Xp | RA | Dec | ℛ0 | ℛ1 | EW(FeXXV) |
|---|---|---|---|---|---|
| 0 | 55.1 | 40.5 | −0.08(0.45) | 0.15(0.61) | < 1.2 |
| 1 | 54.7 | 53.7 | −0.06(0.33) | 0.33(0.31) | < 1.9 |
| 3 | 53.8 | 50.3 | 0.08(0.11) | 0.44(0.07) | < 0.20 |
| 4 | 53.3 | 48.5 | −0.20(0.14) | 0.37(0.11) | < 0.12 |
| 6 | 52.5 | 48.9 | 0.05(0.16) | 0.43(0.15) | < 0.45 |
| 7 | 52.3 | 53.7 | 0.03(0.18) | 0.29(0.13) | < 0.8 |
| 9 | 52.0 | 45.3 | −0.29(0.15) | 0.39(0.11) | < 0.20 |
| 11 | 51.8 | 51.7 | −0.01(0.13) | 0.40(0.13) |
 |
| 13 | 51.3 | 43.6 | −0.21(0.02) | 0.35(0.01) | < 0.01 |
| 14 | 51.0 | 45.4 | −0.21(0.03) | 0.36(0.02) | < 0.02 |
| 16 | 50.1 | 46.5 | −0.07(0.01) | 0.42(0.01) | < 0.01 |
| 18 | 49.4 | 43.6 | −0.20(0.14) | 0.24(0.06) | < 0.06 |
| 19 | 48.9 | 39.8 | −0.29(0.40) | 0.19(0.17) | < 0.24 |
| 20 | 48.9 | 43.7 | −0.43(0.22) | 0.21(0.18) | < 0.26 |
Notes. Source positions are offsets in arcseconds from RA = 09h55m00s and Dec = +69° 40′00″ (J2000). ℛ0 and ℛ1 are the Fe XVV-excess indicators defined in Sect. 3.3. EW(Fe XXV) is the equivalent width of a narrow 6.7 keV line in units of keV (or their 89% upper limit). ( ⋆ )This detection is from the background diffuse emission.
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