Table 2.
Gaussian emission and absorption parameters in the Fe K band corresponding to a total of 41 observations.
| Emission lines | Absorption lines | |||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Source (1) | XMM (2) | Eem (3) | σwidth (4) | Int (5) | EW (6) | Δ𝒞/Δν (PF) (7) | Eabs (8) | σwidth (9) | Int (10) | EW (11) | vGau (12) | Δ𝒞/Δν (PF) (13) | Pℳ𝒞 (14) | |
| ObsID | (keV) | (eV) | (10−6) | (eV) | (keV) | (eV) | (10−6) | (eV) | (c) | |||||
| PG0052+251 | 0841480101 |
 |
10 (f) |
 |
 |
16.3/2 (> 99.9%) | ||||||||
| PG0953+414 | 0841480201 |
 |
10 (f) |
 |
 |
11.95/2 (99.75%) |
 |
10 (f) |
 |
 |
 |
8.56/2 (98.62%) | 82.1% | |
 |
100t |
 |
 |
24.87/2 (> 99.99%) | ||||||||||
| PG1626+554 | 0841480401 |
 |
100 (f) |
 |
 |
21.02/2 (> 99.99%) | ||||||||
 |
100 (f) |
 |
 |
9.87/2 (99.28%) | ||||||||||
| PG1202+281 | 0841480501 |
 |
10 (f) |
 |
 |
13.7/2 (99.89%) |
 |
10 (f) |
 |
 |
 |
10.3/2 (99.42%) | 95.0% | |
 |
10 (f) |
 |
 |
8.0/2 (98.17%) | ||||||||||
| PG1435−067 | 0841480601 |
 |
10 (f) |
 |
 |
19.0/2 (> 99.99%) |
 |
400 (f) |
 |
 |
 |
9.52/2 (99.14%) | 90.9% | |
| SDSS J144414+0633 | 0841480701 |
 |
10 (f) |
 |
 |
37.48/2 (> 99.99%) | ||||||||
| 2MASS J165315+2349 ( † ) | 0841480801 |
 |
10 (f) |
 |
 |
49.09/2 (> 99.99%) |
 |
10 (f) |
 |
 |
 |
14.39/2 (> 99.9%) | > 99.9%( ‡ ) | |
 |
10 (f) |
 |
 |
 |
14.97/2 (> 99.9%) | |||||||||
 |
100 (f) |
 |
 |
10.48/2 (99.64%) | ||||||||||
| PG1216+069 | 0841480901 |
 |
 |
 |
 |
21.28/3 (> 99.99%) | ||||||||
| PG0947+396 (Obs 1) | 0841481001 |
 |
10 (f) |
 |
 |
23.8/2 (> 99.99%) |
 |
10f |
 |
 |
 |
11.65/2 (99.7%) | 96.9% | |
 |
10 (f) |
 |
 |
9.47/2 (99.12%) | ||||||||||
| PG0947+396 (Obs 2) | 0841482301 |
 |
100 (f) |
 |
 |
35.02/2 (> 99.99%) | ||||||||
| WISE J053756−0245 | 0841481101 |
 |
10 (f) |
 |
 |
21.0/2 (> 99.99%) | ||||||||
| HB 891529+050 | 0841481301 |
 |
10 (f) |
 |
 |
38.88/2 (> 99.99%) | ||||||||
| PG1307+085 | 0841481401 |
 |
100 (f) |
 |
 |
35.74/2 (> 99.99%) | ||||||||
| PG1425+267 | 0841481501 |
 |
10 (f) |
 |
 |
48.12/2 (> 99.99%) |
 |
10f |
 |
 |
 |
10.09/2 (99.36%) | 93.2% | |
 |
10 (f) |
 |
 |
11.91/2 (98.74%) | ||||||||||
| PG1352+183 | 0841481601 |
 |
 |
 |
 |
74.69/3 (> 99.99%) | ||||||||
| 2MASS J105144+3539 | 0841481701 |
 |
100 (f) |
 |
 |
35.66/3 (> 99.99%) |
 |
100f |
 |
 |
 |
10.56/2 (99.49%) | 95.9% | |
| 2MASS J0220−0728 | 0841481901 |
 |
10 (f) |
 |
 |
15.58/2 (> 99.9%) | ||||||||
| LBQS 1338−0038 | 0841482101 |
 |
 |
 |
 |
15.09/2 (> 99.99%) |
 |
378 ( ⋆ ) |
 |
 |
 |
24.14/3 (> 99.9%) | > 99.9% | |
 |
378 (f) |
 |
 |
 |
10.00/2 (99.33%) | 87.2% | ||||||||
| PG0804+761 | 0102040401 |
 |
10 (f) |
 |
 |
7.43/2 (97.56%) |
 |
10f |
 |
 |
 |
15.99/2 (> 99.99%) | 99.8% | |
 |
10 (f) |
 |
 |
7.50/2 (97.65%) | ||||||||||
| 0605110101 |
 |
100 (f) |
 |
 |
25.77/2 (> 99.99%) | |||||||||
 |
10 (f) |
 |
 |
13.89/2 (> 99.99%) | ||||||||||
| 0605110201 |
 |
 |
 |
 |
115.0/3 (> 99.99%) | |||||||||
| PG1416−129 | 0203770201 |
 |
10 (f) |
 |
 |
22.13/2 (> 99.99%) | ||||||||
| PG1402+261 | 0400200101 |
 |
10 (f) |
 |
 |
10.88/2 (99.57%) | ||||||||
 |
10 (f) |
 |
 |
7.42/2 (97.55%) | ||||||||||
| 0830470101 |
 |
100 (f) |
 |
 |
11.69/2 (99.71%) | |||||||||
 |
10 (f) |
 |
 |
7.74/2 (97.91%) | ||||||||||
| HB89 1257+286 | 0204040101 |
 |
100f |
 |
 |
38.3/2 (> 99.99%) |
 |
10 (f) |
 |
 |
 |
6.33/2 (95.78%) | 65.8% | |
| 0204040201 |
 |
10 (f) |
 |
 |
27.2/2 (> 99.99%) | |||||||||
| 0204040301 |
 |
100 (f) |
 |
 |
18.9/2 (> 99.99%) | |||||||||
 |
100 (f) |
 |
 |
14.5/2 (98.74%) | ||||||||||
| 0304320201 |
 |
 |
 |
 |
27.2/3 (> 99.99%) | |||||||||
| 0304320301 |
 |
10 (f) |
 |
 |
9.7/2 (99.23%) | |||||||||
| 0304320801 |
 |
10 (f) |
 |
 |
6.36/2 (95.84%) | |||||||||
| PG 1114+445 | 0109080801 |
 |
 |
 |
 |
103.9/2 (> 99.99%) | ||||||||
| 0651330101 |
 |
 |
 |
 |
54.9/2 (> 99.99%) |
 |
300 (f) |
 |
 |
 |
11.71/2 (99.7%) | 95.5% | ||
| 0651330301 |
 |
50 (f) |
 |
 |
29.2/2 (> 99.99%) |
 |
100 (f) |
 |
 |
 |
11.9/2 (99.7%) | 97.2% | ||
| 0651330401 |
 |
 |
 |
 |
56.9/3 (> 99.99%) |
 |
10 (f) |
 |
 |
 |
8.3/2 (98.4%) | 90.5% | ||
| 0651330501 |
 |
10 (f) |
 |
 |
49.6/2 (> 99.99%) |
 |
10 (f) |
 |
 |
– | 10.02/2 (99.33%) | (N/A)(⬧) | ||
| 0651330601 |
 |
100 (f) |
 |
 |
32.3/2 (> 99.99%) | |||||||||
| 0651330701 |
 |
50 (f) |
 |
 |
29.4/2 (> 99.99%) | |||||||||
| 0651330801 |
 |
100 (f) |
 |
 |
21.6/2 (> 99.99%) | |||||||||
 |
 |
 |
 |
12.9/3 (99.51%) | ||||||||||
| 0651330901 |
 |
50 (f) |
 |
 |
21.5/2 (> 99.99%) | |||||||||
| 0651331001 |
 |
 |
 |
 |
48.8/3 (> 99.99%) | |||||||||
| 0651331101 |
 |
50 (f) |
 |
 |
13.1/2 (99.86%) | |||||||||
Notes. (1) Source name; (2) observation ID; (3) measured Gaussian emission line energy in the rest frame; (4) emission line energy width. The absorption lines were fitted with widths ranging between σwidth 10 eV–400 eV; (5) emission line intensity in units of ph cm−2 s−1; (6) equivalent width; (7) change in 𝒞-stat fit statistic, degrees of freedom and the corresponding significance (in per cent) when the emission line is removed from the best fit; (8)–(11) same as (3)–(6) but for the Gaussian absorption line; (12) corresponding outflow velocity inferred from the rest-frame energy of the absorption line with Erest = 6.97 keV as a reference energy; (13) same as (7); (14) ℳ𝒞 significance of the absorption line where the ≳95% values are highlighted in bold. ( † )In this observation the absorption profile is likely arising from a blend of a Fe XXV–XXVI pair, which could be resolved by binning the spectra with grpmin1 (see Appendix C). ( ‡ )as the two absorption lines are consistent with a Fe XXV–XXVI pair, we inferred the null probability of both profiles simultaneously as a false detection by multiplying the probabilities of each line. ( ⋆ )In this P Cygni-like profile the line width of the emission is tied to that of the absorption as σem = (σabs/Eabs)×Eem. (f)denotes a fixed parameter during fitting. (⬧) A ℳ𝒞 test was not applied for this feature as it is likely associated with a neutral Fe K edge.
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