Table A.2
Plasma diagnostics sub-samples – [O III] flux ratios.
| SDSS name | ID-MJD-FIBER | z | Sample | L[OIII] | R[OIII] | |
| (1) | (2) | (3) | (4) | (5) | (6) | (7) |
|
|
||||||
| J122546.7+123942 | 1615-53166-0388 | 0.0086 | G11 | 40.95 | 127 ± 35 | 95 ± 23 |
| J140040.5-015518 | 0915-52443-0437 | 0.0250 | G11 | 41.07 | 102 ± 9 | 19 ± 2 |
| J144012.7+024743 | 0536-52024-0575 | 0.0299 | G11 | 41.16 | 71 ± 3 | 94 ± 15 |
| J103408.5+600152 | 0560-52296-0520 | 0.0510 | G11 | 42.44 | 284 ± 150 | 79 ± 5 |
| J121839.4+470627 | 1451-53117-0190 | 0.0939 | G11 | 42.16 | 245 ± 140 | 61 ± 4 |
| J093952.7+355358 | 1594-52992-0417 | 0.1366 | G11 | 42.34 | 95 ± 15 | 49 ± 2 |
| ∗J090935.5+105210 | 1739-53050-0421 | 0.1654 | T13 | 42.33 | 50 ± 4 | 44 ± 11 |
| ∗J085331.0+175339 | 2281-53711-0179 | 0.1865 | G11 | 42.56 | 63 ± 2 | 90 ± 11 |
| J122548.8+333248 | 2015-53819-0251 | 0.0011 | G11 | 38.92 | 52 ± 1 | – |
| J134208.3+353915 | 2101-53858-0049 | 0.0036 | G11 | 39.38 | 25 ± 1 | – |
| J112613.7+564809 | 1309-52762-0263 | 0.0101 | T13 | 39.44 | 76 ± 4 | – |
| J081937.9+210651 | 1927-53321-0261 | 0.0185 | G11 | 40.39 | 93 ± 6 | – |
| J005329.9−084604 | 0657-52177-0458 | 0.0190 | G11 | 40.79 | 115 ± 7 | – |
| J104341.2+591653 | 0561-52295-0252 | 0.0285 | T13 | 39.68 | 97 ± 4 | – |
| J235951.7−092632 | 0650-52143-0461 | 0.0423 | T13 | 41.09 | 54 ± 3 | – |
| J080535.0+240950 | 1265-52705-0158 | 0.0597 | G11 | 41.43 | 36 ± 2 | – |
| J134427.5+560128 | 1321-52764-0624 | 0.0706 | T13 | 41.12 | 187 ± 4 | – |
| J122137.9+043026 | 2880-54509-0318 | 0.0947 | G11 | 40.69 | 30 ± 2 | – |
|
|
||||||
| ∗J120429.6+201858 | 2608-54474-0555 | 0.0226 | G11 | 41.17 | 41 ± 3 | 41 ± 3 |
| ∗J130125.2+291849 | 2011-53499-0492 | 0.0234 | T13 | 40.67 | 61 ± 26 | 61 ± 26 |
| J112301.3+470308 | 1441-53083-0560 | 0.0252 | G11 | 40.95 | 44 ± 3 | 44 ± 3 |
| J082443.2+295923 | 1207-52672-0500 | 0.0254 | G11 | 41.19 | 89 ± 5 | 89 ± 5 |
| J080359.2+234520 | 1265-52705-0271 | 0.0294 | G11 | 41.08 | 58 ± 4 | 58 ± 4 |
| J104930.9+225752 | 2481-54068-0247 | 0.0328 | G11 | 41.25 | 59 ± 3 | 59 ± 3 |
| J110929.3+284129 | 2213-53792-0223 | 0.0329 | T13 | 40.87 | 32 ± 2 | 32 ± 3 |
| J095914.7+125916 | 1744-53055-0385 | 0.0343 | G11 | 41.47 | 86 ± 10 | 86 ± 10 |
| J115704.8+524903 | 0882-52370-0430 | 0.0356 | G11 | 41.26 | 84 ± 4 | 84 ± 4 |
| J113549.0+565708 | 1311-52765-0262 | 0.0514 | G11 | 41.69 | 75 ± 4 | 75 ± 4 |
| J151640.2+001501 | 0312-51689-0471 | 0.0526 | G11 | 41.04 | 9 ± 1 | 9 ± 1 |
| J150754.3+010816 | 0540-51996-0253 | 0.0610 | G11 | 41.53 | 51 ± 3 | 51 ± 3 |
| J151106.4+054122 | 1833-54561-0404 | 0.0806 | G11 | 41.61 | 49 ± 2 | 49 ± 2 |
| J102147.8+131228 | 1746-53062-0513 | 0.0852 | G11 | 41.09 | 18 ± 2 | 18 ± 2 |
| J103014.4+431520 | 1429-52990-0131 | 0.0985 | T13 | 41.65 | 48 ± 4 | 48 ± 4 |
| ∗J000703.6+155423 | 0751-52251-0577 | 0.1141 | T13 | 41.94 | 97 ± 45 | 97 ± 45 |
| ∗J111847.0+075419 | 1617-53112-0469 | 0.1269 | G11 | 41.49 | 25 ± 2 | 25 ± 2 |
| J165939.7+183436 | 1567-53172-0113 | 0.1708 | T13 | 42.28 | 69 ± 3 | 69 ± 3 |
| J150719.9+002905 | 0310-51616-0565 | 0.1820 | G11 | 42.63 | 55 ± 8 | 55 ± 8 |
| J075820.9+392335 | 0544-52201-0464 | 0.2162 | G11 | 42.66 | 89 ± 7 | 89 ± 7 |
| ∗J090036.8+205340 | 2282-53683-0103 | 0.2357 | G11 | 42.57 | 55 ± 2 | 55 ± 2 |
| J083454.9+553421 | 5153-56577-0372 | 0.2415 | G11 | 42.34 | 53 ± 5 | 53 ± 5 |
| J131403.5+365438 | 2032-53815-0204 | 0.2967 | T13 | 41.82 | 10 ± 1 | 10 ± 1 |
| J134242.3+494439 | 1669-53433-0215 | 0.3473 | T13 | 42.68 | 36 ± 3 | 36 ± 3 |
| J153641.6+543505 | 0616-52374-0442 | 0.4471 | G11 | 42.48 | 15 ± 4 | 15 ± 4 |
| J080754.5+494627 | 1780-53090-0094 | 0.5753 | W12 | 43.34 | 32 ± 3 | 32 ± 3 |
Notes. Columns (1) to (5): see Table A.2 for description. Columns (6) and (7): NC and OC doubly ionised oxygen flux ratios. Horizontal lines separate the sub-samples defined in Sect. 3.1: the first 8 rows are associated with sources with evidence of ionised outflows and well detected (S/N> 10) [O III]λ4363 lines. For these sources, both NC and OC flux ratios have been measured. The following 10 AGNs are not associated with ionised outflows and only NC flux ratios are reported. Finally, the last 26 rows are associated with AGNs with evidence of outflows but faint (5 <S/N< 10) [O III]λ4363 lines. For these sources, NC and OC flux ratios have been imposed to be equal (i.e. Te(NC) = Te(OC)). The sources marked with (∗) are also present in the sample of 28 AGNs with measured [S II] flux ratios.
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