Table 3
Blue outliers and blue wings in γ-ray emitters from Foschini et al. (2015), calculated with respect to narrow Hβ.
| Name | v c | FWHM c | v w | FWHM w | |
|
|
|||||
| J0324+3410 | −7.96 ± 79.04 | 445.59 ± 116.76 | −123.73 ± 565.83 | 1201.40 ± 341.90 | |
| J0849+5108 | 264.47 ± 10.78 | 231.26 ± 8.98 | −498.77 ± 74.25 | 703.64 ± 50.30 | |
| J0948+0022 | −770.79 ± 62.87 | 1438.29 ± 55.69 | − | − | |
| J1102+2239 | −565.41 ± 21.56 | 879.90 ± 11.38 | −749.79 ± 164.06 | 1319.85 ± 83.23 | |
| J1246+0238 | 39.94 ± 20.96 | 382.14 ± 20.36 | −503.49 ± 136.52 | 1245.11 ± 70.06 | |
| J1505+0326 | −352.25 ± 59.28 | 597.88 ± 60.48 | −326.51 ± 317.35 | 1180.25 ± 131.13 | |
| J1644+2619 | −9.76 ± 26.35 | 145.24 ± 9.58 | − | − | |
Notes. Columns: (1) name of the source; (2) velocity of the [O III]λ5007 core component (km s-1); (3) FWHM of the core component (km s-1); (4) shift of the blue wing with respect to the core component (km s-1); (5) FWHM of the blue wing (km s-1).
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