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Table 1.

Properties of the broad emission line components with statistical uncertainties obtained from the full spectral fitting.

Date Instr. vbroad − vnarrow FWHMbroad h3 h4 1017F[O III] 1017FHα, broad LHα, broad MBH
km s−1 km s−1 erg cm−2 s−1 erg cm−2 s−1 1037 erg s−1 103M
2000-07-09 STIS −228 ± 41 2014 ± 80 −0.05 ± 0.03 0.03 ± 0.03 749.3 ± 20.5 65.4 ± 1.8 324.9 ± 26.7

h5 h6

0.05 ± 0.03 −0.09 ± 0.03
2001-01-21 SDSS 32 ± 87 1780 ± 215 0.07 ± 0.06 0.09 ± 0.07 535.0 ± 28.2 476.9 ± 35.6 41.6 ± 3.1 204.6 ± 51.3
2004-02-15 ESI −158 ± 24 2751 ± 77 −0.07 ± 0.01 −0.07 ± 0.01 466.9 ± 2.7 454.9 ± 5.1 39.7 ± 0.4 490.6 ± 28.3
2014-02-10 IDS 234 ± 48 1995 ± 81 0.07 ± 0.03 0.07 ± 0.03 618.1 ± 14.4 53.9 ± 1.3 291.5 ± 24.5

h5 h6

0.00 ± 0.03 −0.11 ± 0.03
2023-03-28 ESI −136 ± 20 2075 ± 59 −0.10 ± 0.02 −0.10 ± 0.02 583.4 ± 6.5 1264.5 ± 19.9 110.3 ± 1.7 439.4 ± 25.7

h5 h6

0.02 ± 0.02 −0.08 ± 0.02
2024-01-15 Binospec 41 ± 3 1762 ± 12 0.00 ± 0.00 0.12 ± 0.00 626.9 ± 1.1 842.0 ± 2.5 73.4 ± 0.2 260.1 ± 3.7
1867 ± 22 756.6 ± 9.6 66.0 ± 0.8 279.0 ± 7.0

Notes. Columns are: 1. Date of the observation; 2. Instrument name; 3. Velocity offset of the broad-line component with respect to the narrow lines; 4. Full width at half-maximum (FWHM) of the broad-line component; 5–6. Gauss-Hermite coefficients h3 and h4 for broad-line component (for the STIS, IDS and ESI (2023) datasets we provide h5 and h6 values in a separate row); 7. Flux in broad Hα component; 8. Luminosity of broad-line component and 9. Virial estimate of the black hole mass from the Hα broad component using relation from Reines et al. (2013). For the Binospec dataset in the last row we also provide a MBH estimate from the spatial-spectral modeling of broad-line component.

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