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Table 4.

Optical spectral line fit results.

MJD (a) Instrument He II flux He II FWHM Hβn flux Hβn FWHM Hβb flux Hβb FWHM
(d) (10−16 erg cm−2 s−1) (km s−1) (10−16 erg cm−2 s−1) (km s−1) (10−16 erg cm−2 s−1) (km s−1)
59449 FORS2 (#1) 100.1 ± 22.6 4573 ± 153 23.1 ± 3.5 889 87.6 ± 9.0 2107 ± 222
59468 SAAO (#2) 48.1 ± 34.6 3733 ± 251 21.3 ± 5.3 551 155.7 ± 22.5 2316 ± 48
59616 SALT (#3) < 4.1 2276 ± 396 10.7 ± 4.9 431 97.7 ± 23.4 2054 ± 65
59680 SAAO (#4) 30.5 ± 18.2 689
59828 SAAO (#5) < 1.9 10.4 ± 7.3 727 36.5 ± 30.8 2924 ± 56

Notes.

(a)

Date (Modified Julian Day) of observations. The subscripts n and b indicate the narrow and broad components of the emission lines, respectively. The velocity width of the narrow Hβ line was tied to that for the narrow [O III] λλ5007,4959 lines.

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