An X-ray and UV flare from the galaxy XMMSL1 J061927.1-655311

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Table 2

Optical line widths and intensities for XMMSL1 J0619-65 from the AAOmega 2dF observation of 2012-12-03.

Line	Rest λ	Intensity relative	FWHM	Flux^a
	Å	to narrow Hα	km s^-1	10^-16 erg s^-1 cm²

Hβ	4862	0.37	300	2.8 ± 1.7
Hβ	4872	8.24	5174	66.8 ± 16.7
[OIII]	5007	1.14	330	8.6 ± 2.2
Hα	6563	1.00	293	8.1 ± 1.0
Hα	6570	33.54	5716	271.9 ± 15.5
Hα	6578	4.61	2687	37.3 ± 9.7
[NII]	6582	0.85	292	6.9 ± 0.9
[SII]	6719	0.42	286	3.4 ± 0.5
[SII]	6730	0.58	285	4.7 ± 0.6

Notes.

^(a)

The quoted errors on the flux represent the statistical error. The estimated systematic error on the absolute line fluxes is ~25%.

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