Table 2:

Equivalent widths () and radial velocities (km s^-1) for the H, Pa and He I 7065 emission lines^a,b.

	H					Pa		He I 7065
date	EW	(b)		(r)		EWc		EW
21/09/2003	-22.3 0.2	-75.4	-51.6	-26.0	49.4	-1.10 0.08	-52.7	-0.79 0.03	-48.9
03/04/2004	-25.4 0.2	-71.2	-58.4	-32.8	38.4	-1.13 0.08	-50.2	-0.49 0.05	-35.0
09/06/2004	-25.2 0.2	-73.8	-61.4	-34.0	39.8	-1.15 0.08	-51.7	-0.86 0.03	-45.6
10/07/2004	-24.5 0.2	-74.2	-59.2	-31.3	42.9	-1.03 0.08	-50.2	-0.87 0.03	-43.3
28/09/2004	-23.9 0.2	-72.6	-61.6	-31.1	41.6	-1.05 0.08	-49.3	-0.84 0.03	-44.1
29/05/2005	-21.2 0.3	-	-	-34.3 6	-	-	-	-0.80 0.06	-47.1

^a For the double-peaked H line radial velocities are given for the bluewards and redwards peaks, (b) and (r), the central absorption feature, , and the separation of the two peaks, .
^b Except where noted, errors are conservatively estimated at 4 km s^-1 for the H radial velocities and  km s^-1 for the He I 7065 and Pa radial velocities.
^c The equivalent width of the Pa line includes the absorption components seen in Fig. 2 on either side of the emission line. If these are excluded, then the equivalent width is broadly constant at 1.35  0.15  (with increased errors due to the difficulty of estimating the continuum).