**Table 5:** Additional data of HR 5999. The $V_{\rm\,obs}^{\rm iue}$ -value marked with () is uncertain, as the brightness is underestimated due to the degradation of the FES counter after 1990 (Sect. B.1). See Table 2 for the other input parameters. The apparently good agreement of the 3 faint spectra (#10-12) at the long wavelength is caused by the fact that we used the same (overexposed) image LWR14027 in these cases.
#	$V_{\rm obs}^{\rm i ue}$	IUE	R^cs	$A_{\rm v}^{\rm cs}$ (mag)			Fig.
	(mag)	images	-	A5 III	A6 III	A7 III	(A6)
1	6.72	09-01	3.10	0.59	0.58	0.48	99
2	6.83 $\dag$	09-02	3.50	0.70	0.69	0.59	100
3	6.81	09-03	3.75	0.68	0.67	0.57	28, 101
4	7.02	09-04	4.50	0.89	0.88	0.78	102
5	7.16	09-05	4.50	1.03	1.02	0.92	103
6	7.17	09-06	4.50	1.04	1.03	0.93	104
7	7.20	09-07	4.50	1.07	1.06	0.96	105
8	7.30	09-08	4.50	1.17	1.16	1.06	106
9	7.39	09-09	5.00	1.26	1.25	1.15	107
10	7.47	09-10	5.25	1.34	1.33	1.23	108
11	7.49	09-11	5.50	1.36	1.35	1.25	109
12	7.57	09-12	5.75	1.44	1.43	1.33	110

Source LaTeX | All tables | In the text