Table 1: Log of the LBV observations. The signal-to-noise ( S/N) was calculated from the noise in flat regions of the continuum. The spectral resolution was calculated using the FWHM of lines in the arc calibration spectra taken at the time and position of the observed star. All observations, including the archive data, were done at the AAT except P Cyg which was done at the WHT. All data was taken using a 1200R grating, except HD 160529 on 18/9/02 which was done using a 600V grating.
Name Coords (2000) $m_{\rm V}$ Obs. date Integration Slit S/N Res.

$\alpha$ $\delta$ time (s) width ( $^{\prime\prime}$ ) (Å)

Galactic

AG Car 10 56 11.58 -60 27 12.8 8.1-6.0 06.05.94 960 1.0 600 1.5

'' '' '' '' 10.02.03 600 1.0 500 1.1

HR Car 10 22 53.84 -59 37 28.4 8.7-7.4 16.03.92 3200 1.0 1300 1.5

'' '' '' '' 10.02.03 680 1.0 600 1.1

$\eta$ Car 10 45 03.59 -59 41 04.3 6.2 13.02.03 12 1.0 300 1.1

Hen 3-519 10 53 59.66 -60 26 44.3 11.0 06.05.94 1600 1.0 500 1.5

'' '' '' '' 10.02.03 8880 1.0 800 1.1

WRA 751 11 08 40.4 -60 42 51 12.3-10.3 11.02.03 8400 1.5 300 1.3

P Cyg 20 17 47.2 +38 01 58.5 4.9 10.12.03 64 1.0 700 0.8

'' '' '' '' 13.12.03 48 1.0 600 0.8

HD 160529 17 41 59.03 -33 30 13.7 6.95-6.4 11.02.03 620 1.0 450 1.1

SMC

R 40 01 07 18.22 -72 28 03.7 10.7-9.9 14.08.03 8400 2.5 350 1.7

''
'' '' '' 15.08.03 4400 2.0 300 1.5

LMC

S Dor 05 18 14.3 -69 14 59 11.4-9.0 11.02.03 4800 1.0 500 1.1

R 71 05 02 07.39 -71 20 13.1 11.0-9.9 12.02.03 7200 1.5 500 1.2

R 110 05 30 51.48 -69 02 58.7 10.6-9.7 12.02.03 7200 1.5 500 1.3

R 116 05 31 52.28 -68 32 38.9 10.6 13.02.03 7200 1.0 600 1.1

R 127 05 36 43.50 -69 29 45.0 11.4-8.8 13.02.03 2880 1.0 400 1.1

R 143 05 38 51.60 -69 08 07.1 12.0-10.6 14.02.03 4800 2.0 350 1.5

**Table 1:** Log of the LBV observations. The signal-to-noise ( *S/N*) was calculated from the noise in flat regions of the continuum. The spectral resolution was calculated using the *FWHM* of lines in the arc calibration spectra taken at the time and position of the observed star. All observations, including the archive data, were done at the AAT except P Cyg which was done at the WHT. All data was taken using a 1200R grating, except HD 160529 on 18/9/02 which was done using a 600V grating.
Name	Coords (2000)	$m_{\rm V}$	Obs. date	Integration	Slit	S/N	Res.
	$\alpha$	$\delta$			time (s)	width ( $^{\prime\prime}$ )		(Å)
Galactic
AG Car	10 56 11.58	-60 27 12.8	8.1-6.0	06.05.94	960	1.0	600	1.5
''	''	''	''	10.02.03	600	1.0	500	1.1
HR Car	10 22 53.84	-59 37 28.4	8.7-7.4	16.03.92	3200	1.0	1300	1.5
''	''	''	''	10.02.03	680	1.0	600	1.1
$\eta$ Car	10 45 03.59	-59 41 04.3	6.2	13.02.03	12	1.0	300	1.1
Hen 3-519	10 53 59.66	-60 26 44.3	11.0	06.05.94	1600	1.0	500	1.5
''	''	''	''	10.02.03	8880	1.0	800	1.1
WRA 751	11 08 40.4	-60 42 51	12.3-10.3	11.02.03	8400	1.5	300	1.3
P Cyg	20 17 47.2	+38 01 58.5	4.9	10.12.03	64	1.0	700	0.8
''	''	''	''	13.12.03	48	1.0	600	0.8
HD 160529	17 41 59.03	-33 30 13.7	6.95-6.4	11.02.03	620	1.0	450	1.1
SMC
R 40	01 07 18.22	-72 28 03.7	10.7-9.9	14.08.03	8400	2.5	350	1.7
''	''	''	''	15.08.03	4400	2.0	300	1.5
LMC
S Dor	05 18 14.3	-69 14 59	11.4-9.0	11.02.03	4800	1.0	500	1.1
R 71	05 02 07.39	-71 20 13.1	11.0-9.9	12.02.03	7200	1.5	500	1.2
R 110	05 30 51.48	-69 02 58.7	10.6-9.7	12.02.03	7200	1.5	500	1.3
R 116	05 31 52.28	-68 32 38.9	10.6	13.02.03	7200	1.0	600	1.1
R 127	05 36 43.50	-69 29 45.0	11.4-8.8	13.02.03	2880	1.0	400	1.1
R 143	05 38 51.60	-69 08 07.1	12.0-10.6	14.02.03	4800	2.0	350	1.5

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observations and data reduction
	3 Results
	4 Discussion
	5 Conclusions
	Appendix A: Atlas of early-type supergiants
	References