Table 1: Star sample.
Name Type RA Dec Distance Period $V_{\rm rad}$ Peak flux

( $\rm ^{h}~^{m}~^{s}$ ) ( $^{\circ}~{'}~{''}$ ) (pc) (days) (km s^-1) (Jy)

S Per Supergiant 02 22 51.72 +58 35 11.4 1610 822 -38.1 76.1

U Her Mira 16 25 47.4713 +18 53 32.867 277 406 -14.5 12.5

NML Cyg Supergiant 20 46 25.7 +40 06 56 1220 940 0.0 48.2

VY CMa Supergiant 07 22 58.3315 -25 46 03.174 1500 2000 22.0 244.1

**Table 1:** Star sample.
Name	Type	RA	Dec	Distance	Period	$V_{\rm rad}$	Peak flux
		( $\rm ^{h}~^{m}~^{s}$ )	( $^{\circ}~{'}~{''}$ )	(pc)	(days)	(km s^-1)	(Jy)
S Per	Supergiant	02 22 51.72	+58 35 11.4	1610	822	-38.1	76.1
U Her	Mira	16 25 47.4713	+18 53 32.867	277	406	-14.5	12.5
NML Cyg	Supergiant	20 46 25.7	+40 06 56	1220	940	0.0	48.2
VY CMa	Supergiant	07 22 58.3315	-25 46 03.174	1500	2000	22.0	244.1

Source LaTeX | All tables | In the text

	1 Introduction
	2 Background
	3 Observations
	4 Results
	5 Discussion
	6 Conclusions
	References