Table 1: The sample with spectral types, variable types, periods (P), luminosities ( $L_{\star }$ ), and distances (D).
Source Spec. Var. P $L_{\star }$ D

Type Type [ days] $[ {L}_\odot]$ [ pc]

LP And C Mira 620 8200 620

CW Leo C Mira 630 8300 120

RW LMi C SRa 640 8500 390

V384 Per C Mira 535 7000 590

AFGL 3068 C Mira 696 9300 1090

TX Cam M Mira 557 11900 440

GX Mon M Mira 527 11100 630

WX Psc M Mira 660 14600 720

IK Tau M Mira 500 10400 300

IRC-10529 M Mira 680 15100 890

**Table 1:** The sample with spectral types, variable types, periods (P), luminosities ( $L_{\star }$ ), and distances (D).
Source	Spec.	Var.		P	$L_{\star }$		D
Type	Type		[ days]	$[ {L}_\odot]$		[ pc]
LP And	C	Mira		620	8200		620
CW Leo	C	Mira		630	8300		120
RW LMi	C	SRa		640	8500		390
V384 Per	C	Mira		535	7000		590
AFGL 3068	C	Mira		696	9300		1090
TX Cam	M	Mira		557	11900		440
GX Mon	M	Mira		527	11100		630
WX Psc	M	Mira		660	14600		720
IK Tau	M	Mira		500	10400		300
IRC-10529	M	Mira		680	15100		890

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