Table 4: Stellar properties for the confirmed field stars observed with DOLORES.
Star Sp. type^a H ${\alpha }$ EW^a $A_{\rm V}~^b$ $N_{\rm H}~^c$ M d Evol. stage

(Å ) (mag) (10²¹ cm^-2) ( $M_{\odot}$ ) (pc)

XEST-05-027 G5 IV/III 2 $7.5\pm 0.3$ $11.0\pm 1.5$ - - giant

XEST-06-041 M2/3 V -1.5 $\rm0.45^{+0.2}_{-0.3}$ $0.50\pm 0.05$ $120\pm 20$ MS

XEST-12-012 M2 V -5 $2.2\pm 0.3$ $0.50\pm 0.05$ $\rm 155^{+30}_{-15}$ MS

XEST-15-075 M4 V -7 $0.3\pm 0.3$ $0.50\pm 0.05$ $115\pm 15$ MS

XEST-18-059^d G0/1 2.8 $\rm 3.1^{+0.4}_{-0.7}$ $1.15\pm 0.15$ $\rm 330^{+130}_{-60}$ MS (or giant?)

XEST-19-002 K4 V 0 $3.3\pm 0.7$ $0.8\pm 0.1$ $\rm 400^{+170}_{-100}$ MS

XEST-22-111 M1/2 V -3.5 $1.7\pm 0.4$ $0.55\pm 0.05$ $175\pm 30$ MS

XEST-27-084 M2 V -4.5 $1.2\pm 0.3$ $0.7\pm 0.4$ $0.55\pm 0.05$ $150\pm 25$ MS

^a From low-resolution spectra (Sect. 4.2); ^b from IR color-color diagram (Sect. 5.2);
^c from X-ray spectral fitting (Scelsi et al. 2007); ^d assuming main sequence star.

**Table 4:** Stellar properties for the confirmed field stars observed with DOLORES.
Star	Sp. type^a	H ${\alpha }$ EW^a	$A_{\rm V}~^b$	$N_{\rm H}~^c$	M	d	Evol. stage
		(Å )	(mag)	(10²¹ cm^-2)	( $M_{\odot}$ )	(pc)
XEST-05-027	G5 IV/III	2	$7.5\pm 0.3$	$11.0\pm 1.5$	-	-	giant
XEST-06-041	M2/3 V	-1.5	$\rm0.45^{+0.2}_{-0.3}$		$0.50\pm 0.05$	$120\pm 20$	MS
XEST-12-012	M2 V	-5	$2.2\pm 0.3$		$0.50\pm 0.05$	$\rm 155^{+30}_{-15}$	MS
XEST-15-075	M4 V	-7	$0.3\pm 0.3$		$0.50\pm 0.05$	$115\pm 15$	MS
XEST-18-059^d	G0/1	2.8	$\rm 3.1^{+0.4}_{-0.7}$		$1.15\pm 0.15$	$\rm 330^{+130}_{-60}$	MS (or giant?)
XEST-19-002	K4 V	0	$3.3\pm 0.7$		$0.8\pm 0.1$	$\rm 400^{+170}_{-100}$	MS
XEST-22-111	M1/2 V	-3.5	$1.7\pm 0.4$		$0.55\pm 0.05$	$175\pm 30$	MS
XEST-27-084	M2 V	-4.5	$1.2\pm 0.3$	$0.7\pm 0.4$	$0.55\pm 0.05$	$150\pm 25$	MS

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