The chemical DNA of the Magellanic Clouds - V. The r-process dominates neutron-capture elements production in the oldest SMC stars

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Table 1

Key information on the spectroscopic targets.

ID	Gaia DR3 ID	Paper I/ APOGEE ID	RA	Dec	G	K_s	E(B − V)	R21
			(degree)	(degree)	(mag)	(mag)	(mag)
UVES-1	4689859031717528576	FLD-121_100330	6.599776	–71.481933	16.82	14.30	0.028	*
UVES-2	4689864941592504064	FLD-121_100514	6.665003	–71.369523	16.14	13.46	0.028	*
UVES-3	4689861093301638272	FLD-121_100683	6.906465	–71.419883	16.00	13.24	0.028	*
UVES-4	4689844153950876928	FLD-121_100767	6.516431	–71.672640	16.44	13.78	0.028
UVES-5	4689844875502755328	FLD-121_100781	6.326978	–71.668756	15.94	13.12	0.028	*
UVES-6	4690236267283684992	FLD-121_100823	7.173361	–71.394368	16.55	13.70	0.028
UVES-7	4687224842392729984	FLD-419_1355	17.095436	–72.890707	16.54	13.76	0.089
MIKE-1	4703711675634898816	2M00422381-6738579	10.599339	–67.649440	16.27	13.84	0.015
MIKE-2	4703647251125414272	2M00432921-6753477	10.871818	–67.896582	16.19	13.54	0.016
MIKE-3	4690030207641834112	2M00301366-7136292	7.556891	–71.608113	16.03	13.25	0.031
MIKE-4	4687923440279636736	2M01410043-7047414	25.251808	–70.794853	15.84	13.10	0.025
MIKE-5	4638332790102640768	2M02091489-7352354	32.312049	–73.876518	15.78	13.16	0.046

Notes. Columns are: Gaia DR3 identification number, together with the identification number adopted in Paper I for the UVES targets and from APOGEE for the MIKE targets, Gaia coordinates, G and K_s magnitudes, colour excesses. Stars analysed by R21 in common with our sample are marked with *.

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