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Table A.1.

Spectroscopic identifier, spectral subclass and metallicity of stars with likely enhancement of neutron-rich elements that are located in SEGUE plates listed in Table 2.

Plate ID Cluster ID SpecobjID Subclass [Fe/H] l Spectral lines detected
3304 3719984370237415424 F5 3 Eu Iλ4594; Eu IIλ4129,4205
3719973924876951552 F5 −1.240 3 Eu Iλ4594; Eu IIλ4129,4205
3720148197469954048 F5 −1.668 3 Eu Iλ4594,4627,4661

2667 M 67 3002942521685941248 F2 −1.519 3 Eu Iλ4594,4627; Eu IIλ4205
3002810305412701184 F5 −0.841 3 Eu Iλ4661; Eu IIλ4129,4205
3002885072203389952 F9 −0.449 3 Eu Iλ4594,4627,4661
3002824049308048384 G2 −0.463 3 Eu Iλ4594,4661; Eu IIλ4205
3002777320063867904 F9 −0.774 4 Eu Iλ4627,4661; Eu IIλ4129,4205
3002878750011530240 F9 −0.841 4 Eu Iλ4594,4661; Eu IIλ4129,4205

1961 M 2 2208063770381622272 F9 −0.519 3 Eu Iλ4594; Eu IIλ4129,4205
2208000273585118208 F9 −0.650 3 Eu Iλ4594,4627; Eu IIλ4205
2207981856765352960 F9 −1.721 3 Eu Iλ4627,4661; Eu IIλ4129
2207959591654890496* G2 −1.790 3 Eu Iλ4627,4661; Eu IIλ4205
2208003297242094592 G2 −1.534 4 Eu Iλ4627,4661; Eu IIλ4129,4205
2208044803806043136 F5 −2.530 5 Eu Iλ4594,4627,4661; Eu IIλ4129,4205

2476 NGC 5053 2787852478346009600* F2 −2.230 3 Eu Iλ4627,4661; Eu IIλ4205
2787767541072763904 F5 −1.052 3 Eu Iλ4594,4627,4661
2787760669125090304 F9 −1.078 3 Eu Iλ4594,4627,4661
2787743351816952832 F5 −1.062 3 Eu Iλ4594,4661; Eu IIλ4129
2787843132497173504 G0 −1.817 3 Eu Iλ4661; Eu IIλ4129,4205
2787852203468102656 G2 −2.113 3 Eu Iλ4627,4661; Eu IIλ4129
2787789256427412480 G2 −1.812 3 Eu Iλ4627,4661; Eu IIλ4129
2787840108840197120 F9 −0.823 3 Eu Iλ4594,4627; Eu IIλ4205
2787877492235541504 F9 −0.691 4 Eu Iλ4594,4627,4661; Eu IIλ4205
2787754072055323648 G2 −1.198 4 Eu Iλ4594,4627,4661; Eu IIλ4205

2475 M 3 2786624599054457856* F9 −0.588 3 Eu Iλ4627,4661; Eu IIλ4205
2786709261449796608 F9 3 Eu Iλ4594,4627; Eu II 4205
2786609755647482880 F9 3 Eu Iλ4627; Eu II 4129,4205
2786707062426541056 F9 3 Eu Iλ4594; Eu IIλ4129,4205
2786708436816075776 F9 3 Eu Iλ4594; Eu IIλ4129,4205
2786700190478867456* F5 3 Eu Iλ4627,4661; Eu IIλ4205
2786633944903293952 G2 3 Eu Iλ4594,4661; Eu IIλ4129
2786630646368410624 F9 3 Eu Iλ4594,4661; Eu IIλ4129
2786611954670738432 F9 −1.213 3 Eu Iλ4594,4661; Eu IIλ4129
2786730152170724352 G0 −1.837 3 Eu Iλ4594,4661; Eu IIλ4205
2786726029002120192 F9 −1.229 3 Eu Iλ4594,4627,4661
2786658409037011968 F5 −1.368 3 Eu Iλ4594,4627,4661
2786681773659102208 F9 −1.475 3 Eu Iλ4627,4661; Eu IIλ4129
2786704863403285504 F5 −1.615 4 Eu Iλ4594,4627,4661; Eu IIλ4129
2786753516792814592 F2 −1.698 4 Eu Iλ4594,4627,4661; Eu IIλ4205
2786720531443981312 F2 −1.621 4 Eu Iλ4594,4627,4661; Eu IIλ4129
2786716958031191040 F5 −2.056 4 Eu Iλ4594,4627,4661; Eu IIλ4129
2786636418804456448 F9 5 Eu Iλ4594,4627,4661; Eu IIλ4129,4205

Notes. Secondary candidates (i.e., lacking both the Eu I 4594 Å and the Eu II 4129 Å lines) are identified with an asterisk.

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