Discovery of a thin lithium plateau among metal-poor red giant branch stars

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Volume 661 (May 2022)

A&A, 661 (2022) A153

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Table 2

Instrument, spectral range and resolution, ID program, and PI for each spectrum used in this work.

ID	Instrument	Spectral range	Resolution	RV	ID program (PI)

		(Å)		(kms⁻¹)
BD+233130	UVES	3281–1562	49620	−283.85 ± 0.01	165.N-0276 (Cayrel)
	UVES	4654–6760	51690	−283.80 ± 0.02	165.N-0276 (Cayrel)
BD-012582	UVES	3027–3884	40970	–	68.D-0546 (Asplund)
	UVES	4729–6835	56990	–	68.D-0546 (Asplund)
BS 16467-062	UVES	3305–4607	40970	–	165.N-0276 (Cayrel)
	UVES	4654–6760	42310	–	165.N-0276 (Cayrel)
BS 16477-003	UVES	3305–4607	40970	–	165.N-0276 (Cayrel)
	UVES	4654–6760	42310	–	165.N-0276 (Cayrel)
CD-241782	UVES	3027–3884	40970	–	68.D-0546 (Asplund)
	UVES	4143–6277	107200	–	69.D-0065 (Asplund)
	UVES	4729–6835	56990	–	68.D-0546 (Asplund)
CD-30298	UVES	3027–3884	40970	–	68.D-0546 (Asplund)
	UVES	4729–6835	56990	–	68.D-0546 (Asplund)
CS 22183-031	UVES	3282–4563	40970	+16.73 ± 0.03	099.D-0287 (Mucciarelli)
	UVES	5655–9464	42310	–	099.D-0287 (Mucciarelli)

Notes. The RV is listed only for the stars for which we analysed spectra not already discussed in previous papers (the quoted errors are computed as the dispersion divided by the root mean square of the measured lines). The entire table is available in electronic form.

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