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Table 5

Equivalent widths (in Å) of the most significant emission lines.

Line ID E W 1 E W 2 E W 3

Ca II K 25.90±3.00 21.25±3.10 23.30±2.50
Ca II H 15.70±3.10 12.40±3.00 13.40±3.00
[SII] 0.24±0.10 0.30±0.10 0.21±0.10
Hβ 1.80±0.30 1.85±0.30 1.53±0.30
He I 0.12±0.06 0.14±0.06 0.10±0.06
[OI] 0.12±0.02 0.11±0.02 0.10±0.02
Hα 2.96±0.20 3.16±0.20 2.42±0.20

Notes. The subscripts indicate the first (2012-01-09), second (2012-02-24), and third (2012-03-07) nights of the UVES observations (Table 1). Error bars represent the 3σ uncertainty.

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