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|
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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