Extended Data Table 1 Seismic parameters of M67 stars

From: Acoustic modes in M67 cluster stars trace deepening convective envelopes

  1. Stars from M67 with measured small frequency separation δν0,2. The uncertainty σΔν is taken from results by the pysyd pipeline. Δν, δν0,2, and \({\sigma }_{\delta {\nu }_{0,2}}\) are calculated as described in Methods. All values are given in μHz.
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