Solar-like oscillators using TESS 2min cadence LCs

Based on all 2 minute cadence TESS light curves from Sector 1 to 60, we provide a catalog of 8651 solar-like oscillators, including frequency at maximum power ({nu}_max_, with its median precision {sigma}=5.39%), large frequency separation ({Delta}{nu}, {sigma}=6.22%), and seismically derived masses, radii, and surface gravity values. In this sample, we have detected 2173 new oscillators and added 4373 new {Delta}{nu} measurements.

Our seismic parameters are consistent with those from Kepler, K2, and previous TESS data. The median fractional residual in {nu}_max_ is 1.63%, with a scatter of 14.75%, and in {Delta}{nu} it is 0.11%, with a scatter of 10.76%. We have detected 476 solar-like oscillators with {nu}_max_ exceeding the Nyquist frequency of Kepler long-cadence data during the evolutionary phases of subgiants and the base of the red giant branch, which provide a valuable resource for understanding angular momentum transport.