Solar-like oscillators properties from Kepler DR25

The catalog was produced by reanalyzing all available Kepler DR25 short-cadence data using pySYD, an automated pipeline to extract global asteroseismic parameters. We find 50 new detections, seven of which are also planet candidate host stars.

We find excellent agreement between our {nu}max and {Delta}{nu} measurements and literature values, with an average offset of 0.2%+/-0.4% ({sigma}=5%) and 0.2%+/-0.7% ({sigma}=2%), respectively. In addition, we derive stellar radii and masses with an average precision of 2.7% and 10.4%, respectively, and find a mean offset of 0.8%+/-0.2% ({sigma}=6%) between our radii derived with asteroseismology and those from Gaia parallaxes.