  The NASA satellite Kepler has gathered about 1420 days-long photometric time
series for more than 20000 red giant stars. For about 6600 of them also APOGEE
spectroscopic parameters are available, making the sample of high interest for
various astrophysical investigations. To optimally exploit the full wealth of
the seismic information, extraction of mode parameters of all significant
individual frequencies is necessary. However, the complex structure of the
mixed mode pattern makes it challenging to automate the peak bagging (i.e., the
extraction of the individual mode parameters from the stars power density
spectra). Even though several approaches have been successfully implemented,
the available results are still limited to a handful of stars. Here I present
frequencies, amplitudes, and lifetimes of more than a quarter of a million
oscillation modes of the spherical degree l=0 to 3, which have been observed in
6179 Kepler red giants. The sample covers evolutionary stages from the lower
red-giant branch to high up the asymptotic giant branch. The modes were
extracted with the Automated Bayesian Peak-Bagging Algorithm (ABBA) and are
publicly available at https://github.com/tkallinger/KeplerRGpeakbagging
