This dataset contains observations of the Jovian decametric radio emission induced by Io, measured on 8 June 2021 with the DE604, FR606 and IE613 LOFAR stations, and used in the Louis et al., 2022 (RASTI journal) paper (doi: TBA). The first file (IE613_Jupiter_2021-06-08T040000-070000_84msec_12khz.fil) contains the data at a resolution of ~83.9 msec by ~12.2 kHz, from 04:00:00 UTC to 07:00:00 UTC and in the [7.8 - 55.5] MHz range. The second file (IE613_Jupiter_2021-06-08T051030-051040_fullres_82musec_12khz.fil) contains 10 seconds of the above data (05:10:30 UTC to 05:10:40 UTC) at the highest resolution (81.92μsec by ~12.2 kHz). The third file (FR606_Jupiter_2021-06-08T051030-051040_fullres_82musec_12khz.fil) contains the same 10 seconds than the above file (05:10:30 UTC to 05:10:40 UTC) observed by the Nançay FR606 LOFAR station, at the highest resolution (81.92μsec by ~12.2 kHz) The fourth file (DE604_Jupiter_2021-06-08T051030-051040_fullres_82musec_12khz.fil) contains the same 10 seconds than the two above files (05:10:30 UTC to 05:10:40 UTC) observed by the Postdam DE604 LOFAR station, at the highest resolution (81.92μsec by ~12.2 kHz) These files can be read and processed using the python plot_raw_data.py routine (Louis, 2022, https://doi.org/10.5281/zenodo.6470741)