X-ray and radio observations of the eruption as observed by Earth, Solar Orbiter, and PSP. The GOES XRS 1–8 Å and 0.5–4 Å channels are shown in panel a. The STIX light curves in four energy bands (flux summed over these energies) are shown in panel (b), where X-ray emission associated with the eruption can be seen clearly. In panel (c), the dynamic spectra observed by HFR and LFR from PSP/FIELDS are plotted, where the Type-III radio bursts associated with the event is observed. Langmuir waves are also observed at ∼0.05 MHz after around 22:20 UT. The times here are all adjusted to UT at the PSP location.