Extended Data Table 2 Summary of spectral fit results for eRO-QPE1

From: X-ray quasi-periodic eruptions from two previously quiescent galaxies

  1. The median value and related 16th and 84th percentile values are reported for every quantity; for unconstrained values 1σ upper limits are quoted using the 84th percentile value of the parameter posterior distribution and are denoted with ↓. Reported results are obtained with the model tbabs convoluted with diskbb, with Galactic NH frozen at 2.23 × 1020 cm−2, as reported by the HI4PI Collaboration50. Fluxes and luminosities are unabsorbed and rest-frame. The two eROSITA states are shown in Fig. 1a, and the three XMM-Newton observations in the table correspond to the three spectra in Extended Data Fig. 5a. The disk flux (Fdisk) is computed within 0.001 and 100 keV.