SN 1987A: Tracing the flux decline and spectral evolution through a comparison of SRG/eROSITA and XMM-Newton observations

The Early Data Release of eROSITA and Mikhail Pavlinsky ART-XC on the SRG mission

Open Access

Fig. 5

Left: eROSITA spectra (TM3, TM4) from the commissioning observation 700016 with the best-fit model obtained from the combined fit (PAT = 15). Right: same for the first-light observation 700161. The spectra from TM1, 2, 3, 4, and 6 were fit simultaneously.

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