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

Table 7

Comparison of observed fluxes between the different eROSITA telescope modules using all valid patterns with the best-fit spectral model (obtained by varying the best-fit spectrum for EPIC-pn).

Observation	Energy band	Flux (10¹³ erg cm² s¹)
	(keV)	TM1	TM2	TM3	TM4	TM6
eROSITA Comm.	0.5-2.0
	3.0-10.0
eROSITA FL	0.5−2.0	68.9 ± 1.2	66.1 ± 1.0	67.2 ± 1.0	68.0 ± 1.1	66.5 ± 1.0
	3.0−10.0	18.7 ± 0.8	18.0 ± 0.7	18.2 ± 0.7	18.5 ± 0.8	18.1 ± 0.7

Notes. Fluxes derived from PAT = 15 spectra. Errors are quoted at 90% confidence.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.