Delving into the depths of NGC 3783 with XRISM - II. Cross-calibration of X-ray instruments used in the large, multi-mission observational campaign

Open Access

Fig. 4

Simple analytical approximation (red) used to reduce excess Resolve flux compared to Xtend and other CCD instruments at the low-energy end of the Resolve band. This expression was derived by approximating the transmission of 10²⁴ atoms m² (black).

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