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Back RGS spectra: dispersion angle vs. CCD pixel energy

RGS spectra: dispersion angle vs. CCD pixel energy


Copyright: ESA/XMM-Newton/RGS

RGS spectra shown as a function of the dispersion angle (x-axis) and the CCD pixel energy (y-axis). The first order spectrum shows up in the brighter, lower bow, the second order is fully separated in the upper bow. The "smudge" on the right is a calibration source.
Last Update: 1 September 2019
21-Jan-2026 19:32 UT

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