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arXiv · 2212.10995

XMM-Newton

Norbert Schartel·Rosario González-Riestra·Peter Kretschmar·Marcus Kirsch·Pedro Rodríguez-Pascual·Simon Rosen·Maria Santos-Lleó·Michael Smith·Martin Stuhlinger·Eva Verdugo-Rodrigo
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Abstract

The X-ray Multi-mirror Mission (XMM-Newton) provides simultaneous non-dispersive spectroscopic X-ray imaging and timing, medium resolution dispersive X-ray spectroscopy and optical/UV imaging, spectroscopy and timing. In combination, the imaging cameras offer an effective area over the energy range from 150 eV to 12 keV of up to 2500 cm$^2$ at 1.5 keV and $\sim$1800 cm$^2$ at 5 keV. The gratings cover an energy range from 0.4 keV to 2.2 keV with a combined effective area of up to 120 cm$^2$ at 0.8 keV. XMM-Newton offers unique opportunities for a wide variety of sensitive X-ray observations accompanied by simultaneous optical/UV measurements. The majority of XMM-Newton's observing time is made available to the astronomical community by peer-reviewed Announcements of Opportunity. The scientific exploitation of XMM-Newton data is aided by an observatory-class X-ray facility which provides analysis software, pipeline processing, calibration and catalogue generation. Around 380 refereed papers based on XMM-Newton data are published each year with a high fraction of papers reporting transformative scientific results.

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Norbert Schartel, Rosario González-Riestra, Peter Kretschmar, Marcus Kirsch, Pedro Rodríguez-Pascual, Simon Rosen, Maria Santos-Lleó, Michael Smith, Martin Stuhlinger, Eva Verdugo-Rodrigo. 2022-12-21. XMM-Newton. https://doi.org/10.1007/978-981-16-4544-0_41-1

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