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XMM-Newton observatory

Astronomy and Astrophysics · 2001 · Vol. 365(1) · pp. L1–L6
F. JansenD. LumbB. AltieriJ. ClavelM. EhleC. ErdC. GabrielM. GuainazziP. GondoinR. MuchR. Weigand MuñozM. SantosN. SchartelD. TexierGiuseppe Vacanti

Abstract

The XMM-Newton Observatory is a cornerstone mission of the European Space Agency's Horizon 2000 programme, and is the largest scientific satellite it has launched to date. This paper summarises the principal characteristics of the Observatory which are pertinent to scientific operations. The scientific results appearing in this issue have been enabled by the unprecedentedly large effective area of the three mirror modules, which are briefly described. The in-orbit performance and preliminary calibrations of the observatory are briefly summarised. The observations from the XMM-Newton calibration and performance verification phase, which are public and from which most papers in this issue have been derived, are listed. The flow of data from the spacecraft, through the ground segment, to the production of preliminary science products supplied to users is also discussed.

Astrophysical Phenomena and ObservationsAdaptive optics and wavefront sensingPulsars and Gravitational Waves ResearchObservatoryPhysicsSpacecraftCalibrationPrincipal (computer security)SatelliteAstronomyRemote sensingAstrophysicsGeography
Citations
2,213
FWCI
75.86
field-weighted impact
References
13
Percentile
100%
vs. same field & year
Citations per year
References
The European Photon Imaging Camera on XMM-Newton: The MOS cameras
Astronomy and Astrophysics · 2001 · 2,280 citations
The Reflection Grating Spectrometer on board XMM-Newton
Astronomy and Astrophysics · 2001 · 988 citations
The European Photon Imaging Camera on XMM-Newton: The pn-CCD camera
Astronomy and Astrophysics · 2001 · 2,845 citations
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