XMM-Newton observatory. I. The spacecraft and operations

By F. Jansen, D. Lumb, B. Altieri, J. Clavel, M. Ehle, C. Erd, C. Gabriel, M. Guainazzi, P. Gondoin, R. Much and 5 more. 2001

1,802 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics

View Paper: https://www.semanticscholar.org/paper/90bfaa3e64c20e1a6707c9abc1711e8026ee6155

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Citations in the corpus

The Cosmic Evolution of Hard X-Ray-selected Active Galactic Nuclei (2004, background): “Ultimately, many of the sources in these surveys will be pinned down with higher resolution Chandra or XMM-Newton observations and their counterparts robustly identified.”
DEEP EXTRAGALACTIC X-RAY SURVEYS (2005, background): “…active X-ray missions, NASA’s Chandra X-ray Observatory (Chandra; Weisskopf et al. 2000) and ESA’s X-ray Multi-Mirror Mission-Newton (XMM-Newton; Jansen et al. 2001), have executed a number of deep extragalactic X-ray observing programs, which comprise by far the most sensitive X-ray surveys…”
A global look at X-ray time lags in seyfert galaxies (2016, methodology): “For this analysis, we use the data from the XMM-Newton EPIC-pn camera because of its higher effective area and fast readout (Strüder et al. 2001; Jansen et al. 2001).”
Probing cosmic isotropy with a new X-ray galaxy cluster sample through the LX–T scaling relation (2020, background): “Another selection criterion was for the clusters to have good quality Chandra (Weisskopf et al. 2000) or XMM-Newton (Jansen et al. 2001) public observations (as of July 2019).”
The Reflection Grating Spectrometer on-board XMM-Newton: Status of the Calibrations (2002, background): “This telescope, of type Wolter I, has a focal length of 7500 mm and includes 58 nested shells (Jansen et al. 2001).”
A long hard look at MCG–6-30-15 with XMM-Newton (2002, methodology): “Some details of the EPIC spectral calibration are investigated in Appendix A. 2 OBSERVATIONS AND DATA REDUCTION 2.1 XMM-Newtonobservations XMM-Newton(Jansen et al. 2001) has observed MCG–6-30-15 twice.”
The XMM-Newton optical/UV monitor telescope (2000, methodology): “The instrument is fulfilling its role of extending the spectral coverage of XMM-Newton into the ultraviolet and optical band, allowing routine observations of targets simultaneously with EPIC and RGS. Specifically, the instrument has successfully been demonstrated to provide wide field simultaneous ”
The first XMM-Newton slew survey catalogue: XMMSL1 (2008, background): “It was long recognised that XMM-Newton (Jansen et al. 2001) with its great collecting area, efficient CCDs, wide energy band and tight point-spread function (PSF) has the potential to make an important contribution to our knowledge of the local universe from its slew data.”
Spectral changes during dipping in low-mass X-ray binaries due to highly-ionized absorbers (2005, methodology): “The XMM-Newton Observatory (Jansen et al. 2001) includes three 1500 cm2 X-ray telescopes each with an European Photon Imaging Camera (EPIC) at the focus.”
The Chandra Deep Field North Survey. XIV. X-Ray-detected Obscured AGNs and Starburst Galaxies in the Bright Submillimeter Source Population (2002, background): “Due to their high-energy X-ray coverage, high X-ray sensitivity, and excellent positional accura y, theChandra(Weisskopf et al. 2000) andXMM-Newton(Jansen et al. 2001) observatories offer the best opportunities forthe X-ray investigation of SCUBA sources.”
Optimal binning of X-ray spectra and response matrix design (2016, background): “%) and very high resolution has become available through grating spectrometers, first on the Extreme Ultraviolet Explorer (EUVE), and later on the Chandra and XMM-Newton observatories.”
Irradiation of an accretion disc by a jet: general properties and implications for spin measurements of black holes (2013, methodology): “For this purpose we use the EPIC-pn camera (Strüder et al. 2001) of the XMM-Newton satellite (Jansen et al. 2001), a widely used instrument for measuring reflection features and determining the spin of a black hole (see, e.g., Wilms et al. 2001; Fabian et al. 2009; Duro et al. 2011).”
The Suzaku High Resolution X-Ray Spectrometer (2007, background): “…that has been made in developing high resolution x-ray optics with increasing collecting areas (e.g., Aschenbach 1988; Serlemitsos et al. 1995; Jansen et al. 2001; Weisskopf et al. 2002), a key component leading to the enormous progress has been the increase in capabilities for high…”
X-Ray Emissions from Accreting White Dwarfs: A Review (2017, background): “XMM-Newton (1999–present; Jansen et al. 2001) and Chandra (1999–present; Weisskopf, O’Dell & van Speybroeck 1996) can reach flux levels below 10−14 ergs cm−2s−1 in the 0.3–10 keV band.”
X-ray Spectroscopy of the Cluster of Galaxies Abell 1795 with XMM-Newton (2000, result): “Here we report the first results from the XMM (Jansen et al. 2001) observations of a rich cluster of galaxies, Abell 1795 (A1795 for short).”
Complex resonance absorption structure in the X-ray spectrum of IRAS 13349+2438 (2000, methodology): “IRAS 13349+2438 was observed with the XMM-Newton observatory (Jansen et al. 2001) on 19–20 June, 2000 during the Performance Verification phase for a total exposure time of 42 ks.”