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Nature, ISSN 0028-0836, 12/2012, Volume 492, Issue 7428, pp. 225 - 228
Highly charged iron (Fe super(16+), here referred to as Fexvii) produces some of the brightest X-ray emission lines from hot astrophysical objects, including... 
Quantum mechanics | X-rays | Oscillator strengths | Emission | Mathematical models | Iron | Modelling | XMM (spacecraft)
Journal Article
Physical Review Letters, ISSN 0031-9007, 12/2014, Volume 113, Issue 25, pp. 251301 - 251301
We report a weak line at 3.52 +/- 0.02 keV in x-ray spectra of the Andromeda galaxy and the Perseus galaxy cluster observed by the metal-oxide-silicon (MOS)... 
EVENT FILES | PHOTON IMAGING CAMERA | MESSIER 31 | COSMOLOGY | CATALOG | PHYSICS, MULTIDISCIPLINARY | XMM-NEWTON OBSERVATIONS | STERILE NEUTRINOS | EDGE | WARM DARK-MATTER | Galactic clusters | Blanks | Andromeda Galaxy | Galaxies | X-rays | CCD cameras | Spectral lines | XMM (spacecraft)
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 04/2016, Volume 590
Context. Thanks to the large collecting area (3 x similar to 1500 cm(2) at 1.5 keV) and wide field of view (30' across in full field mode) of the X-ray cameras... 
surveys | X-rays: general | astronomical databases: miscellaneous | catalogs | PHOTON IMAGING CAMERA | LIGHT CURVES | ALL-SKY SURVEY | VIEW | VARIABILITY | POINT SOURCES | ASTRONOMY & ASTROPHYSICS | GALAXIES | DATA RELEASE | Pipelines | X-rays | X-ray sources | Catalogues | Spectra | XMM (spacecraft) | Arrays | Counting | Physics - High Energy Astrophysical Phenomena
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 09/2015, Volume 452, Issue 3, pp. 2641 - 2641
The Of?p star CPD -28...2561 was monitored at high energies with XMM-Newton and HST. In X-rays, this magnetic oblique rotator displays bright and hard emission... 
Stars | Compounding | X-rays | Displays | XMM (spacecraft) | Minima | Compounds | Maxima
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 01/2015, Volume 573, p. A53
Central compact objects (CCOs) in supernova remnants are isolated thermally emitting neutron stars (NSs). The thermal emission of CCOs can be modeled to obtain... 
Stars: atmospheres | Stars: neutron | Neutron stars | Supernova remnants | Equations of state | Cooling | Stars | Mathematical models | Spectra | XMM (spacecraft)
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 01/2018, Volume 609
We have investigated the ionic column density variability of the ionized outflows associated with NGC 7469, to estimate their location and power. This could... 
Lower bounds | Parameters | Galaxies | Ionization | Feedback | Variability | Dependence | Luminosity | Outflow | XMM (spacecraft) | Density
Journal Article
Astrophysical Journal Letters, ISSN 2041-8205, 11/2016, Volume 831, Issue 2, pp. L14 - L14
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 12/2018, Volume 620
Aims. A well characterised detection pipeline is an important ingredient for X-ray cluster surveys. Methods. We present the final development of the XXL Survey... 
Galactic clusters | Surveys | Active galactic nuclei | Galaxies | Pollution sources | Pipelines | Sky surveys (astronomy) | XMM (spacecraft) | X ray sources
Journal Article
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 04/2017, Volume 466, Issue 3, pp. 2918 - 2918
We report the results of a new XMM-Newton observation of the helium-rich hot subdwarf BD+37 degree 442 carried out in 2016 February. The possible periodicity... 
Stellar winds | Soft x-rays | X rays | Stars | Emission | Luminosity | XMM (spacecraft) | Companion stars
Journal Article
Astronomy & Astrophysics, ISSN 0004-6361, 04/2017, Volume 600
We have used our robotic TIGRE facility to closely monitor the star [tau] Boo during the last three observing seasons 2013-2016 and to determine its S-index... 
X rays | Phase shift | Stars | Monitors | Time | XMM (spacecraft) | Seasons | Solar cycles
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 11/2012, Volume 426, Issue 4, pp. 3271 - 3281
Journal Article
Astronomy & Astrophysics, ISSN 0004-6361, 01/2017, Volume 597
The determination of the thermodynamic properties of clusters of galaxies at intermediate and high redshift can bring new insights into the formation of... 
Galactic clusters | Red shift | Clusters | Pressure distribution | Electronics | Mathematical models | Entropy | XMM (spacecraft)
Journal Article
Astronomy & Astrophysics, ISSN 0004-6361, 01/2017, Volume 597
Aims. PSRJ0855-4644 is a fast-spinning, energetic pulsar discovered at radio wavelengths near the south-eastern rim of the supernova remnant RXJ0852.0-4622. A... 
Stellar winds | Angles (geometry) | X rays | Pulsars | Radio | Modelling | XMM (spacecraft) | Nebulae
Journal Article
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