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XMM-NewtonX-Ray Multi-Mirror Mission
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Luckily enough, the two flagship X-ray observatories, the ESA-led XMM-Newton and the NASA-led Chandra took snapshots of the same area of the sky close in time to the peak of the flare, and again about ten years later.
NuSTAR and XMM-Newton simultaneously observed PDS 456 on five separate occasions in 2013 and 2014.
The discoveries have been made using NASA's flagship observatory Chandra X-ray Observatory and Europe's XMM-Newton Observatory.
On the same day, LogicaCMG also announces the successful deployment of a new generation of ground control software, which will make future operations of Europe's largest scientific satellite, XMM-Newton, more cost effective.
ESA has had many successful missions recently, including the XMM-Newton, Envisat and Rosetta.
Chandra, XMM-Newton and Astro E, since it contains the largest collection of data available on soft x-ray transitions.
She has published more than 150 scientific papers and was co-principal investigator for a telescope experiment that is currently flying on the satellite XMM-Newton, a cornerstone mission of the European Space Agency.
Heinz and his colleagues quickly mounted a series of follow-up observations with the space-based Chandra and XMM-Newton telescopes to discover four bright rings of X-rays, like ripples in a cosmic pond, all around the neutron star at the heart of Circinus X-1.
Washington, June 25 ( ANI ): Researchers are mystified by a mysterious X-ray signal which has been found in a detailed study of galaxy clusters using NASA's Chandra X-ray Observatory and ESA's XMM-Newton.
De Witt attended a COSPAR Capacity Building Workshop on Space Astrophysics with NASA & ESA Missions: Swift, Chandra & XMM-Newton in Alexandria, Egypt in January 2008.
Two teams--one led by Garmire using NASA's Chandra X-ray Observatory and the other led by Andrea De Luca of the National Institute of Astrophysics in Milan using the European Space Agency's XMM-Newton satellite--have found that X rays emitted by the star wax and wane every 6.
Among specific topics are observational population studies of the variables, faint X-ray sources in globular clusters in the XMM-Newton and Chandra era, jets and outflows in micro-quasars, a model for low accretions rate polars, the spreading layer and dwarf nova oscillations, correlated X-ray and optical variability in X-ray binaries, and white dwarfs undergoing hydrogen shell burning single degenerate binary systems.