Integral and XMM-Newton missions extended

In recognition of their superb scientific output, the mission operations of European flagship x-ray and gamma-ray observatories, XMM-Newton and Integral, have been extended until 31 December 2012.

The extension of both missions, which have been producing an incessant flow of science results since launch, was announced this week after a unanimous vote at a meeting of ESA's Science Programme Committee.
Integral science highlights

With its sensitive detectors, Integral has accurately measured the hard Cosmic X-ray Background (CXB), responsible for creating the diffuse background glow spread throughout the universe, and it has confirmed that systems containing white dwarves contribute significantly to the galactic hard X-ray diffuse emission.

The gamma-ray observatory has a found a rare class of anomalous X-ray pulsars, with magnetic fields a thousand million times stronger than the strongest steady magnetic field achievable in a laboratory on Earth, and has found massive stars by looking for their radioactive traces - radioactive decay gamma-ray lines from iron have been observed with the most significant detection to date, forcing re-evaluation of existing theoretical models.

Integral has also discovered a new class of X-ray binary stars called super-giant fast transients - X-ray binary systems containing super giant stars. Integral and other high-energy satellites have discovered that these transient systems are not as rare in the galaxy as initially thought.

Although not designed for the purpose, Integral has also proved to be a great gamma-ray-burst 'watchdog', providing instantaneous, accurate positions of gamma ray bursts to other facilities within minutes or even seconds. In collaboration with NASA's Rossi X-ray Timing Explorer, Integral has also detected what appears to be the fastest spinning neutron star yet.

XMM-Newton science highlights

In the last two years XMM-Newton has made breakthrough observations of a wide variety of compact objects, such as the first detection of an intermediate-mass black hole in globular cluster NGC 4472. This has direct implications for the formation and evolution theories of globular clusters in general.

Thanks to its sensitivity at high energies, XMM-Newton has made the first and only direct probing of the central regions near a black hole, by sampling the presence of iron and the variability of its spectral fingerprints. The satellite's observations have also been fundamental in helping understand the physics of heavy sub-atomic matter ('baryonic') in clusters of galaxies and on studying the dark matter component in clusters.

XMM-Newton has given the first strong indication that very faint active galactic nuclei (AGN) are similar to the 'normal' AGN population, and measured for the first time the size of the emission region of an AGN.

Other major results include the progress in understanding the link between X-ray emission and luminosity of stars, as well as the relation between the X-ray emission and processes such as star accretion or collisions.

The satellite has also discovered the remnants of a new class of supernovae within the so-called 'Ia type', which are used as standard reference, or 'candles', to determine stellar luminosity.

XMM-Newton has also revealed X-ray emission in the Martian exosphere - the first definite detection of X-ray emission induced by exchange of electrical charges from the exosphere of another planet.

Source: European Space Agency
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