|Title||Rev 26, (after RGS-2 door open)|
|Author||Mr Fred Jansen XMM-Newton PS|
|Publication||Calibration and in-orbit performance of the reflection grating spectrometer onboard XMM-Newton . de Vries, C. P., den Herder, J. W., et all. . A&A . 573-128 . 2015 . 2015A&A...573A.128D ,
The Rotation of the Hot Gas around the Milky Way . Hodges-Kluck, Edmund J., Miller, Matthew J., . ApJ . 822-21 . 2016 . 2016ApJ...822...21H ,
Why solar astronomers should be interested in stars . Pallavicini, R., . AdSpR . 32-885 . 2003 . 2003AdSpR..32..885P ,
Studying Cosmic Evolution with the XMM-Newton Distant Cluster Project: X-ray Luminous Galaxy Clusters at z>~1 and their Galaxy Populations . Fassbender, Rene, . PhDT . 0-116 . 2008 . 2008PhDT.......116F ,
A Comparison of X-Ray Photon Indices among the Narrow- and Broad-line Seyfert 1 Galaxies . Ojha, Vineet, Chand, Hum, et all. . ApJ . 896-95 . 2020 . 2020ApJ...896...95O ,
|Mission Description||The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations.
Since Earth's atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
|Publisher And Registrant||European Space Agency|
|Credit Guidelines||European Space Agency, 2000-03-09T00:00:00Z, 011615, 17.56_20190403_1200. https://doi.org/10.5270/esa-zdv80ri|