|Title||EPIC GAIN, CTE AND CONTAMINATION MONITORING-N132D|
|Author||Dr Fred Jansen XMM-Newton PS|
|Description||CAL- During periods of low visibility, the primary target 1es0102 will be supplemented by observations of the bright LMC supernova remnant N132D. Due to source brightmess, small windows are used in EPIC -2.5ks overhead. Only UVW2 and UV grism usable in OM. Overhead 1ks per filter. A tempalate for a repeated observation without PA constraint is provided|
|Publication||No observations found associated with the current proposal|
|Instrument||EMOS1, EMOS2, EPN, OM, RGS1, RGS2|
|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, 2002-02-20T00:00:00Z, 012510, 17.56_20190403_1200. https://doi.org/10.5270/esa-sk46pc0|