|Title||OM UV Photometric calibration using BPM16274|
|Author||Dr Fred Jansen XMM-Newton MM|
|Description||Routine calibration observation for OM photometry - BPM16274 Every 6 months, two different EPIC setup 01: MOS1-2: SW+LW diagnostic-- pn: ff closed noise (18ks) 11: all in FF Diagnostic 12: MOS1-2: Diagnostic 1x1, pn Noise (18ks) 13: MOS1-2: SW+LW diagnostic-- pn: ff closed noise (18ks) 15: MOS1-2: Diagnostic 1x1, pn Noise 16-18: MOS1-2: Diagnostic 1x1, pn Noise 17-19: MOS1-2: SW+LW diagnostic-- pn: ff closed noise (18ks)|
|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, 2016-05-16T22:00:00Z, 070158, 17.56_20190403_1200. https://doi.org/10.5270/esa-sr2lyl7|