obs 6 NRCO: Offset observation to probe field that was contaminated by Jupiterwith V filter setting in rev.3224.obs 7 NRCO: Study effect of Jupiter accident on boresightobs 8 RCO: Hz 2 OM grisms absolute flux & V-grism wavelengthobs 9 RCO: Hz 2 OM grisms absolute flux & V-grism wavelengthobs 10 RCO: Hz 2 OM grisms absolute flux & V-grism wavelengthobs 11 NRCO110: Study effect of Jupiter accident on boresight
Instrument
EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage
2017-08-09T00:19:43Z/2024-02-20T17:58:07Z
Version
21.23_20231215_1101
Mission Description
The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs 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 Earths 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.
European Space Agency, Dr Peter Kretschmar XMM-Newton MM, 2024, 'OM Routine Calibration Observations', 21.23_20231215_1101, European Space Agency, https://doi.org/10.5270/esa-uvnj0e0
