NRCO - proposal to store all OM requests as separate observationsobs1: OM photometric zeropoints (Fei 16 offset)obs2: OM color-transformation (SA 95) and EPIC CALCLOSEDobs3: OM UV flux calibration and UV grism wavelength cal. (GL 172)obs4: OM UV flux calibration (G 191-B2B)obs5: NGC 6712obs6: LTT9491 OM Grism flux calibration
Instrument
EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage
2002-01-31T05:18:18Z/2003-12-05T09:04:17Z
Version
17.56_20190403_1200
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 Fred Jansen XMM-Newton PS, 2004, 'NRCO OM main proposal', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-rm47k23
