NRCO - proposal to store all RGS requests as separate observationsobs1 RGS HTR mode observation of an empty field - BPM16274obs2 RGS observations of Sco-X1 with large offsetobs3 and 4 or 5: Her X-1 RGS HTR observationobs6 Mkn 421 offset dispobs7 and obs8 Mkn 421 offset Xdispobs9 Sco X-1 45. offsetobs 11-12-13 Mkn 421 NRCO 55obs 14 Vela Pulsar NRCO 59
Instrument
EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage
2001-12-14T15:04:38Z/2006-04-29T01:30:26Z
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, 2006, 'NRCO RGS main proposal', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-byvvcax
