|Title||NRCO EPIC main proposal|
|Author||Dr Fred Jansen XMM-Newton PS|
|Description||NRCO - proposal to store all EPIC requests as separate observations: obs1-6:RXJ1856.6-3754 obs7-12: 1E 0102-72.2|
|Publication||Discovery of a 26.2 day period in the long-term X-ray light curve of SXP 1323: a very short orbital period for a long spin period pulsar . Carpano, S., Haberl, F., . A&A . 602-81 . 2017 . 2017A&A...602A..81C ,
Identification of AGN in the XMM-Newton X-ray survey of the SMC . Maitra, Chandreyee, Haberl, Frank, et all. . A&A . 622-29 . 2019 . 2019A&A...622A..29M ,
Hard X-Ray Excess from the Magnificent Seven Neutron Stars . Dessert, Christopher, Foster, Joshua W., . ApJ . 904-42 . 2020 . 2020ApJ...904...42D ,
|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, 2016-05-04T22:00:00Z, 079158, 17.56_20190403_1200. https://doi.org/10.5270/esa-z92aiss|