A dataset provided by the European Space Agency

Proposal ID 011220
Title Study of X-ray emission from Pulsars with XMM
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DOI https://doi.org/10.5270/esa-b5j4jv4
Principal Investigator, PI Prof Keith Mason
Abstract GT- Isolated pulsars, formed in supernova events and powered by the rotationenergy, constitute one of the most energetic and possibly the purest phenomenain high-energy astrophysics.
Publications
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2001-04-03T10:52:28Z/2003-03-27T19:53:32Z
Version PPS_NOT_AVAILABLE
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.
Creator Contact https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published 2004-04-25T00:00:00Z
Keywords "XMM", "purest phenomena", "isolated pulsars", "rotation energy", "supernova events", "energy astrophysics", "xray emission"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Prof Keith Mason, 2004, 'Study of X-ray emission from Pulsars with XMM', PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.5270/esa-b5j4jv4