A dataset provided by the European Space Agency

Proposal ID 011277
Title Spectral Variability of 3C 273
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DOI https://doi.org/10.5270/esa-t2b2sfc
Principal Investigator, PI Dr Martin Turner
Abstract GT-The time variability of 3C 273 is to be studied overthe first two years of XMM by repeated 5 ks observations(8 observations with 40 ks total, to be scheduled accordingto the visibility of the source). XMM is capable of observing the soft and the hard X-ray spectral components simultaneously thereby allowing to study the variability of the spectrum and its features, e.g that of the soft excess.
Publications
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2001-12-16T15:35:23Z/2003-12-14T22:57:30Z
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 2005-01-09T00:00:00Z
Keywords "time variability", "XMM", "soft excess", "spectral variability", "3c 273"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Martin Turner, 2005, 'Spectral Variability of 3C 273', PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.5270/esa-t2b2sfc