A dataset provided by the European Space Agency

Name 015936
Title RGS long-term long-wavelength contamination monitor
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0159360101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0159360301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0159360401
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https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0159360801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0159360901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0159361001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0159361101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0159361201
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https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0159361301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0159361401
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DOI https://doi.org/10.5270/esa-pw8lzwd
Author European Space Agency
Description Although contamination monitoring was introduced and vigorously pursued after
the RGS and MOS were cooled in 2002 November, it is important to establish a
long-term contamination monitor. The star zeta Puppis is an ideal target because
of the exceptional strength of its NVI and NVII lines at about 25 and 30A
respectively. So far, XMM has not been able to detect any variability in this
star above the few percent level. It is visible for 2 months every 6 months and
for this long-term programme, I propose a longer observation time than used
during the immediate post-cooling period, prefering instead the 60ks used for
the PV phase.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2003-05-30T09:29:28Z/2013-10-23T07:24:34Z
Version 17.56_20190403_1200
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.
Creator Contact https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published 2009-04-26T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2009, Rgs Long-Term Long-Wavelength Contamination Monitor, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-pw8lzwd