A dataset provided by the European Space Agency

Name 021208
Title THE OM UV red leak and other NRCO
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0212080101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0212080201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0212080301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0212080401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0212080501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0212080601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0212080701

DOI https://doi.org/10.5270/esa-k82voqt
Author Dr Fred Jansen XMM-Newton MM
Description The OM UV filters have effective wavelengths of 2910, 2310, and 2120
angstroms for UVW1, UVM2, UVW2, respectively. Some evidence has shown
that the UV filters might have a red leak which allows light outside
nominal bandpass through to the detector.
In order to get a quantitative measurement of the UV red leaks, we
need to observe one set of stars with different spectral type and
interstellar reddening. In this NRCO, we ask for 45 ks observing time
to observe 5 targets, with spectral type from O5 to M3.5 and extinction
up to Av=15.8 mag. Each requested target should be observed in all six
filters and two grisms.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2004-12-18T20:00:41Z/2005-05-09T01:06:02Z
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 2005-05-09T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Fred Jansen XMM-Newton MM, 2005, 021208, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-k82voqt