A dataset provided by the European Space Agency

Proposal ID 015556
Title OM UV Flux Calibration
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DOI https://doi.org/10.5270/esa-epkwoh2
Principal Investigator, PI Dr Fred Jansen XMM-Newton PS
Abstract UV Flux calibration for OM using White Dwarfs:HZ 4GD 50BD+33 2642G93-48BD+284211, Feige 66, Feige 67, Feige 110TT AriT Tau
Publications
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2002-08-11T12:58:47Z/2003-09-03T05:48:27Z
Version 17.56_20190403_1200
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 2004-03-21T00:00:00Z
Keywords "2642 g93", "uv flux calibration", "white dwarfs"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Fred Jansen XMM-Newton PS, 2004, 'OM UV Flux Calibration', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-epkwoh2