A dataset provided by the European Space Agency

Proposal ID 081081
Title RGS long-wavelength response and the MOS CTI with the Vela
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DOI https://doi.org/10.5270/esa-ouy89bz
Principal Investigator, PI Dr Peter Kretschmar XMM-Newton MM
Abstract Routine Calibration RGS: RGS long-wavelength response
Publications No publications found for current proposal!
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2019-05-17T20:20:29Z/2024-05-31T06:22:06Z
Version 21.23_20231215_1101
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 2024-06-07T00:00:00Z
Keywords "wavelength response", "mos cti", "routine calibration rgs"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Dr Peter Kretschmar XMM-Newton MM, 2024, 'RGS long-wavelength response and the MOS CTI with the Vela', 21.23_20231215_1101, European Space Agency, https://doi.org/10.5270/esa-ouy89bz