A dataset provided by the European Space Agency

Proposal ID 012832
Title OM performance Verification of Fast Mode: OY Car
Download Data Associated to the proposal

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0128320301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0128320401

DOI https://doi.org/10.5270/esa-ngr30z7
Principal Investigator, PI Prof Keith Mason
Abstract PV- The aim is to observe the eclipsing dwarf nova system OY Car to verify theoperation of OM fast mode.
Publications
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2000-08-07T07:56:02Z/2000-08-07T15:24:00Z
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 2001-12-29T00:00:00Z
Keywords "oy car", "om fast mode", "fast mode", "om performance verification"
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Prof Keith Mason, 2001, 'OM performance Verification of Fast Mode: OY Car', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-ngr30z7