A dataset provided by the European Space Agency

Name 012832
Title OM performance Verification of Fast Mode: OY Car
URL

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
Author European Space Agency
Description PV- The aim is to observe the eclipsing dwarf nova system OY Car to verify the
operation of OM fast mode.
Publication No observations found associated with the current proposal
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 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 2001-12-29T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2001, Om Performance Verification Of Fast Mode: Oy Car, 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-ngr30z7