Proposal ID | 041458 |
Title | NRCO 64: Investigation of EPIC soft flux discrepancies |
Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0414580101 |
DOI | https://doi.org/10.5270/esa-djvnejj |
Principal Investigator, PI | Dr Arvind Parmar XMM-Newton MM |
Abstract | see NRCO 64http://xmm.esac.esa.int/cgi-doc/ccb/NRCO_read?NRC=64 |
Publications |
|
Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
Temporal Coverage | 2007-04-24T06:54:00Z/2007-04-24T23:04:12Z |
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 | 2007-04-25T00:00:00Z |
Keywords | "epic soft flux", "cgi doc", "http :// xmm", "EPIC" |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, Dr Arvind Parmar XMM-Newton MM, 2007, 'NRCO 64: Investigation of EPIC soft flux discrepancies', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-djvnejj |