Proposal ID | 011409 |
Title | EPIC mode and pile-up dependence - PKS0537 |
Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0114090101 |
DOI | https://doi.org/10.5270/esa-0c3uzmp |
Principal Investigator, PI | Dr Fred Jansen XMM-Newton PS |
Abstract | CAL- The effect of changing count rates on the spectral responce is measuredby observing similar AGN spectra at a range of fluxes.New proposal for observations on PKS0537 in replacement of PG1634+706 (propId = 10252), which was lacking visibility with XMM. |
Publications |
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Instrument | EMOS1, EMOS2, EPN, OM |
Temporal Coverage | 2000-03-19T12:11:49Z/2000-03-20T02:55:52Z |
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 | 2003-03-02T00:00:00Z |
Last Update | 2025-01-27 |
Keywords | "EPIC", "706 propid", "epic mode", "agn spectra", "spectral responce", "XMM", "changing count rates", "lacking visibility" |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, Dr Fred Jansen XMM-Newton PS, 2003, 'EPIC mode and pile-up dependence - PKS0537', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-0c3uzmp |