| Proposal ID | 085379 |
| Title | NRCO-108: Long term energy scale of PN Large Window Mode |
| Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0853790101 |
| DOI | https://doi.org/10.5270/esa-o6ues2k |
| Principal Investigator, PI | Dr Peter Kretschmar XMM-Newton MM |
| Abstract | There are not enough suitable EPIC-pn observations in Large Window mode inCalClosed or sky sources with Fe Kalpha line at 6.4 keV to derive a correctionfor the long-term CTI for this mode above 6 keV.The objective of this observation is to match an early observation of Kepler SNR(0084100101, rev 229, 10 March 2001) with a new observation in order toestablish the long-term behaviour the CTI at 6.4 keV. This can potentially beextended to other lines in the Kepler SNR at lower energies, e.g. Si K line at1.8 keV and S K line at 2.4 keV. The setup should match as much as possible thatof the original observation 0084100101. |
| Publications | No publications found for current proposal! |
| Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
| Temporal Coverage | 2020-03-11T04:29:01Z/2020-03-11T15:14:01Z |
| Version | 18.02_20200221_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 | 2020-03-28T00:00:00Z |
| Last Update | 2025-01-27 |
| Keywords | "EPIC", "nrco 108", "window mode", "suitable epic pn", "lower energies", "fe kalpha line", "rev 229", "kepler supernova remnant", "term cti", "term energy scale", "sky sources" |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, Dr Peter Kretschmar XMM-Newton MM, 2020, 'NRCO-108: Long term energy scale of PN Large Window Mode', 18.02_20200221_1200, European Space Agency, https://doi.org/10.5270/esa-o6ues2k |