| Proposal ID | 021028 |
| Title | The Creation of the Intracluster Medium in High-z Galaxy Clusters |
| Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0210280101 |
| DOI | https://doi.org/10.5270/esa-pynkepz |
| Principal Investigator, PI | Dr Adam Stanford |
| Abstract | We propose to observe a newly discovered galaxy cluster around the radio galaxy3C 210 at z=1.17. We intend to obtain a 20 Ksec ACIS exposure to identify pointsources, which can severely bias measurements of extended emission in high-zclusters, and to study the radio galaxy itself. We also ask to obtain a 100 ksEPIC exposure to measure the properties of the intracluster medium including itsX-ray temperature and morphology. These observations will help to understand theway that galaxy clusters create an ICM as they evolve from the protoclustersrecently discovered at 2 |
| Publications |
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| Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
| Temporal Coverage | 2005-04-09T19:26:15Z/2005-04-11T02:58:20Z |
| 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 | 2006-07-07T00:00:00Z |
| Last Update | 2025-01-27 |
| Keywords | "EPIC", "z clusters", "epic exposure", "redshift galaxy cluster", "xray temperature", "galaxy cluster", "future exploitation", "bias measurements", "acis exposure", "dark energy", "z galaxy clusters", "galaxy cluster create", "intracluster medium", "radiogalaxy 3c 210" |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, Dr Adam Stanford, 2006, 'The Creation of the Intracluster Medium in High-z Galaxy Clusters', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-pynkepz |