| Proposal ID | 076391 |
| Title | Determining the effects of baryonic feedback on galaxy cluster scaling relations |
| Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0763910301 |
| DOI | https://doi.org/10.5270/esa-fenfmog |
| Principal Investigator, PI | Mr Kimmo Kettula |
| Abstract | Calibration of scaling relations between weak lensing mass and X-ray observablesis a powerful tool for cluster count cosmology. Recent studies show thatenergetics due to feedback from active galaxies and star formation becomessignificant at group and low-mass cluster levels, implying that low mass systemsmight follow a different scaling than massive clusters. Here we propose toextend the X-ray coverage of low mass clusters in the CFHTLS field by a factorof approximately 4 in order to measure the effects of feedback on clusterscaling relations. |
| Publications |
|
| Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
| Temporal Coverage | 2015-07-07T10:29:49Z/2016-01-08T23:56:55Z |
| 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 | 2017-01-20T23:00:00Z |
| Last Update | 2025-01-27 |
| Keywords | "massive clusters", "cluster count cosmology", "cfhtls field", "scaling relations", "cluster scaling relations", "star formation", "xray coverage", "low mass cluster", "active galaxy", "powerful tool", "low mass systems", "baryonic feedback", "xray observables", "weak lensing mass" |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, Mr Kimmo Kettula, 2017, 'Determining the effects of baryonic feedback on galaxy cluster scaling relations', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-fenfmog |