Proposal ID | 080076 |
Title | Scaling Properties and the Effects of Feedback for a Complete Sample of Groups |
Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0800760101 |
DOI | https://doi.org/10.5270/esa-t0bl41r |
Principal Investigator, PI | Dr Lorenzo Lovisari |
Abstract | The largest fraction of matter content in the Universe is attributed to galaxygroups, therefore they play a key role in astrophysics and cosmology. UpcomingX-ray surveys like eROSITA, require precise calibration between X-rayobservables and mass, down to the low mass regime to set tight constraints onthe fundamental cosmological parameters. We propose to observe 14 galaxy groupswith a total exposure time of 137 ks to complete observations for a flux limitedsample consisting of 69 objects. The requested data will allow to preciselycorrect for selection effects the scaling relations, with an improvement on thecorrected scaling relations by a factor of 2 with respect to what can be donewith the current data. |
Publications |
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Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
Temporal Coverage | 2017-06-10T07:17:04Z/2018-04-20T02:52:14Z |
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 | 2019-05-14T22:00:00Z |
Last Update | 2025-08-04 |
Keywords | "total exposure time", "key role", "scaling properties", "require precise calibration", "low mass regime", "corrected scaling relations", "matter content", "largest fraction", "requested data", "fundamental cosmological parameters", "selection effects", "precisely correct", "xray surveys", "set tight constraints", "scaling relations", "complete sample", "xray observables" |
Publisher And Registrant | European Space Agency |
Credit Guidelines | European Space Agency, Dr Lorenzo Lovisari, 2019, 'Scaling Properties and the Effects of Feedback for a Complete Sample of Groups', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-t0bl41r |