| Proposal ID | 082735 |
| Title | Witnessing the culmination of structure formation in the Universe |
| Download Data Associated to the proposal | https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0827350101 |
| DOI | https://doi.org/10.5270/esa-rvblmo7 |
| Principal Investigator, PI | Dr M S Arnaud-Ettori |
| Abstract | This is a Heritage program to study the ultimate products of structure formationin mass and time\: a large, unbiased, signal-to-noise limited sample of galaxyclusters detected by Planck via their Sunyaev-Zeldovich effect. Completing thehigh-fidelity XMM coverage of this sample has extraordinary legacy value. Wewill (i) obtain an unbiased vision of the statistical properties of the clusterpopulation; (ii) uncover the provenance of non-gravitational heating; (iii)measure how their gas is shaped by the collapse into dark matter haloes and themergers that built todays clusters; (iv) resolve the major uncertainties in massdeterminations that limit cosmological inferences; (v) build the foundation forcluster science with next-generation surveys. |
| Publications |
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| Instrument | EMOS1, EMOS2, EPN, OM, RGS1, RGS2 |
| Temporal Coverage | 2020-11-02T14:08:50Z/2021-01-05T13:25:48Z |
| 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 | 2021-01-13T00:00:00Z |
| Keywords | "statistical properties", "dark matter haloes", "noise limited sample", "gravitational heating", "cluster science", "major uncertainties", "built todays clusters", "fidelity xmm coverage", "iv resolve", "cluster population", "limit cosmological inferences", "XMM", "generation surveys", "planck via", "ii uncover", "unbiased vision", "time \:", "heritage program", "galaxy cluster", "sunyaev zeldovich effect", "structure formation", "mass determinations" |
| Publisher And Registrant | European Space Agency |
| Credit Guidelines | European Space Agency, Dr M S Arnaud-Ettori, 2021, 'Witnessing the culmination of structure formation in the Universe', 18.02_20200221_1200, European Space Agency, https://doi.org/10.5270/esa-rvblmo7 |