A dataset provided by the European Space Agency

Name 082706
Title Witnessing the culmination of structure formation in the Universe
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0827060201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0827060601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0827060701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0827060801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0827061001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0827061301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0827061401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0827061701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0827061801

DOI https://doi.org/10.5270/esa-wtsyx76
Author Dr M S Arnaud-Ettori
Description This is a Heritage program to study the ultimate products of structure formation in mass and time: a large, unbiased, signal-to-noise limited sample of galaxy clusters detected by Planck via their Sunyaev-Zel.dovich effect. Completing the high-fidelity XMM coverage of this sample has extraordinary legacy value. We will (i) obtain an unbiased vision of the statistical properties of the cluster population; (ii) uncover the provenance of non-gravitational heating; (iii) measure how their gas is shaped by the collapse into dark matter haloes and the mergers that built today.s clusters; (iv) resolve the major uncertainties in mass determinations that limit cosmological inferences; (v) build the foundation for cluster science with next-generation surveys.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2019-08-20T04:56:33Z/2021-08-26T02:55:30Z
Version 19.16_20210326_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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 2021-09-28T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2021-09-28T00:00:00Z, 082706, 19.16_20210326_1200. https://doi.org/10.5270/esa-wtsyx76