A dataset provided by the European Space Agency

Name 072070
Title Baryons and Dark Matter in Hubble Treasury Clusters
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0720700101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0720700201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0720700301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0720700401

DOI 10.5270/esa-dxd2r3y
Author Dr Megan Donahue
Description The distribution of dark matter, baryons, and stars in a cluster gravitational potential is a fundamental prediction of large-scale structure formation. We have 524 orbits of HST imaging together with Subaru and VLT spectroscopy to measure the strong and weak lensing properties of 20 relaxed and 5 high-magnification galaxy clusters (z = 0.18 - 0.90, Tgas > 5 keV). Observing the last 3 relaxed clusters with good visibility lacking XMM data will permit uniform joint Xray-lensing-SZ analysis for 17 of the relaxed systems to advance our understanding of the shapes and concentrations of the mass profiles, providing precise observational benchmarks for baryonic and dark matter distributions over a range of redshifts.
Publication Scaling Relations and X-Ray Properties of Moderate-luminosity Galaxy Clusters from 0.3 < z < 0.6 with XMM-Newton . Connor, Thomas, Donahue, Megan, et all. . ApJ . 794-48 . 2014 . 2014ApJ...794...48C ,
High angular resolution Sunyaev-Zel.dovich observations of MACS J1423.8+2404 with NIKA: Multiwavelength analysis . Adam, R., Comis, B., et all. . A&A . 586-122 . 2016 . 2016A&A...586A.122A ,
XMM-Newton publication statistics . Ness, J.-U., Parmar, A. N., et all. . AN . 335-210 . 2014 . 2014AN....335..210N ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Recovering galaxy cluster gas density profiles with XMM-Newton and Chandra . Bartalucci, I., Arnaud, M., et all. . A&A . 608-88 . 2017 . 2017A&A...608A..88B ,
LoCuSS: pre-processing in galaxy groups falling into massive galaxy clusters at z = 0.2 . Bianconi, M., Smith, G. P., et all. . MNRAS . 473-79 . 2018 . 2018MNRAS.473L..79B ,
Thermodynamic profiles of galaxy clusters from a joint X-ray-SZ analysis . Shitanishi, Jennifer A., Pierpaoli, Elena, et all. . MNRAS . 481-749 . 2018 . 2018MNRAS.481..749S ,
Astrophysics with the Spatially and Spectrally Resolved Sunyaev-Zeldovich Effects. A Millimetre-Submillimetre Probe of the Warm and Hot Universe . Mroczkowski, Tony, Nagai, Daisuke, et all. . SSRv . 215-17 . 2019 . ...,
The XMM Cluster Survey: new evidence for the 3.5-keV feature in clusters is inconsistent with a dark matter origin . Bhargava, S., Giles, P. A., et all. . MNRAS . 497-656 . 2020 . 2020MNRAS.497..656B ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2013-08-22T22:03:38Z/2014-02-09T14:25:01Z
Version 17.56_20190403_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 2015-02-27T23:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2015-02-27T23:00:00Z, 072070, 17.56_20190403_1200. https://doi.org/10.5270/esa-dxd2r3y