A dataset provided by the European Space Agency

Name 067501
Title A combined X-ray and SZ study of the growth of cosmic structure


DOI 10.5270/esa-g16634z
Author Dr Karl Andersson
Description We propose to study the growth of cosmic structure by completing X-ray observations of the 20 z>0.7 clusters discovered in the first 600d of the SPT cluster survey. This proposal requests 545 ksec for 9 clusters with measured redshifts 0.73x10^14 M_sun. These observations are a critical part of a multi-wavelength campaign to calibrate SZE selected cluster masses using X-ray, weak lensing and velocity dispersions. In addition, the X-ray observations will directly constrain properties of clusters at z~1, including the metallicity of the ICM, the cool core fraction, and the deviations from self-similar evolution at high redshift. When combined with WMAP 7-year results and the SPT survey, the X-ray mass calibration will allow a 6% constraint on w, the dark energy equation of state parameter.
Publication SPT-CL J0205-5829: A z = 1.32 Evolved Massive Galaxy Cluster in the South Pole Telescope Sunyaev-Zel.dovich Effect Survey . Stalder, B., Ruel, J., et all. . ApJ . 763-93 . 2013 . 2013ApJ...763...93S ,
Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift . Yershov, V. N., . Ap&SS . 354-97 . 2014 . 2014Ap&SS.354...97Y ,
Baryon content of massive galaxy clusters at 0.57 < z < 1.33 . Chiu, I., Mohr, J., et all. . MNRAS . 455-258 . 2016 . 2016MNRAS.455..258C ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Cluster mass calibration at high redshift: HST weak lensing analysis of 13 distant galaxy clusters from the South Pole Telescope Sunyaev-Zel.dovich Survey . Schrabback, T., Applegate, D., et all. . MNRAS . 474-2635 . 2018 . 2018MNRAS.474.2635S ,
X-Ray Properties of SPT-selected Galaxy Clusters at 0.2 < z < 1.5 Observed with XMM-Newton . Bulbul, Esra, Chiu, I.-Non, et all. . ApJ . 871-50 . 2019 . 2019ApJ...871...50B ,
Mass calibration of the CODEX cluster sample using SPIDERS spectroscopy - II. The X-ray luminosity-mass relation . Capasso, R., Mohr, J. J., et all. . MNRAS . 494-2736 . 2020 . 2020MNRAS.494.2736C ,
Constraining radio mode feedback in galaxy clusters with the cluster radio AGNs properties to z u223c 1 . Gupta, N., Pannella, M., et all. . MNRAS . 4...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2011-06-07T19:48:58Z/2012-03-29T22:19:37Z
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 2013-04-18T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013-04-18T00:00:00Z, 067501, 17.56_20190403_1200. https://doi.org/10.5270/esa-g16634z