A dataset provided by the European Space Agency

Name 040663
Title Radio source ageing and the quenching of cooling cores in clusters
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0406630201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0406630501

DOI 10.5270/esa-uw3c2ua
Author Dr Elena Belsole
Description We propose to complete the high-quality X-ray observations of a sample of 35 intermediate-redshift bright galaxy clusters by observing 4 with XMM-Newton. The sample is unbiased in X-ray morphology and radio-source content, and is of sufficient size to permit us to address the extent to which cooling flows are halted by mechanical energy injected by radio sources, and if the dynamical state of the cluster gas correlates with the radio environment. This will be achieved by comparing the X-ray-derived temperature, entropy and pressure structures with the energy contents, ages and distributions of the radio-source components within the clusters.
Publication The Origin of the Hot Gas in the Galactic Halo: Confronting Models with XMM-Newton Observations . Henley, David B., Shelton, Robin L., et all. . ApJ . 723-935 . 2010 . 2010ApJ...723..935H ,
An XMM-Newton Survey of the Soft X-ray Background. I. The O VII and O VIII Lines Between l = 120 and l = 240 . Henley, David B., Shelton, Robin L., . ApJS . 187-388 . 2010 . 2010ApJS..187..388H ,
A serendipitous XMM survey of the SDSS: the evolution of the colour-magnitude diagram of X-ray AGN from z= 0.8 to 0.1 . Georgakakis, Antonis, Nandra, K., . MNRAS . 414-992 . 2011 . 2011MNRAS.414..992G ,
Exospheric solar wind charge exchange as seen by XMM-Newton . Carter, J. A., Semba, S., . AN . 333-313 . 2012 . 2012AN....333..313C ,
The cosmological analysis of X-ray cluster surveys - II. Application of the CR-HR method to the XMM archive . Clerc, N., Sadibekova, T., et all. . MNRAS . 423-3561 . 2012 . 2012MNRAS.423.3561C ,
An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities . Henley, David B., Shelton, Robin L., . ApJS . 202-14 . 2012 . 2012ApJS..202...14H ,
Joint Analysis of Cluster Observations. II. Chandra-XMM-Newton X-Ray and Weak Lensing Scaling Relations for a Sample of 50 Rich Clusters of Galaxies . Mahdavi, Andisheh, Hoekstra, Henk, et all. . ApJ . 767-116 . 2013 . 2013ApJ...767..116M ,
An XMM-Newton Surve...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2007-04-12T12:14:39Z/2007-04-13T02:02:32Z
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 2008-05-09T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2008-05-09T00:00:00Z, 040663, 17.56_20190403_1200. https://doi.org/10.5270/esa-uw3c2ua