A dataset provided by the European Space Agency

Name 030203
Title Radio relic-merger connection in the clusters A548b and A1664
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0302030101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0302030201

DOI 10.5270/esa-usdpyoa
Author Dr Luigina Feretti
Description The clusters A548b and A1664 are peculiar in the radio domain because of the presence of radio relics. These are very extended diffuse radio sources, located in cluster peripheral regions, and associated with the intracluster medium. According to theoretical models, the radio relics are energized by cluster merger shocks. We wish to investigate the cluster X-ray properties, the status of the intracluster medium, the presence of shocks, filaments or cold fronts, in order to analyze the energy transfer between the thermal gas and the radio emitting particles. The study of the connection between X-ray and radio emission will be crucial to understand the formation of relics, and more generally of the non-thermal components in clusters, and their relation to the cluster dynamics.
Publication The dynamical state of A548 from XMM-Newton data: X-ray and radio connection . Solovyeva, L., Anokhin, S., et all. . A&A . 484-621 . 2008 . 2008A&A...484..621S ,
The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue . Watson, M. G., Schroder, A. C., et all. . A&A . 493-339 . 2009 . 2009A&A...493..339W ,
Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras . Mateos, S., Saxton, R. D., et all. . A&A . 496-879 . 2009 . 2009A&A...496..879M ,
The XMM Cluster Survey: optical analysis methodology and the first data release . Mehrtens, Nicola, Romer, A. Kathy, et all. . MNRAS . 423-1024 . 2012 . 2012MNRAS.423.1024M ,
An All-Sky Atlas of Radio-X-ray Associations . Flesch, E., . PASA . 27-283 . 2010 . 2010PASA...27..283F ,
The XMM Cluster Survey: X-ray analysis methodology . Lloyd-Davies, E. J., Romer, A. Kathy, et all. . MNRAS . 418-14 . 2011 . 2011MNRAS.418...14L ,
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 ,
Classification of X-Ray Sources in t...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2005-07-28T07:29:36Z/2006-02-17T20:29:17Z
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 2007-03-04T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2007-03-04T00:00:00Z, 030203, 17.56_20190403_1200. https://doi.org/10.5270/esa-usdpyoa