A dataset provided by the European Space Agency

Name 050243
Title Probing structure formation physics with the evolution of cluster properties
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0502430101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0502430201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0502430301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0502430401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0502430601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0502430701
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0502430801

DOI 10.5270/esa-ofxde6e
Author Dr Monique ARNAUD
Description We have been awarded a Large Program in AO4 to study the evolution of cluster structural and scaling properties, using an unbiased sample of 23 distant clusters (z~ 0.5) covering a wide dynamic range in mass (2.5 < kT < 12 keV). Our aim is to provide new insight into the physics of structure formation, both for the dark matter and the baryonic components. We propose to re-observe 6 targets, the observations of which are dramatically affected by flares.
Publication An XMM-Newton spatially-resolved study of metal abundance evolution in distant galaxy clusters . Baldi, A., Ettori, S., et all. . A&A . 537-142 . 2012 . 2012A&A...537A.142B ,
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 ,
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 ,
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 ,
X-ray variability of 104 active galactic nuclei. XMM-Newton power-spectrum density profiles . Gonzalez-Martin, O., Vaughan, S., . A&A . 544-80 . 2012 . 2012A&A...544A..80G , ...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2007-07-26T12:04:59Z/2007-12-09T15:19:12Z
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 2009-01-31T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2009-01-31T00:00:00Z, 050243, 17.56_20190403_1200. https://doi.org/10.5270/esa-ofxde6e