A dataset provided by the European Space Agency

Name 030211
Title A Detailed X-ray Study of a Supercluster at z = 0.9
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0302110201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0302110601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0302111001
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0302111101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0302111201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0302111301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0302111401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0302111501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0302111601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0302111701
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0302111801
...
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0302111901

DOI 10.5270/esa-helsqji
Author Prof Lori Lubin
Description We propose to obtain detailed X-ray data for an optically-selected supercluster at z = 0.9. This large scale structure contains at least seven massive clusters, most of which are known X-ray emitters. These observations will allow us to place accurate constraints on the temperature, surface-brightness profile, and mass fraction of the intracluster medium in the member clusters. The clusters are extremely well-studied in the optical; thus, the addition of XMM data will enable us to study the small-scale relation between the galaxies and gas, to quantify the variation between the X-ray-optical properties of clusters at a fixed epoch, and to explore a large scale system of clusters in the process of formation.
Publication An Extremely Luminous Panchromatic Outburst from the Nucleus of a Distant Galaxy . Levan, A. J., Tanvir, N. R., et all. . Sci . 333-199 . 2011 . 2011Sci...333..199L ,
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 ,
Are Optically Selected Quasars Universally X-Ray Luminous? X-Ray-UV Relations in Sloan Digital Sky Survey Quasars . Gibson, Robert R., Brandt, W. N., . ApJ . 685-773 . 2008 . 2008ApJ...685..773G ,
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 ,
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 ,
Cross-correlation of the 2XMMi catalogue with Data Release 7 of the Sloan Digital Sky Survey . Pineau, F.-X., Motch, C., et all. . A&A . 527-126 . 2011 . 2011A&A...527A.126P ,
Exploring X-ray and radio emission of type 1 AGN up to z ~ 2.3 . Ballo, L., Heras, F. J. H., et all. . A&A . 545-66 . 2012 . 2012A&A...545A..66B ,...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2005-12-20T02:48:30Z/2006-02-28T05:36:54Z
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 2007-06-17T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2007-06-17T00:00:00Z, 030211, 17.56_20190403_1200. https://doi.org/10.5270/esa-helsqji