A dataset provided by the European Space Agency

Name 010986
Title High-resolution X-ray spectroscopy of the NGC 533 group of galaxies
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0109860101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0109860201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0109860401

DOI 10.5270/esa-7g0zbhv
Author Dr Albert Brinkman
Description We propose to observe the group of galaxies NGC 533 in order to perform spatially resolved spectroscopy with the RGS. This group is an ideal target for this since it has a FWHM of only 1.0 arcmin, allowing a high spectral resolution with the RGS and also an almost complete coverage of the cooling flow region of the cluster within the cross-dispersion width of the detector. In particular we will study the temperature and abundance distribution within the central region using the RGS. The EPIC observations will supplement this for the outer regions of the cluster, where we will study the abundance and temperature gradients as well as investigate the existence of non-thermal components.
Publication Exploring the X-ray sky with the XMM-Newton bright serendipitous survey . Della Ceca, R., Maccacaro, T., et all. . A&A . 428-383 . 2004 . 2004A&A...428..383D ,
High-precision multi-band measurements of the angular clustering of X-ray sources . Ebrero, J., Mateos, S., et all. . A&A . 500-749 . 2009 . 2009A&A...500..749E ,
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 ,
The x-ray luminous galaxy cluster population at 0.9 < z ≲ 1.6 as revealed by the XMM-Newton Distant Cluster Project . Fassbender, R., Bohringer, H., et all. . NJPh . 13-125014 . 2011 . 2011NJPh...13l5014F ,
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 ,
XMM-Newton study of 0.012 < z < 0.024 groups - I. Overview of the IGM thermodynamics . Finoguenov, A., Ponman, T. J., et all. . MNRAS . 374-737 . 2007 . 2007MNRAS.374..737F ,
A statistical analysis of the Two-Dimensional XMM-Newton Group Survey: the impact of feedback on group properties . Johnson, Ria, Ponman, Trevor J....
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2000-12-31T21:05:07Z/2002-01-01T18:19:27Z
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 2003-01-26T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2003-01-26T00:00:00Z, 010986, 17.56_20190403_1200. https://doi.org/10.5270/esa-7g0zbhv