A dataset provided by the European Space Agency

Name 010987
Title High-resolution X-ray spectroscopy of the cluster of galaxies 2A 0335+096
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0109870101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0109870201

DOI 10.5270/esa-82prywh
Author Dr Albert Brinkman
Description We propose to observe the cluster of galaxies 2A 0335+096 in order to perform spatially resolved spectroscopy with the RGS. 2A 0335+096 is an ideal target for this since it has a FWHM of only 1.4 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 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 Swift Burst Alert Telescope Perspective on Non-thermal Emission in HIFLUGCS Galaxy Clusters . Wik, Daniel R., Sarazin, Craig L., et all. . ApJ . 748-67 . 2012 . 2012ApJ...748...67W ,
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 confirmation of soft X-ray excess emission in clusters of galaxies - The discovery of O VII emission from an extended warm baryonic component . Kaastra, J. S., Lieu, R., et all. . A&A . 397-445 . 2003 . 2003A&A...397..445K ,
Spatially resolved X-ray spectroscopy of cooling clusters of galaxies . Kaastra, J. S., Tamura, T., et all. . A&A . 413-415 . 2004 . 2004A&A...413..415K ,
Elemental abundances in the intracluster medium as observed with XMM-Newton . Tamura, T., Kaastra, J. S., et all. . A&A . 420-135 . 2004 . 2004A&A...420..135T ,
Temperature and entropy profiles of nearby cooling flow clusters observed with XMM-Newton . Piffaretti, R., Jetzer, Ph...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2001-02-09T11:15:37Z/2001-02-09T22:48:49Z
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 2002-08-07T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2002-08-07T00:00:00Z, 010987, 17.56_20190403_1200. https://doi.org/10.5270/esa-82prywh