A dataset provided by the European Space Agency

Name 010995
Title High-resolution X-ray spectroscopy of the cluster of galaxies A 4059
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0109950101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0109950201

DOI 10.5270/esa-yt392k1
Author Dr Albert Brinkman
Description We propose to observe the cluster of galaxies A 4059 in order to perform spatially resolved spectroscopy with the RGS. A 4059 is an ideal target for this since it has a FWHM of only 2.5 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 Metal abundances in the cool cores of galaxy clusters . de Grandi, S., Molendi, S., . A&A . 508-565 . 2009 . 2009A&A...508..565D ,
HIFLUGCS: Galaxy cluster scaling relations between X-ray luminosity, gas mass, cluster radius, and velocity dispersion . Zhang, Y.-Y., Andernach, H., et all. . A&A . 526-105 . 2011 . 2011A&A...526A.105Z ,
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 ,
Normal galaxies in the XMM-Newton fields. X-rays as a star formation indicator . Rovilos, E., Georgantopoulos, I., et all. . A&A . 502-85 . 2009 . 2009A&A...502...85R ,
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 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. . ...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2000-11-24T04:04:18Z/2000-11-24T20:58:35Z
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 2002-03-20T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2002-03-20T00:00:00Z, 010995, 17.56_20190403_1200. https://doi.org/10.5270/esa-yt392k1