X-ray and lensing mass estimates in galaxy clusters

In this Thesis we have presented our work on the analysis of galaxy clusters through their X-ray emission and the gravitational lensing effect that they induce. Our research work was mainly finalised to verify and possibly explain the observed mismatch between the galaxy cluster mass distribution...

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Bibliographic Details
Main Author: Donnarumma, Annamaria <1981>
Other Authors: Moscardini, Lauro
Format: Doctoral Thesis
Language:en
Published: Alma Mater Studiorum - Università di Bologna 2010
Subjects:
Online Access:http://amsdottorato.unibo.it/2955/
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spelling ndltd-unibo.it-oai-amsdottorato.cib.unibo.it-29552014-03-24T16:28:48Z X-ray and lensing mass estimates in galaxy clusters Donnarumma, Annamaria <1981> FIS/05 Astronomia e astrofisica In this Thesis we have presented our work on the analysis of galaxy clusters through their X-ray emission and the gravitational lensing effect that they induce. Our research work was mainly finalised to verify and possibly explain the observed mismatch between the galaxy cluster mass distributions estimated through two of the most promising techniques, i.e. the X-ray and the gravitational lensing analyses. Moreover, it is an established evidence that combined, multi-wavelength analyses are extremely effective in addressing and explaining the open issues in astronomy: however, in order to follow this approach, it is crucial to test the reliability and the limitations of the individual analysis techniques. In this Thesis we also assessed the impact of some factors that could affect both the X-ray and the strong lensing analyses. Alma Mater Studiorum - Università di Bologna Moscardini, Lauro 2010-04-13 Doctoral Thesis PeerReviewed application/pdf en http://amsdottorato.unibo.it/2955/ info:eu-repo/semantics/restrictedAccess
collection NDLTD
language en
format Doctoral Thesis
sources NDLTD
topic FIS/05 Astronomia e astrofisica
spellingShingle FIS/05 Astronomia e astrofisica
Donnarumma, Annamaria <1981>
X-ray and lensing mass estimates in galaxy clusters
description In this Thesis we have presented our work on the analysis of galaxy clusters through their X-ray emission and the gravitational lensing effect that they induce. Our research work was mainly finalised to verify and possibly explain the observed mismatch between the galaxy cluster mass distributions estimated through two of the most promising techniques, i.e. the X-ray and the gravitational lensing analyses. Moreover, it is an established evidence that combined, multi-wavelength analyses are extremely effective in addressing and explaining the open issues in astronomy: however, in order to follow this approach, it is crucial to test the reliability and the limitations of the individual analysis techniques. In this Thesis we also assessed the impact of some factors that could affect both the X-ray and the strong lensing analyses.
author2 Moscardini, Lauro
author_facet Moscardini, Lauro
Donnarumma, Annamaria <1981>
author Donnarumma, Annamaria <1981>
author_sort Donnarumma, Annamaria <1981>
title X-ray and lensing mass estimates in galaxy clusters
title_short X-ray and lensing mass estimates in galaxy clusters
title_full X-ray and lensing mass estimates in galaxy clusters
title_fullStr X-ray and lensing mass estimates in galaxy clusters
title_full_unstemmed X-ray and lensing mass estimates in galaxy clusters
title_sort x-ray and lensing mass estimates in galaxy clusters
publisher Alma Mater Studiorum - Università di Bologna
publishDate 2010
url http://amsdottorato.unibo.it/2955/
work_keys_str_mv AT donnarummaannamaria1981 xrayandlensingmassestimatesingalaxyclusters
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