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<ArticleSet>
<Article>
<Journal>
				<PublisherName>The Physics Society of Iran</PublisherName>
				<JournalTitle>Iranian Journal of Physics Research</JournalTitle>
				<Issn>1682-6957</Issn>
				<Volume>11</Volume>
				<Issue>1</Issue>
				<PubDate PubStatus="epublish">
					<Year>2019</Year>
					<Month>11</Month>
					<Day>26</Day>
				</PubDate>
			</Journal>
<ArticleTitle>Searching in GaBoDS deep survey for clusters of galaxies by weak gravitational lensing</ArticleTitle>
<VernacularTitle>Searching in GaBoDS deep survey for clusters of galaxies by weak gravitational lensing</VernacularTitle>
			<FirstPage>69</FirstPage>
			<LastPage>77</LastPage>
			<ELocationID EIdType="pii">912</ELocationID>
			
			
			<Language>FA</Language>
<AuthorList>
<Author>
					<FirstName>M</FirstName>
					<LastName>Rahimi</LastName>
<Affiliation></Affiliation>

</Author>
<Author>
					<FirstName>SA</FirstName>
					<LastName>Najafi Shoushtari</LastName>
<Affiliation></Affiliation>

</Author>
<Author>
					<FirstName>S</FirstName>
					<LastName>Ghassemi</LastName>
<Affiliation></Affiliation>

</Author>
<Author>
					<FirstName>MT</FirstName>
					<LastName>Mirtorabi</LastName>
<Affiliation></Affiliation>

</Author>
</AuthorList>
				<PublicationType>Journal Article</PublicationType>
			<History>
				<PubDate PubStatus="received">
					<Year>2019</Year>
					<Month>11</Month>
					<Day>26</Day>
				</PubDate>
			</History>
		<Abstract>The aim of the present work is detection of galaxy clusters based on weak gravitational lensing method. We apply mass aperture statistics method to 0.32 square degrees data obtained with the WFI@MPG/ESO 2.2 m telescope and detect mass peaks based on their mass not the luminosity. So by the application of proper filter function, shear profile and mass map are produced. Finally mass peaks with higher detection significance are extracted. In future works, redshift of these mass concentrations and so their mass can be obtained.‎</Abstract>
			<OtherAbstract Language="FA">The aim of the present work is detection of galaxy clusters based on weak gravitational lensing method. We apply mass aperture statistics method to 0.32 square degrees data obtained with the WFI@MPG/ESO 2.2 m telescope and detect mass peaks based on their mass not the luminosity. So by the application of proper filter function, shear profile and mass map are produced. Finally mass peaks with higher detection significance are extracted. In future works, redshift of these mass concentrations and so their mass can be obtained.‎</OtherAbstract>
		<ObjectList>
			<Object Type="keyword">
			<Param Name="value">weak gravitational lensing</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">galaxies</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">galaxy clusters</Param>
			</Object>
		</ObjectList>
<ArchiveCopySource DocType="pdf">https://ijpr.iut.ac.ir/article_912_2a9d121cd9c3a1832bb6d2cc6bd7a8a7.pdf</ArchiveCopySource>
</Article>
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