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<Article>
<Journal>
				<PublisherName>Damghan University Press</PublisherName>
				<JournalTitle>Iranian Journal of Astronomy and Astrophysics</JournalTitle>
				<Issn>2322-4924</Issn>
				<Volume>10</Volume>
				<Issue>4</Issue>
				<PubDate PubStatus="epublish">
					<Year>2023</Year>
					<Month>12</Month>
					<Day>30</Day>
				</PubDate>
			</Journal>
<ArticleTitle>Identification of Gamma-Ray Point Sources in Fermi-LAT Data with Minimum Spanning Tree Algorithm</ArticleTitle>
<VernacularTitle></VernacularTitle>
			<FirstPage>327</FirstPage>
			<LastPage>334</LastPage>
			<ELocationID EIdType="pii">385</ELocationID>
			
<ELocationID EIdType="doi">10.22128/ijaa.2023.736.1170</ELocationID>
			
			<Language>EN</Language>
<AuthorList>
<Author>
					<FirstName>Mehran </FirstName>
					<LastName>Soor</LastName>
<Affiliation>Department of Physics, K.N. Toosi University of Technology, Tehran, Iran</Affiliation>

</Author>
<Author>
					<FirstName>Fatemeh </FirstName>
					<LastName>Akhondi</LastName>
<Affiliation>Department of Physics, K.N Toosi University of Technology, 4 P.O. Box 15875-4416, Tehran, Iran</Affiliation>

</Author>
<Author>
					<FirstName>Hadi </FirstName>
					<LastName>Hedayati</LastName>
<Affiliation>Department of Physics, K.N. Toosi University of Technology, Tehran, Iran</Affiliation>

</Author>
</AuthorList>
				<PublicationType>Journal Article</PublicationType>
			<History>
				<PubDate PubStatus="received">
					<Year>2023</Year>
					<Month>09</Month>
					<Day>28</Day>
				</PubDate>
			</History>
		<Abstract>Gamma rays are the most energetic photons in the electromagnetic spectrum, detected with ground-based and space-based detectors in different energy ranges from sources in our galaxy and beyond. Gamma-ray point sources can be identified by special clustering of these photons. The minimum spanning tree (MST) algorithm is a graph-based method in order to find clusters. In this paper, we use the MST algorithm for finding point sources in Fermi gamma-ray space telescope data which is sensitive to photons with energies of 20 MeV up to more than 300 GeV. To this end, we selected eight completely random (10°×10°) fields of Fermi gamma-ray sky and tested the algorithm on the 12-year Fermi-LAT sky (Pass 8) at energy ranges above 3 GeV and above 6 GeV and with different cluster selection criteria. The calculation of Precision and Recall for both fields shows that MST is a useful algorithm in order to identify the point.</Abstract>
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			<Object Type="keyword">
			<Param Name="value">Astronomy data analysis</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">clustering</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">Gamma-ray sources</Param>
			</Object>
		</ObjectList>
<ArchiveCopySource DocType="pdf">https://ijaa.du.ac.ir/article_385_9e13b5118e28445c89addefd40f41ca2.pdf</ArchiveCopySource>
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