Please use this identifier to cite or link to this item: http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/7841
Full metadata record
DC FieldValueLanguage
dc.contributor.advisorBhattacharyya, Sudip-
dc.contributor.authorNAIR, SHASWAT-
dc.date.accessioned2023-05-13T06:51:20Z-
dc.date.available2023-05-13T06:51:20Z-
dc.date.issued2023-05-
dc.identifier.citation51en_US
dc.identifier.urihttp://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/7841-
dc.description.abstractPSR J102347.6 +003841 (also known as PSR J1023) is one of three known transitional millisecond pulsars (tMSP). We analyze EPIC X-ray data from the XMM-Newton satellite to probe multiple X-ray states of this star. By analyzing a combined total of 18 bservations across multiple years, we hope to provide a comprehensive picture of the spectral properties of this source and analyze the effectiveness of various models in successfully describing its behavior. We perform the spectral fitting and modeling of the source using the spectral modeling software XSPEC and other tools within the publicly available Heasoft package.en_US
dc.language.isoenen_US
dc.subjectpulsars: generalen_US
dc.subjectpulsars:PSR J1023+0038en_US
dc.subjectstars:neutronen_US
dc.subjectX-rays:binariesen_US
dc.titleThe spectral analysis of the transitional millisecond pulsar J1023+0038en_US
dc.typeThesisen_US
dc.description.embargoOne Yearen_US
dc.type.degreeBS-MSen_US
dc.contributor.departmentDept. of Physicsen_US
dc.contributor.registration20181187en_US
Appears in Collections:MS THESES

Files in This Item:
File Description SizeFormat 
20181187_NAIR_SHASWAT_MS_ThesisMS Thesis430.06 kBAdobe PDFView/Open


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.