Surveying the Gamma-ray sky with the BATSE and INTEGRAL satellites

Saved in:
Bibliographic Details
Title: Surveying the Gamma-ray sky with the BATSE and INTEGRAL satellites
Authors: Hill, Adam Ben
Summary: This thesis describes the developments and contributions made by Adam Hill to survey the Gamma-ray sky with the BATSE and INTEGRAL satellites. The soft γ-ray sky has been relatively unexplored on large scales. The last survey of the entire sky in this energy band was made by the HEAO-1 A4 mission in the late 1970's. This thesis takes advantage of new techniques and instruments to probe the source populations of the γ-ray sky in the energy band 20-160 keV. The BATSE instrument served as the all-sky monitor on-board the Compton Gamma-Ray Observatory for 9 years. By applying the newly developed LIMBO software and CLEAN algorithms an all-sky map of the sky is constructed using all 9 years of BATSE data. The map is constructed using data which spans the 30-160 keV energy band and produces a source catalogue of 36 sources down to a flux of ~20 mCrab. The performance and limitations of this new technique are assessed and presented. IBIS is the imager on-board the INTEGRAL γ-ray observatory. Data from IBIS is used in the construction of mosaics of the γ-ray sky which span the 20-100 keV energy band. The techniques and methods of the 1st and 2nd IBIS/ISGRI Survey Catalogues are presented which identify 123 and 209 discrete γ-ray sources respectively. The global properties of the sources of the 1st IBIS/ISGRI Survey Catalogue are analysed on a statistical basis. The properties of the X-ray binary populations and the unclassified INTEGRAL sources are presented. The unclassified source population are seen to share many of the characteristics of the high mass systems. A detailed study of IGR J18027-2016 indicates that it is a proto-typical example of the new INTEGRAL sources and is identified to be an obscured, supergiant high mass X-ray binary with a neutron star companion.
URL: https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.434099
Database: OpenDissertations
FullText Text:
  Availability: 0
Header DbId: ddu
DbLabel: OpenDissertations
An: ddu.oai.ethos.bl.uk.434099
AccessLevel: 6
PubType: Dissertation/ Thesis
PubTypeId: dissertation
PreciseRelevancyScore: 0
IllustrationInfo
Items – Name: Title
  Label: Title
  Group: Ti
  Data: Surveying the Gamma-ray sky with the BATSE and INTEGRAL satellites
– Name: Author
  Label: Authors
  Group: Au
  Data: <searchLink fieldCode="AR" term="%22Hill%2C+Adam+Ben%22">Hill, Adam Ben</searchLink>
– Name: Abstract
  Label: Summary
  Group: Ab
  Data: This thesis describes the developments and contributions made by Adam Hill to survey the Gamma-ray sky with the BATSE and INTEGRAL satellites. The soft γ-ray sky has been relatively unexplored on large scales. The last survey of the entire sky in this energy band was made by the HEAO-1 A4 mission in the late 1970's. This thesis takes advantage of new techniques and instruments to probe the source populations of the γ-ray sky in the energy band 20-160 keV. The BATSE instrument served as the all-sky monitor on-board the Compton Gamma-Ray Observatory for 9 years. By applying the newly developed LIMBO software and CLEAN algorithms an all-sky map of the sky is constructed using all 9 years of BATSE data. The map is constructed using data which spans the 30-160 keV energy band and produces a source catalogue of 36 sources down to a flux of ~20 mCrab. The performance and limitations of this new technique are assessed and presented. IBIS is the imager on-board the INTEGRAL γ-ray observatory. Data from IBIS is used in the construction of mosaics of the γ-ray sky which span the 20-100 keV energy band. The techniques and methods of the 1st and 2nd IBIS/ISGRI Survey Catalogues are presented which identify 123 and 209 discrete γ-ray sources respectively. The global properties of the sources of the 1st IBIS/ISGRI Survey Catalogue are analysed on a statistical basis. The properties of the X-ray binary populations and the unclassified INTEGRAL sources are presented. The unclassified source population are seen to share many of the characteristics of the high mass systems. A detailed study of IGR J18027-2016 indicates that it is a proto-typical example of the new INTEGRAL sources and is identified to be an obscured, supergiant high mass X-ray binary with a neutron star companion.
– Name: URL
  Label: URL
  Group: URL
  Data: <link linkTarget="URL" linkTerm="https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.434099" linkWindow="_blank">https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.434099</link>
PLink https://search.ebscohost.com/login.aspx?direct=true&site=eds-live&db=ddu&AN=ddu.oai.ethos.bl.uk.434099
RecordInfo BibRecord:
  BibEntity:
    Languages:
      – Code: eng
        Text: English
    Subjects:
      – SubjectFull: 522.68
        Type: general
    Titles:
      – TitleFull: Surveying the Gamma-ray sky with the BATSE and INTEGRAL satellites
        Type: main
  BibRelationships:
    HasContributorRelationships:
      – PersonEntity:
          Name:
            NameFull: Hill, Adam Ben
    IsPartOfRelationships:
      – BibEntity:
          Dates:
            – D: 01
              M: 01
              Type: published
              Y: 2006
ResultId 1