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  • 1
    UID:
    b3kat_BV047094017
    Format: 1 Online-Ressource (XXIV, 311 p. 208 illus., 130 illus. in color)
    Edition: 1st ed. 2021
    ISBN: 9783030603618
    Series Statement: Springer Theses, Recognizing Outstanding Ph.D. Research
    Additional Edition: Erscheint auch als Druck-Ausgabe ISBN 978-3-030-60360-1
    Additional Edition: Erscheint auch als Druck-Ausgabe ISBN 978-3-030-60362-5
    Additional Edition: Erscheint auch als Druck-Ausgabe ISBN 978-3-030-60363-2
    Language: English
    URL: Volltext  (URL des Erstveröffentlichers)
    Library Location Call Number Volume/Issue/Year Availability
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  • 2
    UID:
    almahu_9948612922502882
    Format: XXIV, 311 p. 208 illus., 130 illus. in color. , online resource.
    Edition: 1st ed. 2021.
    ISBN: 9783030603618
    Series Statement: Springer Theses, Recognizing Outstanding Ph.D. Research,
    Content: This thesis describes the application of state-of-the-art high-energy X-ray studies to the astronomical quest for understanding obscured active galactic nuclei (AGN). These AGN are supermassive black holes growing by accretion of matter located in the nuclei of galaxies. The material that feeds these black holes also obscures them from view, rendering them challenging to study. It is possible to study them by effectively 'X-raying' galactic nuclei to peer through these obscuring veils. Beginning with the proof-of-concept application of novel X-ray Monte Carlo codes to the Nuclear Spectroscopic Telescope ARray (NuSTAR) spectrum of a known heavily obscured AGN, the thesis establishes the relevant parameters that characterise the AGN spectrum and central black hole growth rate. Next the largest sample of known heavily obscured AGN is compiled, finding the strength of a prominent iron spectral feature to weaken with AGN power. This is puzzling, and suggests that there may be more hidden AGN than previously thought. Finally by combining an all-sky infrared selection with NuSTAR follow-up, new heavily obscured AGN are identified. Obscuration emits infrared radiation, meaning that the infrared-selected AGN catalogue should be representative of the underlying AGN population. The absence of such representative catalogues has continually plagued cosmological studies, and the resultant obscured AGN fraction will be strongly constraining for AGN models.
    Note: Introduction -- IC 3639 - A New Bona Fide Compton-thick AGN Unveiled by NuSTAR -- An Iwasawa-Taniguchi Effect for Compton-thick Active Galactic Nuclei -- The NuSTAR Local AGN NH Distribution Survey: Prospects for Mitigating Obscuration Bias in Local AGN Selection -- The NuLANDS NH Distribution -- Summary, Conclusions & Outlook.
    In: Springer Nature eBook
    Additional Edition: Printed edition: ISBN 9783030603601
    Additional Edition: Printed edition: ISBN 9783030603625
    Additional Edition: Printed edition: ISBN 9783030603632
    Language: English
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  • 3
    UID:
    gbv_1743800754
    Format: 1 Online-Ressource (XXIV, 311 Seiten) , Illustrationen, Diagramme
    ISBN: 9783030603618
    Series Statement: Springer Theses
    Content: Introduction -- IC 3639 – A New Bona Fide Compton-thick AGN Unveiled by NuSTAR -- An Iwasawa-Taniguchi Effect for Compton-thick Active Galactic Nuclei -- The NuSTAR Local AGN NH Distribution Survey: Prospects for Mitigating Obscuration Bias in Local AGN Selection -- The NuLANDS NH Distribution -- Summary, Conclusions & Outlook.
    Content: This thesis describes the application of state-of-the-art high-energy X-ray studies to the astronomical quest for understanding obscured active galactic nuclei (AGN). These AGN are supermassive black holes growing by accretion of matter located in the nuclei of galaxies. The material that feeds these black holes also obscures them from view, rendering them challenging to study. It is possible to study them by effectively 'X-raying' galactic nuclei to peer through these obscuring veils. Beginning with the proof-of-concept application of novel X-ray Monte Carlo codes to the Nuclear Spectroscopic Telescope ARray (NuSTAR) spectrum of a known heavily obscured AGN, the thesis establishes the relevant parameters that characterise the AGN spectrum and central black hole growth rate. Next the largest sample of known heavily obscured AGN is compiled, finding the strength of a prominent iron spectral feature to weaken with AGN power. This is puzzling, and suggests that there may be more hidden AGN than previously thought. Finally by combining an all-sky infrared selection with NuSTAR follow-up, new heavily obscured AGN are identified. Obscuration emits infrared radiation, meaning that the infrared-selected AGN catalogue should be representative of the underlying AGN population. The absence of such representative catalogues has continually plagued cosmological studies, and the resultant obscured AGN fraction will be strongly constraining for AGN models.
    Note: Dissertation University of Southampton
    Additional Edition: ISBN 9783030603601
    Additional Edition: ISBN 9783030603625
    Additional Edition: ISBN 9783030603632
    Additional Edition: Erscheint auch als Druck-Ausgabe ISBN 9783030603601
    Additional Edition: Erscheint auch als Druck-Ausgabe ISBN 9783030603625
    Additional Edition: Erscheint auch als Druck-Ausgabe ISBN 9783030603632
    Language: English
    Keywords: Hochschulschrift
    Library Location Call Number Volume/Issue/Year Availability
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