prikaz prve stranice dokumenta Undetected Active Galactic Nuclei observed by the MAGIC Telescopes
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master's thesis
Undetected Active Galactic Nuclei observed by the MAGIC Telescopes
Rijeka: University of Rijeka, 2017. urn:nbn:hr:194:947393
Tolo, Marlena
University of Rijeka
Faculty of Physics

Cite this document

Tolo, M. (2017). Undetected Active Galactic Nuclei observed by the MAGIC Telescopes (Master's thesis). Rijeka: University of Rijeka. Retrieved from https://urn.nsk.hr/urn:nbn:hr:194:947393

Tolo, Marlena. "Undetected Active Galactic Nuclei observed by the MAGIC Telescopes." Master's thesis, University of Rijeka, 2017. https://urn.nsk.hr/urn:nbn:hr:194:947393

Tolo, Marlena. "Undetected Active Galactic Nuclei observed by the MAGIC Telescopes." Master's thesis, University of Rijeka, 2017. https://urn.nsk.hr/urn:nbn:hr:194:947393

Tolo, M. (2017). 'Undetected Active Galactic Nuclei observed by the MAGIC Telescopes', Master's thesis, University of Rijeka, accessed 26 April 2024, https://urn.nsk.hr/urn:nbn:hr:194:947393

Tolo M. Undetected Active Galactic Nuclei observed by the MAGIC Telescopes [Master's thesis]. Rijeka: University of Rijeka; 2017 [cited 2024 April 26] Available at: https://urn.nsk.hr/urn:nbn:hr:194:947393

M. Tolo, "Undetected Active Galactic Nuclei observed by the MAGIC Telescopes", Master's thesis, University of Rijeka, Rijeka, 2017. Available at: https://urn.nsk.hr/urn:nbn:hr:194:947393

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Metadata
TitleUndetected Active Galactic Nuclei observed by the MAGIC Telescopes
Title (croatian)Nedetektirane aktivne galaktičke jezgre opažane teleskopima MAGIC
AuthorMarlena Tolo
MentorDijana Dominis Prester (mentor)
Committee memberTomislav Terzić (predsjednik povjerenstva)
Committee memberDijana Dominis Prester (član povjerenstva)
Committee memberSaša Mićanović (član povjerenstva)
GranterUniversity of Rijeka
(Faculty of Physics)
Rijeka
Defense date and country2017-09-27, Croatia
Scientific / art field,
discipline and subdiscipline		NATURAL SCIENCES
Physics
Astronomy and Astrophysics
Abstract
Active galactic nuclei are among the most powerful sources of luminosity in the Universe. Observations of these astrophysical objects are important due to dierent physical processes and acceleration of particles that can occur. The main goal of this research is the analysis of active galactic nuclei that have been observed by MAGIC telescopes but not detected. Analysis of MAGIC observations of CTA102 was performed, and confirmed no detection. Based on data observed by MAGIC and Fermi-LAT telescopes, sources of particular interest are selected to be discussed in a detail : 3c454.3 and 4C+55.17, including CTA102. Light curves observed by Fermi-LAT space telescope with corresponding spectral indices are presented for these sources. Observations of CTA102, are used in order to extrapolate Fermi spectrum into VHE range.
Abstract (croatian)
Aktivne galaktičke jezgre pripadaju najmoćnijim izvorima svjetlosti u Svemiru. Opažanja ovih astrofizičkih objekata važna su zbog ubrzanja čestica i različitih fizičkih procesa koji se mogu dogoditi. Glavni cilj ovog rada je analiza nedetektiranih aktivnih galaktičkih jezgri koje su opažane MAGIC teleskopima. Za CTA102 analiza MAGIC opažanja potvrdila je nedetekciju. Na temelju opažanja MAGIC i Fermi-LAT teleskopa, detaljno su opisani posebno značajni izvori: 3c454.3 i 4C+55.17, uključujući i CTA102. Svjetlosne krivulje i pripadne spektralne indekse ovih izvora dobili smo pomoću opažanja Fermi- LAT teleskopa. Za ekstrapolaciju spektra u VHE područje korišteni su podaci dobiveni opažanjem izvora CTA102.
Keywords
Keywords (croatian)
Languageenglish
URN:NBNurn:nbn:hr:194:947393
Study programmeTitle: physics
Study programme type: university
Study level: graduate
Academic / professional title: magistar/magistra fizike (magistar/magistra fizike)
Type of resourceText
File originBorn digital
Access conditionsAccess restricted to students and staff of home institution
Terms of useLicence In copyright icon
RepositoryRepository of the University of Rijeka, Faculty of Physics
Created on2017-10-26 09:15:21

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