A search for new γ-ray blazars from infrared selected candidates

dc.contributor.authorMusiimenta, Blessing
dc.contributor.authorArsioli, Bruno Sversut
dc.contributor.authorJurua, Edward
dc.contributor.authorMutabazi, Tom
dc.date.accessioned2022-10-25T12:43:24Z
dc.date.available2022-10-25T12:43:24Z
dc.date.issued2021
dc.description.abstractWe present a systematic study of gamma-ray blazar candidates based on a sample of 40 objects taken from the WIBR catalogue. By using a likelihood analysis, 26 of the 40 sources showed significant gamma-ray signatures 3σ. Using high-energy test statistics (TS) maps, we confirm 8 sources, which are completely new, and show another 15 promising γ-ray candidates. The results from this analysis show that a multi-frequency approach can help to improve the current description of the gamma-ray skyen_US
dc.identifier.citationMusiimenta, B., Arsioli, B. S., Jurua, E., & Mutabazi, T. (2019). A search for new γ-ray blazars from infrared selected candidates. Proceedings of the International Astronomical Union, 15(S356), 329-331.en_US
dc.identifier.urihttp://ir.must.ac.ug/handle/123456789/2581
dc.language.isoen_USen_US
dc.publisherProceedings of the International Astronomical Unionen_US
dc.subjectGalaxiesen_US
dc.subjectActiveen_US
dc.subjectGamma-raysen_US
dc.subjectBlazarsen_US
dc.titleA search for new γ-ray blazars from infrared selected candidatesen_US
dc.typeArticleen_US

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