Determination of K4000 of potential blazar candidates among EGRET unidentified gamma-ray sources

Blazars are radio-loud Active Galactic Nuclei (AGN) with relativistic jets oriented towards the observer's line-of-sight. Based on their optical spectra, blazars may be classified as flat-spectrum radio quasars (FSRQs) or BL Lacs. FSRQs are more luminous blazars with both narrow and broad emiss...

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Veröffentlicht in:arXiv.org 2020-04
Hauptverfasser: Uwitonze, Emmanuel, Nkundabakura, Pheneas, Mutabazi, Tom
Format: Artikel
Sprache:eng
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Zusammenfassung:Blazars are radio-loud Active Galactic Nuclei (AGN) with relativistic jets oriented towards the observer's line-of-sight. Based on their optical spectra, blazars may be classified as flat-spectrum radio quasars (FSRQs) or BL Lacs. FSRQs are more luminous blazars with both narrow and broad emission and absorption lines, while BL Lacs are less luminous and featureless. Recent studies show that blazars dominate (93%) the already-identified EGRET sources (142), suggesting that among the unidentified sources (129) there could still be faint blazars. Due to the presence of a strong non-thermal component inside their jets, blazars are found to display a weaker depression at 4000 Å (K4000
ISSN:2331-8422
DOI:10.48550/arxiv.2004.03154