Redshift determination of the BL Lac object 3C 66A by the detection of its host galaxy cluster at z = 0.340
The BL Lac object 3C 66A is one of the most luminous extragalactic sources at TeV γ -rays (very high energy, i.e. E > 100 GeV). Since TeVγ -ray radiation is absorbed by the extragalactic background light (EBL), it is crucial to knowthe redshift of the source in order to reconstruct its original s...
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| Autores principales: | Torres Zafra, Juanita, Cellone, Sergio Aldo, Buzzoni, Alberto, Andruchow, Ileana, Portilla Barbosa, José Gregorio |
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| Formato: | Articulo Preprint |
| Lenguaje: | Inglés |
| Publicado: |
2018
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/93902 https://academic.oup.com/mnras/article-abstract/474/3/3162/4349751 https://ri.conicet.gov.ar/handle/11336/87892 |
| Aporte de: |
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