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by Giovanni Ceribella
| Institution: | Università degli Studi di Padova |
|---|---|
| Department: | |
| Degree: | |
| Year: | 2022 |
| Keywords: | MAGIC, Blazar, EBL, BL-Lac, Redshift, Cherenkov, Gamma Astronomy; Settore FIS/01 - Fisica Sperimentale; Settore FIS/05 - Astronomia e Astrofisica |
| Posted: | 3/25/2025 |
| Record ID: | 2231772 |
| Full text PDF: | http://hdl.handle.net/20.500.12608/28167 |
Attraverso il confronto tra gli indici spettrali nei domini HE e VHE dello spettro del blazar PKS 1424+240 si determina un limite superiore al redshift dello stesso. Tale valore risulta essere compatibile con le piu' recenti misure sperimentali, suggerendo che PKS 1424+240 appartenga ad una nuova classe di blazar con emissione ad energie estremamente alte. open
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