General physical properties of bright Fermi blazars
G. GhiselliniINAF – Osservatorio Astronomico di Brera, Via Bianchi 46, I-23807 Merate, ItalyF. TavecchioINAF – Osservatorio Astronomico di Brera, Via Bianchi 46, I-23807 Merate, ItalyL. FoschiniINAF – Osservatorio Astronomico di Brera, Via Bianchi 46, I-23807 Merate, ItalyG. GhirlandaINAF – Osservatorio Astronomico di Brera, Via Bianchi 46, I-23807 Merate, ItalyL. MaraschiINAF – Osservatorio Astronomico di Brera, Via Brera 28, I–20100 Milano, ItalyA. CelottiSISSA, V. Beirut 2–4, I‐34014 Trieste, Italy
2009en
ABI
Аннотация
The Large Area Telescope (LAT) onboard the Fermi Satellite, in the first months of operation succeeded to double the number of know γ–ray emitting blazars (Abdo et al. 2009a, hereafter A09). Excluding radio–galaxies, in the list of the LAT 3–months survey
Ҳали таржима қилинмаган
Идентификаторлар
Иқтибослар ва манбалар
3 та иқтибос0 та фойдаланилган манба