Abstract
We report the discovery by the Large Area Telescope (LAT) onboard the Fermi Gamma-Ray Space Telescope of high-energy γ-ray (GeV) emission from the flat-spectrum radio quasar PKS 1454-354 (z = 1.424). On 2008 September 4, the source rose to a peak flux of (3.5 0.7) × 10-6 ph cm -2 s-1 (E > 100 MeV) on a timescale of hours and then slowly dropped over the following 2 days. No significant spectral changes occurred during the flare. Fermi/LAT observations also showed that PKS 1454-354 is the most probable counterpart of the unidentified EGRET source 3EG J1500-3509. Multiwavelength measurements performed during the following days (7 September with Swift; 6-7 September with the ground-based optical telescope Automated Telescope for Optical Monitoring; 13 September with the Australia Telescope Compact Array) resulted in radio, optical, UV, and X-ray fluxes greater than archival data, confirming the activity of PKS 1454-354.
Original language | English |
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Pages (from-to) | 934-941 |
Number of pages | 8 |
Journal | Astrophysical Journal |
Volume | 697 |
Issue number | 1 |
DOIs | |
Publication status | Published - 2009 |
Keywords
- Galaxies: active
- Gamma rays: observations
- Quasars: individual (PKS 1454-354)
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science