Abstract
We report on very high energy (>100GeV) gamma-ray observations of Swift J164449.3+573451, an unusual transient object first detected by the Swift Observatory and later detected by multiple radio, optical, and X-ray observatories. A total exposure of 28hr was obtained on Swift J164449.3+573451 with the Very Energetic Radiation Imaging Telescope Array System (VERITAS) during 2011 March 28-April 15. We do not detect the source and place a differential upper limit on the emission at 500GeV during these observations of 1.4 × 10-12ergcm-2s-1 (99% confidence level). We also present time-resolved upper limits and use a flux limit averaged over the X-ray flaring period to constrain various emission scenarios that can accommodate both the radio-through-X-ray emission detected from the source and the lack of detection by VERITAS.
Original language | English (US) |
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Article number | L30 |
Journal | Astrophysical Journal Letters |
Volume | 738 |
Issue number | 2 |
DOIs | |
State | Published - Sep 10 2011 |
Keywords
- accretion, accretion disks
- galaxies: active
- gamma rays: galaxies
- radiation mechanisms: non-thermal