VERITAS Observations of the Unusual Extragalactic Transient Swift J164449.3+573451
arXiv:1107.1738 · doi:10.1088/2041-8205/738/2/L30
Abstract
We report on very-high-energy (100 GeV) gamma-ray observations of Swift J164449.3+573451, an unusual transient object first detected by the {\it Swift} Observatory and later detected by multiple radio, optical and X-ray observatories. A total exposure of 28 hours was obtained on Swift J164449.3+573451 with VERITAS during 2011 March 28 -- April 15. We do not detect the source and place a differential upper limit on the emission at 500 GeV during these observations of erg cm s (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.
References in corpus (4)
Cited by in corpus (10)
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- Swift J1644+57: an Ideal Test Bed of Radiation Mechanisms in a Relativistic Super-Eddington Jet
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- A Very-High-Energy Gamma-Ray View of the Transient Sky
- Internal shock model for the X-ray flares of Swift J1644+57
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