Speaker
Gregory Richards
(Georgia Institute of Technology)
Description
In recent years, the Fermi-LAT gamma-ray telescope has detected a population of over 160 gamma-ray pulsars, which has enabled the detailed study of gamma-ray emission from pulsars at energies above 100 MeV. Further, since the surprising detection of the Crab pulsar in very high-energy (VHE; E > 100 GeV) gamma rays by the MAGIC and VERITAS collaborations, there has been an ongoing effort in the gamma-ray astrophysics community to detect new pulsars in the VHE band. However, the Crab remains the only pulsar so far detected in VHE gamma rays, raising the question of whether or not the Crab is unique and also making it more difficult to constrain model predictions that attempt to explain the VHE emission. Presented here are recent VERITAS results from observational campaigns on the brightest northern-hemisphere high-energy gamma-ray pulsar Geminga and the missing link binary pulsar PSR J1023+0038, which have both resulted in upper limits on a possible gamma-ray flux. These limits are placed into context with the current theoretical framework attempting to explain the origin of VHE gamma-ray emission from pulsars. Additionally, future plans for pulsar observations with VERITAS will be briefly discussed.
| Registration number following "ICRC2015-I/" | 918 |
|---|---|
| Collaboration | VERITAS |
Primary author
Gregory Richards
(Georgia Institute of Technology)
