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Publication details

Constraints on the Steady and Pulsed Very High Energy Gamma-Ray Emission from Observations of PSR B1951+ 32/CTB 80 with the MAGIC Telescope

MAGIC collaboration, Albert et al.

First author:
J.Albert

Journal

The Astrophysical Journal 669, 1143, 2007

ticlealbert2007constraints, title=Constraints on the Steady and Pulsed Very High Energy Gamma-Ray Emission from Observations of PSR B1951+ 32/CTB 80 with the MAGIC Telescope, author=Albert, J and Aliu, E and Anderhub, H and Antoranz, P and Armada, A and B

Abstract:

We report on very high energy gamma-observations with the MAGIC Telescope of the pulsar PSR B1951+32 and its associated nebula, CTB 80. Our data constrain the cutoff energy of the pulsar to be less than 32 GeV, assuming the pulsed gamma-ray emission to be exponentially cut off. The upper limit on the flux of pulsed gamma-ray emission above 75 GeV is 4.3*10^-11 photons cm^-2 sec^-1, and the upper limit on the flux of steady emission above 140 GeV is 1.5*10^-11 photons cm^-2 sec^-1. We discuss our results in the framework of recent model predictions and other studies.