Abstract
During a balloon flight of the High Energy Astronomical Telescope on 1995 July 29, a region of the sky of 25 width around the Seyfert galaxy MCG 8-11-11 was studied over the photon energy range 20-300 keV. An excess at the 9 σ level—well described by a power-law photon spectrum with a slope of α = 2.1 ± 1.2, plus a Gaussian line centered at 112 ± 6 keV having a flux of (9.0 ± 3.4) × 10-4 photons cm-2 s-1 and a FWHM of 32 ± 6 keV—was detected in the energy range 20-160 keV. A contemporary detection of a strong γ-ray flux in the veto system of the telescope suggests that the observed spectral feature may be the result of double-Compton backscattering of a 511 keV line source incident on an external cloud. If associated with the Seyfert galaxy MCG 8-11-11, the present measurement would provide the first evidence for electron-positron pair annihilation flux emission from an active galactic nucleus. An observation of the Crab Nebula as an in-flight calibration source of the telescope is also decribed.
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