activity
19972004
most citedSPI observations of positron annihilation radiation from the 4th galactic quadrant: sky distribution

5 citations · 6 across the 3 of their papers we have counts for

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astro-ph2004

SPI observations of positron annihilation radiation from the 4th galactic quadrant: Spectroscopy

V. Lonjou, G. Weidenspointner, J. Knodlseder +13

The status of the analysis of the electron/positron annihilation radiation performed by INTEGRAL/SPI in the 4th GALACTIC QUADRANT is reported. We use data from the first two Galact…

astro-ph20045 cited

SPI observations of positron annihilation radiation from the 4th galactic quadrant: sky distribution

G. Weidenspointner, V. Lonjou, J. Knoedlseder +14

During its first year in orbit the INTEGRAL observatory performed deep exposures of the Galactic Center region and scanning observations of the Galactic plane. We report on the sta…

astro-ph20041 cited

MGGPOD: a Monte Carlo Suite for Gamma-Ray Astronomy

G. Weidenspointner, M. Harris, C. Ferguson +3

We have developed MGGPOD, a user-friendly suite of Monte Carlo codes built around the widely used GEANT (Version 3.21) package. The MGGPOD Monte Carlo suite and documentation are p…

astro-ph2001

Limits from CGRO/EGRET Data on the Use of Antimatter as a Power Source by Extraterrestrial Civilizations

Michael J. Harris

I argue that the existence of cold antimatter in bulk is not permitted by the Standard Model, so that if a gamma-ray signature from antiproton annihilation were to be detected, it…

astro-ph2001

Transient Gamma Ray Spectrometer Measurements of Gamma-Ray Lines from Novae. III. The 478 keV Line from 7Be Decay

M. J. Harris, B. J. Teegarden, G. Weidenspointner +4

The "Wind" spacecraft carrying the Transient Gamma Spectrometer (TGRS) moves in an extremely elliptical orbit that largely avoids Earth's trapped radiation belts and albedo gamma-r…

astro-ph1997

Astrophysical Effects of nu+gamma-->nu+gamma+gamma and Its Crossed Processes

Michael Harris, Jian Wang, Vigdor L. Teplitz

Recently, Dicus and Repko computed nu gamma --> nu gamma gamma for energies below the threshold for e^{+}e^{-} pair production. They found across section on the order of 10^{-52} o…