Abstract
Observations of a weak cosmic gamma ray burst of integrated intensity 2×10−6 erg cm−2, two solar flare events, and pulsed emission profiles of A0534+26 and NP0532 are reported for several energy intervals in the energy range from 45 to 520 keV. The measurements were made with a NaI(Tl) detector array flown on a balloon to 4 g cm−2 residual atmosphere from Palestine, Texas, on October 6–8, 1980, for 28 hours. The detector is a prototype of the Burst and Transient Source Experiment (BATSE) to be flown on the Gamma‐Ray Observatory (GRO).
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