Abstract
The spectrometer SPI is one of the main detectors of ESA’s INTEGRAL mission. The instrument offers two interesting and valuable capabilities for the detection of the prompt emission of Gamma‐ray bursts. Within a field of view of 16 degrees, SPI is able to localize Gamma‐ray bursts with an accuracy of 10 arcmin. The large anticoincidence shield, ACS, consisting of 512 kg of BGO crystals, detects Gamma‐ray bursts quasi omnidirectionally above ∼70keV. Burst alerts from SPI/ACS are distributed to the interested community via the INTEGRAL Burst Alert System. The ACS data have been implemented into the 3rd Interplanetary Network and have proven valuable for the localization of bursts using the triangulation method. During the first 8 months of the mission approximately one Gamma‐ray burst per month was localized within the field of flew of SPI and 145 Gamma‐ray burst candidates were detected by the ACS from which 40 % have been confirmed by other instruments.
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