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Gamma-ray view of the sky before and during the GRB 130427A event

Record-Setting 'Shockingly Bright' Burst

A record-setting blast of gamma rays from a dying star in a distant galaxy has wowed astronomers around the world.

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GRB 111209A exploded on Dec. 9, 2011. The blast produced high energy emission for an astonishing seven hours.

Dying Supergiant Stars Implicated in Hours-long ...

Three unusually long-lasting stellar explosions discovered by NASA's Swift satellite represent a new class of gamma-ray bursts that likely arise from ...

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Swift Features

Mission Overview

    Swift is a first-of-its-kind multi-wavelength observatory dedicated to the study of gamma-ray burst (GRB) science. Its three instruments will work together to observe GRBs and afterglows in the gamma ray, X-ray, ultraviolet, and optical wavebands. The main mission objectives for Swift are to:

    • Determine the origin of gamma-ray bursts
    • Classify gamma-ray bursts and search for new types
    • Determine how the blastwave evolves and interacts with the surroundings
    • Use gamma-ray bursts to study the early universe
    • Perform the first sensitive hard X-ray survey of the sky

Mission News

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