BurstCube Image: Science

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Simulation of combining BurstCube and LIGO locationizations of a gravitational wave and burst event (such as binary black hole merger such as GW151226)


The integrated relative exposure of BurstCube over a single orbit shown in celestial coordinates (Mollweide projection).


BurstCube localizes short gamma-ray burst sources (sGRB) to an accuracy of ∼7° when viewed by three or more detectors. The localization errors (in degrees radius) are shown here across the entire BurstCube field of view (in Az/El coordinates). There is some attenuation of signals seen through the spacecraft bus, and complete occulation of sources by the Earth.

Graph of effective area of BurstCube detectors versus energy
Detector simulation of the effective area of the BurstCube detectors as a function of energy (shown at 15 degree incidence), including comparison to the Gamma ray Burst Monitor (GBM) instrument on the Fermi satellite. The effective area is ∼70% of the larger GBM NaI detectors at 100 keV.


Total sky coverage in search for Gamma Ray Burst sources, with Swift Burst Alert Telescope (BAT), Fermi Gamma ray Burst Monitor (GBM), and combination with BurstCube.

Other BurstCube Images

Other Image Resources Online

CubeSats (NASA Scientific Visualization Studio)