BurstCube: A CubeSat for Gravitational Wave Counterparts

Abstract

BurstCube will detect long GRBs, attributed to the collapse of massive stars, short GRBs (sGRBs), resulting from binary neutron star mergers, as well as other gamma-ray transients in the energy range 10-1000 keV. sGRBs are of particular interest because they are predicted to be the counterparts of gravitational wave (GW) sources soon to be detectable by LIGO/Virgo. BurstCube contains 4 CsI scintillators coupled with arrays of compact low-power Silicon photomultipliers (SiPMs) on a 6U Dellingr bus, a flagship modular platform that is easily modifiable for a variety of 6U CubeSat architectures. BurstCube will complement existing facilities such as Swift and Fermi in the short term, and provide a means for GRB detection, localization, and characterization in the interim time before the next generation future gamma-ray mission flies, as well as space-qualify SiPMs and test technologies for future use on larger gamma-ray missions. The ultimate configuration of BurstCube is to have a set of $\sim 10$ BurstCubes to provide all-sky coverage to GRBs for substantially lower cost than a full-scale mission.

arXiv commentIn the 35th International Cosmic Ray Conference, Busan, Korea

References in corpus (12)

• Observation of Gravitational Waves from a Binary Black Hole Merger
• GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence
• GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2
• Electromagnetic Counterparts of Compact Object Mergers Powered by the Radioactive Decay of R-process Nuclei
• The Rate of Binary Black Hole Mergers Inferred from Advanced LIGO Observations Surrounding GW150914
• Fermi GBM Observations of LIGO Gravitational Wave event GW150914
• The 2nd Fermi GBM Gamma-Ray Burst Catalog: The First Four Years
• Demonstrating the feasibility of probing the neutron star equation of state with second-generation gravitational wave detectors
• Electromagnetic Counterparts to Black Hole Mergers Detected by LIGO
• The Swift short gamma-ray burst rate density: implications for binary neutron star merger rates
• The BATSE-Swift luminosity and redshift distributions of short-duration GRBs
• Using ISS Telescopes for Electromagnetic Follow-up of Gravitational Wave Detections of NS-NS and NS-BH Mergers

Cited by in corpus (3)

• On the Verge of an Astronomy CubeSat Revolution
• Compact CubeSat Gamma-Ray Detector for GRID Mission
• Constraining short gamma-ray burst jet properties with gravitational waves and gamma rays