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A compact instrument for gamma-ray burst detection on a CubeSat platform I: Design drivers and expected performance.
Murphy, David; Ulyanov, Alexey; McBreen, Sheila; Doyle, Maeve; Dunwoody, Rachel; Mangan, Joseph; Thompson, Joseph; Shortt, Brian; Martin-Carrillo, Antonio; Hanlon, Lorraine.
Afiliação
  • Murphy D; School of Physics and Centre for Space Research, University College Dublin, Dublin 4, Ireland.
  • Ulyanov A; School of Physics and Centre for Space Research, University College Dublin, Dublin 4, Ireland.
  • McBreen S; School of Physics and Centre for Space Research, University College Dublin, Dublin 4, Ireland.
  • Doyle M; School of Physics and Centre for Space Research, University College Dublin, Dublin 4, Ireland.
  • Dunwoody R; School of Physics and Centre for Space Research, University College Dublin, Dublin 4, Ireland.
  • Mangan J; School of Physics and Centre for Space Research, University College Dublin, Dublin 4, Ireland.
  • Thompson J; School of Mechanical and Materials Engineering and Centre for Space Research, University College Dublin, Dublin 4, Ireland.
  • Shortt B; European Space Agency, ESTEC, 2200 AG Noordwijk, The Netherlands.
  • Martin-Carrillo A; School of Physics and Centre for Space Research, University College Dublin, Dublin 4, Ireland.
  • Hanlon L; School of Physics and Centre for Space Research, University College Dublin, Dublin 4, Ireland.
Exp Astron (Dordr) ; 52(1-2): 59-84, 2021.
Article em En | MEDLINE | ID: mdl-34744308
ABSTRACT
The Educational Irish Research Satellite 1 (EIRSAT-1) is a 2U CubeSat being developed under ESA's Fly Your Satellite! programme. The project has many aspects, which are primarily educational, but also include space qualification of new detector technologies for gamma-ray astronomy and the detection of gamma-ray bursts (GRBs). The Gamma-ray Module (GMOD), the main mission payload, is a small gamma-ray spectrometer comprising a 25 mm × 25 mm × 40 mm cerium bromide scintillator coupled to an array of 16 silicon photomultipliers. The readout is provided by IDE3380 (SIPHRA), a low-power and radiation tolerant readout ASIC. GMOD will detect gamma-rays and measure their energies in a range from tens of keV to a few MeV. Monte Carlo simulations were performed using the Medium Energy Gamma-ray Astronomy Library to evaluate GMOD's capability for the detection of GRBs in low Earth orbit. The simulations used a detailed mass model of the full spacecraft derived from a very high-fidelity 3D CAD model. The sky-average effective area of GMOD on board EIRSAT-1 was found to be 10 cm2 at 120 keV. The instrument is expected to detect between 11 and 14 GRBs, at a significance greater than 10σ (and up to 32 at 5σ), during a nominal one-year mission. The shape of the scintillator in GMOD results in omni-directional sensitivity which allows for a nearly all-sky field of view.
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Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Tipo de estudo: Diagnostic_studies Idioma: En Revista: Exp Astron (Dordr) Ano de publicação: 2021 Tipo de documento: Article

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Tipo de estudo: Diagnostic_studies Idioma: En Revista: Exp Astron (Dordr) Ano de publicação: 2021 Tipo de documento: Article