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(Presentations)
(Presentations)
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== Presentations ==
 
== Presentations ==
  
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* [https://fermi.gsfc.nasa.gov/science/mtgs/symposia/2018/program/thu/Jakub_Ripa.pdf Jakub Řípa - Future mission CAMELOT for localisation of gamma-ray transients by fleet of cubesats]
 
* [https://www.grbnanosats.net/mediawiki/images/2/24/2.7_BudapestConfWerner.pdf Norbert Werner - CAMELOT: Cubesats Applied for MEasuring and LOcalising Transients]
 
* [https://www.grbnanosats.net/mediawiki/images/2/24/2.7_BudapestConfWerner.pdf Norbert Werner - CAMELOT: Cubesats Applied for MEasuring and LOcalising Transients]
 
* [https://www.grbnanosats.net/mediawiki/images/f/f2/1.4_-_Localization_-_Ohno.pdf Masanori Ohno - GRB localization by timing in LEO]
 
* [https://www.grbnanosats.net/mediawiki/images/f/f2/1.4_-_Localization_-_Ohno.pdf Masanori Ohno - GRB localization by timing in LEO]

Revision as of 14:08, 28 November 2018

CAMELOT

This page describes Cubesats Applied for MEasuring and LOcalising Transients (CAMELOT) and provides more information including publications, presentations, etc.

CAMELOT will be a constellation of at least nine 3U CubeSats (10 cm x 10 cm x 30 cm) each composed of 4 CsI(Tl) scintillator detectors read out by silicon Multi-Pixel Photon Counters (MPPC). CAMELOT will automatically detect gamma-ray transients onboard (GRBs, SGRs, Solar flares, TGFs, etc.), sending alerts to the ground to allow rapid calculation of the localization of the source via triangulation at LEO and to allow quick follow-up observations. CAMELOT is currently in the phase of feasibility study and the detectors are being developed and tested.

Publications

Presentations