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CAMELOT - Concept study and early results for onboard data processing and GPS-based timestamping

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arxiv 1806.03685 v1 pith:3KIFJFAW submitted 2018-06-10 astro-ph.IM astro-ph.HE

András Pál (1 , 2) , László Mészáros (1 , Norbert Tarcai (3) , Norbert Werner (4 , 5 , 6) , Jakub Řípa (4
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classification astro-ph.IMastro-ph.HE
keywords camelotaccuracyearlyresultselectronicsgamma-raylocalizationpayload
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abstract

Due to recent advances in nanosatellite technology, it is now feasible to integrate scintillators with an effective area of hundreds of square-centimeters on a single three-unit cubesat. We present the early test results for the digital payload electronics developed for the proposed CAMELOT (Cubesats Applied for MEasuring and LOcalising Transients) mission. CAMELOT is a fleet of nanosatellites intended to do full-sky monitoring and perform accurate timing-based localization of gamma-ray transients. Here we present the early results on the GPS timestamping capabilities of the CAMELOT payload electronics, concluding that the investigated setup is capable to timestamp the received gamma-ray photons with an accuracy and precision better than 0.02 millisecond, which corresponds to a timing based localization accuracy of $\sim 3.5^{\prime}$. Further refinements will likely allow us to improve the timing accuracy down to the sub-microsecond level.

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  1. Estimation of the detected background by the future gamma-ray transient mission CAMELOT

    astro-ph.HE 2019-09 conditional novelty 4.0 of 10

    At 500 km, one CAMELOT scintillator would see roughly 620 to 1000 background counts per second outside the South Atlantic Anomaly, giving a typical short gamma-ray burst a signal-to-noise ratio of 4.3 to 5.1.

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