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Träfflista för sökning "WFRF:(Bouchet F.) srt2:(2010-2014)"

Sökning: WFRF:(Bouchet F.) > (2010-2014)

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1.
  • Acharya, B. S., et al. (författare)
  • Introducing the CTA concept
  • 2013
  • Ingår i: Astroparticle physics. - : Elsevier BV. - 0927-6505 .- 1873-2852. ; 43, s. 3-18
  • Tidskriftsartikel (övrigt vetenskapligt/konstnärligt)abstract
    • The Cherenkov Telescope Array (CTA) is a new observatory for very high-energy (VHE) gamma rays. CTA has ambitions science goals, for which it is necessary to achieve full-sky coverage, to improve the sensitivity by about an order of magnitude, to span about four decades of energy, from a few tens of GeV to above 100 TeV with enhanced angular and energy resolutions over existing VHE gamma-ray observatories. An international collaboration has formed with more than 1000 members from 27 countries in Europe, Asia, Africa and North and South America. In 2010 the CTA Consortium completed a Design Study and started a three-year Preparatory Phase which leads to production readiness of CTA in 2014. In this paper we introduce the science goals and the concept of CTA, and provide an overview of the project. (C) 2013 Elsevier B.V. All rights reserved.
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2.
  • Bouchet, L., et al. (författare)
  • Tools for analyzing large data-set and handling intensity variations of sources with INTEGRAL/SPI
  • 2014
  • Ingår i: Proceedings of Science. - : Sissa Medialab Srl.
  • Konferensbidrag (refereegranskat)abstract
    • The INTEGRAL/SPI X/gamma-ray spectrometer (20 keV-8 MeV) is an instrument for which it is essential to process many exposures at the same time to increase the low signal-to-noise ratio of the weakest sources and/or low-surface brightness extended emission. The processing of several years of data simultaneously (10 years actually) with traditional methods of data reduction is ineffective and sometimes not possible at all. Thanks to the newly developed tools, processing large data-sets from SPI is possible with both a reasonable turnaround time and low memory usage. We present also techniques that we have developed to overcome difficulties related to the intensity variation of sources/background between sources between consecutive exposures.
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  • Resultat 1-3 av 3

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