Comparison of Fermi-LAT and CTA in the region between 10-100 GeV

作者: Stefan Funk , JA Hinton , CTA Consortium

DOI: 10.1016/J.ASTROPARTPHYS.2012.05.018

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摘要: Abstract The past decade has seen a dramatic improvement in the quality of data available at both high (HE: 100 MeV to 100 GeV) and very (VHE: 100 GeV 100 TeV) gamma-ray energies. With three years from Fermi Large Area Telescope (LAT) deep pointed observations with arrays Cherenkov telescope, continuous spectral coverage ∼10 TeV exists for first time brightest sources. Fermi-LAT is likely continue several years, resulting significant improvements energy sensitivity. On same timescale, Array (CTA) will be constructed providing unprecedented VHE capabilities. optimisation CTA must take into account competition complementarity Fermi, particularly overlapping range 10–100 GeV. Here we compare performance current baseline design steady transient, point-like extended

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