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The new gamma-ray observatory: CTA

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Figure

Figure 1. Example layouts of telescopes on the two sites in the southern hemisphere (top) and northernhemisphere (bottom) with different scales
Figure 3. Point source sensitivity of for an example array layout (solid black line, filled squares)compared to that of its component sub-systems: 3 LSTs (red, open circles), 18 MSTs (green, opensquares), and 56 SSTs (blue, open triangles)
Figure 4. Integral sensitivity for CTA from MC simulations, together with the sensitivities incomparable conditions (50 h for IACTs, 1 year for Fermi-LAT and HAWC) for some gamma-rayobservatories.
Figure 6. Comparison of predicted sensitivities inLarge Magellanic Cloud and the dwarf galaxy Sculptor

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