File:Sensitivietiesgamma17.pdf
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Summary[edit]
| Description |
English: Point source continuum differential sensitivity of X- and
gamma-ray instruments. The curves for INTEGRAL/JEM-X, IBIS (ISGRI and PICsIT), and SPI are for an effective observation time T_obs = 1 Ms. The COMPTEL and EGRET sensitivities are given for the typical observation time accumulated during the 9 years of the CGRO mission. The Fermi/LAT sensitivity is for a high Galactic latitude source in 10 years of observation in survey mode. For MAGIC, HESS/VERITAS, and CTA, the sensitivities are given for T_obs = 50 hours. For HAWC Tobs = 5 yr, for LHAASO T_obs = 1 yr, and for HiSCORE T_obs = 1000 h. The e-ASTROGAM sensitivity is calculated for an effective exposure of 1 year and for a source at high Galactic latitude. |
| Date | |
| Source | Own work |
| Author | Alessandro.de.angelis |
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| current | 19:08, 27 December 2017 |  | 1,235 × 660 (54 KB) | Alessandro.de.angelis (talk | contribs) | User created page with UploadWizard |
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