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I analysis results obtained from the Std and Loose cut configurations. The number of events in the ON and OFF regions n ON , n OFF , the number of excess events n excess , significance S LiMa , signal to background ratio (S/B) and the rate of gammas for each cut configuration are given, 98 List of Figures ,
Fluxes are calculated in 1-day bins for VERITAS (red squares) The red dashed line shows the yearly averaged TeV flux in 2011 (8.0 × 10 ?12 cm ?2 s ?1 ) [121]. The Fermi-LAT fluxes are calculated with 1-day integration bins (blue crosses), in the energy range 100 MeV < E < 500 GeV. The blue dashed line correspond to the average flux from the 3FGL catalog [44]. For the Fermi-LAT data, down-pointing triangles indicate 95 % c.l. upper limits for time bins with signal smaller than 2?, p.74, 2013. ,
The Crab pulsar as seen from Chandra X-ray Observatory. (b) Composite image of the Crab Nebula from five telescopes: the Karl G Jansky Very Large Array, the Spitzer Space Telescope, the Hubble Space Telescope, the XMM-Newton Observatory, and the Chandra X-ray Observatory, Image, vol.3, p.94 ,
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red squares) The integral fluxes, calculated above 1 TeV are normalized to the average flux from the H. E. S. S. flux from 2006 publication [113]. The dashed red line correspond to the average flux for this period, whereas the black line to the average flux from In the bottom part of the plot, the Crab Nebula integral flux of the synchrotron component between 57632-57692 MJD as derived from Fermi-LAT data is plotted (blue crosses). The integral fluxes are calculated in 3-day time bins, from 100 MeV < E < 500 GeV and normalized to the published average synchrotron flux from, p.130, 2006. ,
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