Image Details
Caption: Figure 6.
Weekly light curves from the direction of the pulsar binary system PSR B1259−63/LS 2883 (2FAV J1302−63.7). The top panels show the relative variation of counts, ﹩{\rm{\Delta }}{N}_{\mathrm{rel}}=(N-{N}^{\exp })/{N}^{\exp },﹩ where N is the number of observed counts in a given time bin and Nexp is the number of expected counts. The bottom panels show the significance that corresponds to these counts variations. Plots on the left refer to low-energy analysis, while the ones on the right refer to high-energy analysis.
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