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OBSERVATIONS OF MICROQUASAR CANDIDATES WITH THE MAGIC TELESCOPE

机译:带有望远镜的微季候候选者的观测

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摘要

We report on the results from the observations in very high energy band (VHE, E-gamma >= 100 GeV) of the gamma-ray binary LS I +61 303 and the black hole X-ray binary (BHXB) Cygnus X-1. LS I +61 303 was recently discovered at VHE by MAGIC(1) and here we present the preliminary results from an extensive observation campaign, comprising 112 observation hours covering 4 orbital cycles, aiming at determining the time-dependent features of the VHE emission. Cygnus X-1 was observed for a total of 40 hours during 26 nights, spanning the period between June and November 2006. We report on the results of the searches for steady and variable gamma-ray signals from Cygnus X-1, including the first experimental evidence for an intense flare, of duration between 1.5 and 24 hours.
机译:我们报告了在非常高的能带(VHE,E-γ> = 100 GeV)中观察到的结果,这些结果是伽玛射线二进制LS I +61 303和黑洞X射线二进制(BHXB)天鹅座X-1 。 MAGIC(1)最近在VHE上发现了LS I +61 303,在这里,我们介绍了一项广泛的观测活动的初步结果,该活动包括112个观测小时,涵盖4个轨道周期,旨在确定VHE发射的时变特征。在2006年6月至2006年11月之间的26个夜晚中,共观测了Cygnus X-1 40个小时。我们报告了从Cygnus X-1中搜索稳定且可变的伽马射线信号的结果,包括第一个实验证明强烈耀斑,持续时间在1.5到24小时之间。

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