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MAGIC and Multi-Wavelength Observations of Mrk 180 and 1ES 2344+514 in 2008

机译:2008年MRK 180和1ES 2344 + 514的Magr和多波长观测

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Simultaneous multi-wavelength (MW) campaigns are the most promising approaches to investigate the still unrevealed nature of blazars, active galactic nuclei which are variable on all time scales from radio to TeV energies. In 2008, two MW campaigns on the high-frequency peaked blazars Mrk 180 and 1ES 2344+514 have been organised by the MAGIC collaboration. From radio to TeV gamma rays, RATAN-600, Mets¨ahovi, Effelsberg, VLBA (only 1ES 2344+514), IRAM, KVA, Swif t, AGILE, Fermi-LAT and MAGIC-I were taking part in these campaigns. Mrk 180 had just been discovered at TeV energies by MAGIC in 2006, whereas 1ES 2344+514 is a known TeV emitter since many years. Due to their rather faint emission particularly at TeV energies, the campaigns represented quite challenging observations. In fact, Mrk 180 has not been investigated until now in MW campaigns, and for 1ES 2344+514 only one campaign including TeV measurements has been reported in literature up to now. In this contribution, we will present detailed MW light curves for both sources and describe the composite wide range spectral energy distributions by theoretical models.
机译:同时多波长(MW)运动是调查Blazars仍然未虚弱的性质,活跃的半乳核的最有希望的方法,这些方法在从无线电到TEV Energies的所有时间尺度上都是可变的。 2008年,通过魔法协作组织了高频峰值布拉齐尔MRK 180和1ES 2344 + 514上的两个MW竞选活动。从Radio到Tev Gamma Rays,Ratan-600,Metsbovi,Effelsberg,VLBA(只有1ES 2344 + 514),Iram,KVA,SWIF T,Agile,Fermi-Lat和Magic-I正在参加这些竞选活动。 MRK 180刚刚在2006年通过魔术发现了TEV Energies,而1ES 2344 + 514是一个已知的Tev发射器,自多年以来。由于他们尤其是TEV Energies特别淡淡的发射,该活动代表了相当具有挑战性的观察。事实上,迄今为止尚未调查MRK 180,并且对于1ES 2344 + 514只有一个包括TEV测量的一个广告系列,目前已经报告。在这一贡献中,我们将为两个来源提供详细的MW光曲线,并通过理论模型描述复合宽范围谱能量分布。

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