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First bounds on the very high energy gamma-ray emission from Arp 220

J. Albert et al.
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Abstract

Using the Major Atmospheric Gamma Imaging Cherenkov Telescope (MAGIC), we have observed the nearest ultra-luminous infrared galaxy Arp 220 for about 15 hours. No significant signal was detected within the dedicated amount of observation time. The first upper limits to the very high energy $γ$-ray flux of Arp 220 are herein reported and compared with theoretical expectations.

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J. Albert et al.. 2006-11-26. First bounds on the very high energy gamma-ray emission from Arp 220. https://doi.org/10.1086/511173

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