A survey of HC3N in extragalactic sources - Is HC3N a tracer of activity in ULIRGs?

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Fig. 3

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HC₃N 16-15 spectra for NGC 1056, NGC 1377, and NGC 3079 (non-detections). The absorption-like features in the NGC 1056 spectrum are most likely due to a problem with the backend of the receiver.

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