arXiv (All)
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Detection of kilosecond hard lags in the new pulsating ULX candidate NGC 7456 ULX-1
Context. Ultraluminous X-ray sources (ULXs) are thought to be powered, in many cases, by super-Eddington accretion onto compact objects. While soft X-ray lags have been detected in several ULXs, hard lags remain rare and poorly understood. Aims. We investigate the temporal and energy dependence of X
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