Observational survey reveals diverse point source detections across celestial bodies, highlighting extensive high-energy emission over seven years of Swift X-ray monitoring.
Context. The Swift satellite is a multi-wavelength observatory specifically designed for gamma-ray burst (GRB) astronomy that is operational since 2004. Swift is also a very flexible multi-purpose facility that supports a wide range of scientific fields such as active galactic nuclei, supernovae, cataclysmic variables, Galactic transients, active stars and comets. The Swift X-ray Telescope (XRT) has collected more than 150 Ms of observations in its first seven years of operations.
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D’Elia et al. (2012) studied this question.
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