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Swift J1753.5โ0127: The Black Hole Candidate with the Shortest Orbital Period
We present time-resolved photometry of the optical counterpart to the black hole candidate Swift J1753.5โ0127 which has remained in the low/hard X-ray state and bright at optical/IR wavelengths since its discovery in 2005. At the time of our observations Swift J1753.5โ0127 does not show a decay trend but remains stable โฆ