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We analyse the Rossi X‐ray Timing Explorer (RXTE) and Swift observations of the 2009 outburst from a newly discovered transient and black hole candidate XTE J1652−453. The behaviour of the source was observed by RXTE to be a sequence of spectral states that are typical of black‐hole X‐ray binaries. During the first seven observations, it is determined that the source remains in a high/soft state....
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