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The compact jets of the black hole X-ray binary Swift J1753.5-0127 during its 2023-2024 outburst
X-ray binaries are excellent laboratories to study the coupling between accretion and ejection phenomena around compact objects through multiwavelength observations. Swift J1753.5-0127 is a black hole low-mass X-ray binary discovered in outburst in 2005 that remained active for 11 years, followed by
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