Fig. 26
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UVW1 light curve and the different image stamps of the transient detected using TUVOpipe at RA = 18:20:21.94, Dec = +07:11:07.3. This source was identified as the known source MAXI J1820+070, a black hole X-ray binary, and was the target of the Swift observations. In Fig. 27, we show the long-term (PV) light curve of this source.
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