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The radio and X-ray light increased to a peak 150 days after the merger, [33] [34] diminishing afterwards. [35] Astronomers have monitored the optical afterglow of GW170817 using the Hubble Space Telescope. [36] [37] In March 2020, continued X-ray emission at 5-sigma was observed by the Chandra Observatory 940 days after the merger. [38]
This list contains a list of EC numbers for the third group, EC 3, hydrolases, placed in numerical order as determined by the Nomenclature Committee of the International Union of Biochemistry and Molecular Biology.