The full JWP reports were published on 21 January 2016. The JWP recognised the discovery of element 113, assigning priority to Riken. They noted that while the individual decay energies of each nuclide in the decay chain of 278113 were inconsistent, their sum was now confirmed to be consistent, strongly suggesting that the initial and final states in 278113 and its daughter 262Db were the same for all three events. The decay of 262Db to 258Lr and 254Md was previously known, firmly anchoring the decay chain of 278113 to known regions of the chart of nuclides. The JWP considered that the JINR–LLNL collaborations of 2004 and 2007, producing element 113 as the daughter of element 115, did not meet the discovery criteria as they had not convincingly determined the atomic numbers of their nuclides through cross-bombardments, which were considered necessary since their decay chains were not anchored to previously known nuclides. They also considered that the previous JWP's concerns over their chemical identification of the dubnium daughter had not been adequately addressed. The JWP recognised the JINR–LLNL–ORNL–Vanderbilt collaboration of 2010 as having discovered elements 117 and 115, and accepted that element 113 had been produced as their daughter, but did not give this work shared credit.
The full JWP reports were published on 21 January 2016 The JWP recognised the discovery of element 113 assigning priority to Riken They noted that while the individual decay energies of each nuclide in the decay chain of 278113 were inconsistent their sum was now confirmed to be consistent strongly suggesting that the initial and final states in 278113 and its daughter 262Db were the same for all three events The decay of 262Db to 258Lr and 254Md was previously known firmly anchoring the decay chain of 278113 to known regions of the chart of nuclides The JWP considered that the JINR–LLNL collaborations of 2004 and 2007 producing element 113 as the daughter of element 115 did not meet the discovery criteria as they had not convincingly determined the atomic numbers of their nuclides through cross-bombardments which were considered necessary since their decay chains were not anchored to previously known nuclides They also considered that the previous JWP's concerns over their chemical identification of the dubnium daughter had not been adequately addressed The JWP recognised the JINR–LLNL–ORNL–Vanderbilt collaboration of 2010 as having discovered elements 117 and 115 and accepted that element 113 had been produced as their daughter but did not give this work shared credit