TeV-scale gravity at the LHC, and the way forward in an era lacking significant excesses

Here, the numerical data described in Fig. 4 of the paper "Kerr black holes with synchronised hair: an analytic model and dynamical formation", arXiv:1706.06597, together with an explanatory pdf file and two Mathematica notebooks, is made available for public use.
The data consists of four solutions of Kerr black holes with scalar hair and six solutions of Kerr black holes with Proca hair. These families of solutions were first presented in the papers:
Abstract: We study wormhole solutions obtained via applying dualities and complexifications to the vacuum Weyl metrics generated by massive rods and by point masses. The most interesting finding are wormholes with locally flat geometry supported by rings of negative energy.
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Gr@v members Pedro Cunha and Carlos Herdeiro at the LIGO LIvingston Control Room, in the state of Louisiana, USA, during a visit to the site. More exciting news should be announced in the summer by the collaboration!
Read the CQG+ viewpoint article on "Can Astrophysical Black Holes have hair", by Gr@v members C. Herdeiro and E. Radu, on the recently published Classical and Quantum Gravity Focus issue wherein they were guest editors.
Gr@v members P. Cunha and C. Herdeiro were amongst the participants of the StronGBaD workshop, at the University of Mississippi, USA.