When using this data, please cite the original publication:
CMS
Collaboration
(2018).
Search for new physics in dijet angular distributions using proton-proton collisions at $\sqrt{s}=$ 13 TeV and constraints on dark matter and other models. Eur.Phys.J.C 78 (2018) 789.
https://doi.org/10.1140/epjc/s10052-018-6242-x
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INSPIRE Record
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Additionally, you should cite the
record:
CMS
Collaboration
(2018).
Search for new physics in dijet angular distributions using proton-proton collisions at $\sqrt{s}=$ 13 TeV and constraints on dark matter and other models. HEPData (collection).
https://doi.org/10.17182/hepdata.82308
or, if you prefer, a specific version of the
record:
CMS
Collaboration
(2018).
Search for new physics in dijet angular distributions using proton-proton collisions at $\sqrt{s}=$ 13 TeV and constraints on dark matter and other models (Version 1). HEPData (collection).
https://doi.org/10.17182/hepdata.82308.v1
You can also cite this table directly.
CMS
Collaboration
(2018).
“Table 13” of “Search for new physics in dijet angular distributions using proton-proton collisions at $\sqrt{s}=$ 13 TeV and constraints on dark matter and other models” (Version 1). HEPData (dataset).
https://doi.org/10.17182/hepdata.82308.v1/t13