Published January 10, 2021 | Version v1
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Supplementary Material for Global fits of axion-like particles to XENON1T and astrophysical data

  • 1. Monash University, Nanjing Normal University
  • 2. Monash University
  • 3. Université catholique de Louvain
  • 4. Imperial College London
  • 5. Nanjing Normal University
  • 6. Georg-August-Universität Göttingen
  • 7. RWTH Aachen
  • 8. Rheinische Friedrich-Wilhelms-Universität Bonn
  • 9. INFN Torino
  • 10. The University of Queensland, Imperial College London
  • 11. University of Adelaide


This record contains the YAML files used in Athron et al., “Global fits of axion-like particles to XENON1T and astrophysical data.” The semantic file names refer to the scenario considered: the solar ALP hypothesis (alp), the DM ALP hypothesis (dm), the tritium hypothesis (3h), the R parameter constraints (r), and/or the White Dwarf cooling hints (wd). The include/ folder contains YAML files with the common settings, while the other folders contain YAML files for reproducing our prior dependence study in Fig. 4. More details can be found in the associated paper.

The YAML files can be run with the GAMBIT software as described in e.g. the GAMBIT release paper.


Other grants: NSFC Research Fund for International Young Scientists grant 1195041050; Alexander von Humboldt Foundation and the German Federal Ministry of Education and Research; F.N.R.S. through the F.6001.19 convention; Emmy Noether grant KA 4662/1-1, ARC grants DP180102209, FT160100274, and FT190100814; STFC grant ST/P000762/1.


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Is supplement to
Journal article: arXiv:2007.05517 (arXiv)


Discovery Projects - Grant ID: DP180102209 DP180102209
Australian Research Council