DOI:https://doi.org/10.1103/PhysRevLett.129.089901
Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Open access publication funded by the Max Planck Society.
Published by the American Physical Society
The corrected upper limits (at 90% C.I.) on the coupling strengths of pseudoscalar (top) and vector (bottom) super-WIMPs. Only part of the data was acquired with a lower energy threshold, resulting in a lower exposure for data below and causing the steplike feature around this energy. Results from other experiments (see text) are also shown, together with indirect constraints from anomalous energy losses in horizontal branch (HB) and red giant (RG) stars (we refer to Ref. [6] for details).
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