One of the tasks is to distinguish signals from background sources so as not to confuse them with real signals of dark matter. Experiments are underway to separate the effects of gravitational lensing and anomalies in the distribution of galaxies, which may indicate the properties of dark matter particles. The results push the theory towards new scenarios for the interaction of particles and the energy horizon of the Universe.
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Data from various observatories allows us to build more coherent models of cosmological processes and clarify the contribution of dark matter to the evolution of the structure in the Universe. In the future, astronomers are counting on additional missions and improved detectors that can bring humanity closer to answering fundamental questions about the nature of matter.
