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The OCAPi project develops advanced data analysis techniques to optimize the use of galaxy shape data from the Euclid mission and Rubin Observatory. By analyzing lensing maps at the pixel level, it aims to improve the precision of cosmological parameters and enhance understanding of dark energy and dark matter.
Distorted by the gravity of cosmic structures, galaxy shapes can answer the biggest questions in cosmology:
How do cosmic structures form?
What is the nature of dark energy and dark matter?While the cosmological model succeeds at explaining a wide range of observations, it relies on two components whose nature remains unknown: dark matter and dark energy.
Moreover, weak lensing surveys have found that the Universe is more homogeneous than expected from the cosmic microwave background, indicating…
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