A new cylindrical cosmological simulation method with radially varying resolution enables self-consistent N-body evolution in S¹×ℝ² topology for systems mismatched to cubic periodicity.
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astro-ph.CO 2years
2026 2verdicts
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A new deep-to-wide transfer function reduces mean redshift biases in Euclid tomographic bins by matching reference sample color distributions to the wide survey.
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Cylindrical cosmological simulations with StePS
A new cylindrical cosmological simulation method with radially varying resolution enables self-consistent N-body evolution in S¹×ℝ² topology for systems mismatched to cubic periodicity.
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Euclid: Improving redshift distribution reconstruction using a deep-to-wide transfer function
A new deep-to-wide transfer function reduces mean redshift biases in Euclid tomographic bins by matching reference sample color distributions to the wide survey.