Our cosmological initial conditions are based on the simulation Phi-4096 of ref. 51. In this work, a dark-matter-only N-body simulation was performed in a comoving box of side length 16 h−1 Mpc. The initial condition is generated by MUSIC52 at a redshift of 127. The cosmological parameters used follow the latest measurement by Planck53: Ωm = 0.31, ΩΛ = 0.69, Ωb = 0.048, h = 0.68,
Observations and data reduction In this work we present observations acquired on 14 April 2025 between 21:38 ut and 21:41 ut using the world’s largest telescope for optical and infrared observations of the Sun, DKIST21. During the data acquisition, the atmospheric conditions were variable, with Fried parameter values during the best periods measured around \(Check back often
