The Institute of Cosmos Sciences of the University of Barcelona (ICCUB) releases its first waveform catalog of eccentric binary black holes, with 128 simulations. This set focuses on non-precessing systems with mass ratios of q=1 and explores a range of initial conditions. The component black hole spins (χ1,χ2) range from -0.5 to 0.5, while the initial eccentricities ϵ0 range from 0.62 to 0.78. Each simulation includes detailed initial data, waveforms extrapolated to infinity, and the properties of the final remnant black hole.
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