The SXS collaboration has produced a catalog of about 90 simulations of binary black holes with spins aligned with the orbital angular momentum. We sample systems with both spins co-rotating, one co-rotating and one counter-rotating, or both counter-rotating. We compare these simulations with several waveform models in use by LIGO, and find generally excellent agreement. The papers can be accessed [arXiv:1512.06800] and [arXiv:1601.05396].