Millisecond magnetars produced in the center of dying massive stars are one prominent model to power gamma-ray bursts (GRBs). However, their detailed nature remains a mystery. To explore effects initial mass, rotation rate, wind mass loss, and metallicity on GRB progenitors newborn magnetar properties, we evolve 227 $10-30~M_\odot$ single star models from pre-main-sequence core collapse by usin...