Discovery spectra of the new quasars at z ≥ 6.9. The redshifts estimated from the Lyα breaks, the short names, and the instruments for the discoveries are noted in the each panels. The spectra are fluxed, but not corrected for telluric absorption. They are also smoothed with inverse-variance weights and a 3 or 11 pixel window for Magellan or Keck, respectively. The red curves in each panel show the smoothed noise vectors. The dashed, vertical light blue lines indicate the positions of Lyα and N V lines.