Erratum: Constraints on dark photon dark matter using data from LIGO’s and Virgo’s third observing run [Phys. Rev. D 105, 063030 (2022)]

Figure 1

Updated Fig. 3 of the original article, showing the effect of the reduced ORF on the cross-correlation upper limits (BSD limits remain the same). Even though the fast Fourier transform length $T_{\mathrm{FFT}}$ is lower (compared to that of cross correlation) at higher frequencies, the improvement factor resulting from the finite time correction is orders of magnitude larger than the reduction in sensitivity due to a shorter $T_{\mathrm{FFT}}$.