Delays between the time when a redshift was recorded vs. when the first relevant observation was obtained. We differentiate between redshifts that are only photometric, those that have been obtained by low-to-medium resolution spectrographs (resolution R< 3000) and those that have been obtained by medium-to-high resolution spectrographs (R> 3000). For each observation, the redshift itself is color-coded. Finally, with gray areas, we highlight the expected observation and report times for the initial PIRT observation, our planned follow-up with large ground-based facilities, and planned follow-up with JWST NIRSpec.