All RUBIES LRDs (red) found in this work followed by rest-optical point sources with v-shaped continua (orange) all organized by redshift. In each column in each row we show the following: the 1″ × 1″ F444W/F277W/F150W RGB cutouts (left), the log-scaled PRISM spectra with the location of the Balmer limit marked with a dashed line (middle), and the linear-scaled G395M ±3000 km s⁻¹ zoom-in of the Hα line where available, otherwise Hβ, with the broad unite fit superimposed (right).