Image Details
Caption: Figure 1.
CEERS NIRCam filters and their coverage of extreme emission lines as a function of redshift. Colored filters are utilized in photometric identification while gray filters are not. We select EELGs using only Hα and Hβ + [O III], but also show Paα, Paβ, and [Ne III] + [O II] to showcase their locations in photometric filters at lower and higher redshifts.
© 2024. The Author(s). Published by the American Astronomical Society.