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A Census from JWST of Extreme Emission-line Galaxies Spanning the Epoch of Reionization in CEERS

Authors: Kelcey Davis, Jonathan R. Trump, Raymond C. Simons, Elizabeth J. McGrath, Stephen M. Wilkins, Pablo Arrabal Haro, Micaela B. Bagley, Mark Dickinson, Vital Fernández, Ricardo O. Amorín, Bren E. Backhaus, Nikko J. Cleri, Mario Llerena, Samantha W. Brunker, Guillermo Barro, Laura Bisigello, Madisyn Brooks, Luca Costantin, Alexander de la Vega, Avishai Dekel, Steven L. Finkelstein, Nimish P. Hathi, Michaela Hirschmann, Jeyhan S. Kartaltepe, Anton M. Koekemoer, Ray A. Lucas, Casey Papovich, Pablo G. Pérez-González, Nor Pirzkal, Giulia Rodighiero, Caitlin Rose, L. Y. Aaron Yung

Kelcey Davis et al 2024 The Astrophysical Journal 974 .

Provider: AAS Journals

Caption: Figure 6.

Examples of sources with a single extreme emission feature that is consistent with their z _phot, classified in confidence Tier 1B. Photometry postage stamps show a continuum filter (top) and an extreme emission filter (bottom), with north up and east left. All postage stamps are 4″ in width and height. Panel (A): extreme emission in F444W consistent with Hβ + [O III] and a Lyman break between the F150W and F115W filters. Panel (B): extreme emission in F444W consistent with Hβ + [O III]. The images indicate at least one nearby companion. Panel (C): extreme emission in F410M consistent with Hβ + [O III]. While this EELG has a close neighbor in its image, this companion galaxy does not exhibit the same dramatic differences between continuum and emission-line filter morphologies as the EELG.

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