Extreme emission line galaxies detected in JADES JWST/NIRSpec I: inferred galaxy properties

Extreme emission line galaxies detected in JADES JWST/NIRSpec I: inferred galaxy properties

Extreme emission line galaxies (EELGs) exhibit large equivalent widths (EW) in their rest-optical emission lines ([OIII]$\lambda5007$ or H$\alpha$ rest-frame EW$ > 750\r{A}$) which can be tied to a recent upturn in star formation rate, due to the sensitivity of the nebular line emission and the r...

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Hauptverfasser: Boyett, Kit, Bunker, Andrew J, Curtis-Lake, Emma, Chevallard, Jacopo, Cameron, Alex J, Jones, Gareth C, Saxena, Aayush, Charlot, Stéphane, Curti, Mirko, Wallace, Imaan E. B, Arribas, Santiago, Carniani, Stefano, Willott, Chris, Alberts, Stacey, Eisenstein, Daniel J, Hainline, Kevin, Hausen, Ryan, Johnson, Benjamin D, Rieke, Marcia, Robertson, Brant, Stark, Daniel P, Tacchella, Sandro, Williams, Christina C, Chen, Zuyi, Egami, Eiichi, Endsley, Ryan, Kumari, Nimisha, Laseter, Isaac, Looser, Tobias J, Maseda, Michael V, Scholtz, Jan, Shivaei, Irene, Simmonds, Charlotte, Smit, Renske, Übler, Hannah, Witstok, Joris
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Sprache:eng
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Physics - Astrophysics of Galaxies
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Zusammenfassung:Extreme emission line galaxies (EELGs) exhibit large equivalent widths (EW) in their rest-optical emission lines ([OIII]$\lambda5007$ or H$\alpha$ rest-frame EW$ > 750\r{A}$) which can be tied to a recent upturn in star formation rate, due to the sensitivity of the nebular line emission and the rest-optical continuum to young ($
DOI:10.48550/arxiv.2401.16934