The AURORA Survey: The Nebular Attenuation Curve of a Galaxy at z=4.41 from Ultraviolet to Near-Infrared Wavelengths

• Main Authors: Sanders, Ryan L, Shapley, Alice E, Topping, Michael W, Reddy, Naveen A, Berg, Danielle A, Bouwens, Rychard J, Brammer, Gabriel, Carnall, Adam C, Cullen, Fergus, Davé, Romeel, Dunlop, James S, Ellis, Richard S, Schreiber, N. M. Förster, Furlanetto, Steven R, Glazebrook, Karl, Illingworth, Garth D, Jones, Tucker, Kriek, Mariska, McLeod, Derek J, McLure, Ross J, Narayanan, Desika, Oesch, Pascal A, Pahl, Anthony J, Pettini, Max, Schaerer, Daniel, Stark, Daniel P, Steidel, Charles C, Tang, Mengtao, Clarke, Leonardo, Donnan, Callum T, Kehoe, Emily
• Format: Journal Article
• Language: English
• Published: 09.08.2024
• Subjects: Physics - Astrophysics of Galaxies

We use JWST/NIRSpec observations from the Assembly of Ultradeep Rest-optical Observations Revealing Astrophysics (AURORA) survey to constrain the shape of the nebular attenuation curve of a star-forming galaxy at z=4.41, GOODSN-17940. We utilize 11 unblended HI recombination lines to derive the atte...