The Physical Conditions of Emission-line Galaxies at Cosmic Dawn from JWST/NIRSpec Spectroscopy in the SMACS 0723 Early Release Observations
Creators: name: Trump, Jonathan R
name: Haro, Pablo Arrabal
name: Simons, Raymond C
name: Backhaus, Bren E
name: Amorín, Ricardo O
name: Dickinson, Mark
name: Fernández, Vital
name: Papovich, Casey
name: Nicholls, David C
name: Kewley, Lisa J
name: Brunker, Samantha W
name: Salzer, John J
name: Wilkins, Stephen M
name: Almaini, Omar
name: Bagley, Micaela B
name: Berg, Danielle A
name: Bhatawdekar, Rachana
name: Bisigello, Laura
name: Buat, Véronique
name: Burgarella, Denis
name: Calabrò, Antonello
name: Casey, Caitlin M
name: Ciesla, Laure
name: Cleri, Nikko J
name: Cole, Justin W
name: Cooper, MC
name: Cooray, Asantha R
name: Costantin, Luca
name: Croton, Darren
name: Ferguson, Henry C
name: Finkelstein, Steven L
name: Fujimoto, Seiji
name: Gardner, Jonathan P
name: Gawiser, Eric
name: Giavalisco, Mauro
name: Grazian, Andrea
name: Grogin, Norman A
name: Hathi, Nimish P
name: Hirschmann, Michaela
name: Holwerda, Benne W
name: Huertas-Company, Marc
name: Hutchison, Taylor A
name: Jogee, Shardha
name: Juneau, Stéphanie
name: Jung, Intae
name: Kartaltepe, Jeyhan S
name: Kirkpatrick, Allison
name: Kocevski, Dale D
name: Koekemoer, Anton M
name: Lotz, Jennifer M
name: Lucas, Ray A
name: Magnelli, Benjamin
name: Matharu, Jasleen
name: Pérez-González, Pablo G
name: Pirzkal, Nor
name: Rafelski, Marc
name: Rose, Caitlin
name: Seillé, Lise-Marie
name: Somerville, Rachel S
name: Straughn, Amber N
name: Tacchella, Sandro
name: Vanderhoof, Brittany N
name: Weiner, Benjamin J
name: Wuyts, Stijn
name: Aaron Yung, LY
name: Zavala, Jorge A
Publisher: name: Apollo - University of Cambridge Repository
Year: 2023
Subjects: 310
Galaxies and Cosmology

description: Abstract We present rest-frame optical emission-line flux ratio measurements for five z &gt; 5 galaxies observed by the James Webb Space Telescope Near-Infared Spectrograph (NIRSpec) in the SMACS 0723 Early Release Observations. We add several quality-control and post-processing steps to the NIRSpec pipeline reduction products in order to ensure reliable relative flux calibration of emission lines that are closely separated in wavelength, despite the uncertain absolute spectrophotometry of the current version of the reductions. Compared to z ∼ 3 galaxies in the literature, the z &gt; 5 galaxies have similar [O iii]λ5008/Hβ ratios, similar [O iii]λ4364/Hγ ratios, and higher (∼0.5 dex) [Ne III]λ3870/[O II]λ3728 ratios. We compare the observations to MAPPINGS V photoionization models and find that the measured [Ne III]λ3870/[O II]λ3728, [O iii]λ4364/Hγ, and [O iii]λ5008/Hβ emission-line ratios are consistent with an interstellar medium (ISM) that has very high ionization ( log ( Q ) ≃ 8 − 9 , units of cm s<sup>−1</sup>), low metallicity (Z/Z <sub>⊙</sub> ≲ 0.2), and very high pressure ( log ( P / k ) ≃ 8 − 9 , units of cm<sup>−3</sup>). The combination of [O iii]λ4364/Hγ and [O iii]λ(4960 + 5008)/Hβ line ratios indicate very high electron temperatures of 4.1 &lt; log ( T e / K ) &lt; 4.4 , further implying metallicities of Z/Z <sub>⊙</sub> ≲ 0.2 with the application of low-redshift calibrations for “T <sub> e </sub>-based” metallicities. These observations represent a tantalizing new view of the physical conditions of the ISM in galaxies at cosmic dawn.