The Physical Conditions of Emission-line Galaxies at Cosmic Dawn from JWST/NIRSpec Spectroscopy in the SMACS 0723 Early Release Observations
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The Physical Conditions of Emission-line Galaxies at Cosmic Dawn from JWST/NIRSpec Spectroscopy in the SMACS 0723 Early Release Observations. / Trump, Jonathan R.; Haro, Pablo Arrabal; Simons, Raymond C.; Backhaus, Bren E.; Amorin, Ricardo O.; Dickinson, Mark; Fernandez, Vital; Papovich, Casey; Nicholls, David C.; Kewley, Lisa J.; Brunker, Samantha W.; Salzer, John J.; Wilkins, Stephen M.; Almaini, Omar; Bagley, Micaela B.; Berg, Danielle A.; Bhatawdekar, Rachana; Bisigello, Laura; Buat, Veronique; Burgarella, Denis; Calabro, Antonello; Casey, Caitlin M.; Ciesla, Laure; Cleri, Nikko J.; Cole, Justin W.; Cooper, M. C.; Cooray, Asantha R.; Costantin, Luca; Croton, Darren; Ferguson, Henry C.; Finkelstein, Steven L.; Fujimoto, Seiji; Gardner, Jonathan P.; Gawiser, Eric; Giavalisco, Mauro; Grazian, Andrea; Grogin, Norman A.; Hathi, Nimish P.; Hirschmann, Michaela; Holwerda, Benne W.; Huertas-Company, Marc; Hutchison, Taylor A.; Jogee, Shardha; Juneau, Stephanie; Jung, Intae; Kartaltepe, Jeyhan S.; Kirkpatrick, Allison; Kocevski, Dale D.; Koekemoer, Anton M.; Lotz, Jennifer M.; Lucas, Ray A.; Magnelli, Benjamin; Matharu, Jasleen; Perez-Gonzalez, Pablo G.; Pirzkal, Nor; Rafelski, Marc; Rose, Caitlin; Seille, Lise-Marie; Somerville, Rachel S.; Straughn, Amber N.; Tacchella, Sandro; Vanderhoof, Brittany N.; Weiner, Benjamin J.; Wuyts, Stijn; Aaron Yung, L. Y.; Zavala, Jorge A.
In: Astrophysical Journal, Vol. 945, No. 1, 35, 01.03.2023.Research output: Contribution to journal › Journal article › Research › peer-review
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TY - JOUR
T1 - The Physical Conditions of Emission-line Galaxies at Cosmic Dawn from JWST/NIRSpec Spectroscopy in the SMACS 0723 Early Release Observations
AU - Trump, Jonathan R.
AU - Haro, Pablo Arrabal
AU - Simons, Raymond C.
AU - Backhaus, Bren E.
AU - Amorin, Ricardo O.
AU - Dickinson, Mark
AU - Fernandez, Vital
AU - Papovich, Casey
AU - Nicholls, David C.
AU - Kewley, Lisa J.
AU - Brunker, Samantha W.
AU - Salzer, John J.
AU - Wilkins, Stephen M.
AU - Almaini, Omar
AU - Bagley, Micaela B.
AU - Berg, Danielle A.
AU - Bhatawdekar, Rachana
AU - Bisigello, Laura
AU - Buat, Veronique
AU - Burgarella, Denis
AU - Calabro, Antonello
AU - Casey, Caitlin M.
AU - Ciesla, Laure
AU - Cleri, Nikko J.
AU - Cole, Justin W.
AU - Cooper, M. C.
AU - Cooray, Asantha R.
AU - Costantin, Luca
AU - Croton, Darren
AU - Ferguson, Henry C.
AU - Finkelstein, Steven L.
AU - Fujimoto, Seiji
AU - Gardner, Jonathan P.
AU - Gawiser, Eric
AU - Giavalisco, Mauro
AU - Grazian, Andrea
AU - Grogin, Norman A.
AU - Hathi, Nimish P.
AU - Hirschmann, Michaela
AU - Holwerda, Benne W.
AU - Huertas-Company, Marc
AU - Hutchison, Taylor A.
AU - Jogee, Shardha
AU - Juneau, Stephanie
AU - Jung, Intae
AU - Kartaltepe, Jeyhan S.
AU - Kirkpatrick, Allison
AU - Kocevski, Dale D.
AU - Koekemoer, Anton M.
AU - Lotz, Jennifer M.
AU - Lucas, Ray A.
AU - Magnelli, Benjamin
AU - Matharu, Jasleen
AU - Perez-Gonzalez, Pablo G.
AU - Pirzkal, Nor
AU - Rafelski, Marc
AU - Rose, Caitlin
AU - Seille, Lise-Marie
AU - Somerville, Rachel S.
AU - Straughn, Amber N.
AU - Tacchella, Sandro
AU - Vanderhoof, Brittany N.
AU - Weiner, Benjamin J.
AU - Wuyts, Stijn
AU - Aaron Yung, L. Y.
AU - Zavala, Jorge A.
PY - 2023/3/1
Y1 - 2023/3/1
N2 - We present rest-frame optical emission-line flux ratio measurements for five z > 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 similar to 3 galaxies in the literature, the z > 5 galaxies have similar [O iii]lambda 5008/H beta ratios, similar [O iii]lambda 4364/H gamma ratios, and higher (similar to 0.5 dex) [Ne III]lambda 3870/[O II]lambda 3728 ratios. We compare the observations to MAPPINGS V photoionization models and find that the measured [Ne III]lambda 3870/[O II]lambda 3728, [O iii]lambda 4364/H gamma, and [O iii]lambda 5008/H beta emission-line ratios are consistent with an interstellar medium (ISM) that has very high ionization ( log(Q)?8-9 , units of cm s(-1)), low metallicity (Z/Z (?) ? 0.2), and very high pressure ( log(P/k)?8-9, units of cm(-3)). The combination of [O iii]lambda 4364/H gamma and [O iii]lambda(4960 + 5008)/H beta line ratios indicate very high electron temperatures of 4.1 < log(T-e/K) < 4.4, further implying metallicities of Z/Z(?)?0.2 with the application of low-redshift calibrations for "T-e -based " metallicities. These observations represent a tantalizing new view of the physical conditions of the ISM in galaxies at cosmic dawn.
AB - We present rest-frame optical emission-line flux ratio measurements for five z > 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 similar to 3 galaxies in the literature, the z > 5 galaxies have similar [O iii]lambda 5008/H beta ratios, similar [O iii]lambda 4364/H gamma ratios, and higher (similar to 0.5 dex) [Ne III]lambda 3870/[O II]lambda 3728 ratios. We compare the observations to MAPPINGS V photoionization models and find that the measured [Ne III]lambda 3870/[O II]lambda 3728, [O iii]lambda 4364/H gamma, and [O iii]lambda 5008/H beta emission-line ratios are consistent with an interstellar medium (ISM) that has very high ionization ( log(Q)?8-9 , units of cm s(-1)), low metallicity (Z/Z (?) ? 0.2), and very high pressure ( log(P/k)?8-9, units of cm(-3)). The combination of [O iii]lambda 4364/H gamma and [O iii]lambda(4960 + 5008)/H beta line ratios indicate very high electron temperatures of 4.1 < log(T-e/K) < 4.4, further implying metallicities of Z/Z(?)?0.2 with the application of low-redshift calibrations for "T-e -based " metallicities. These observations represent a tantalizing new view of the physical conditions of the ISM in galaxies at cosmic dawn.
KW - STAR-FORMING GALAXIES
KW - MASS-METALLICITY RELATION
KW - SIMILAR-TO 2
KW - NEAR-INFRARED SPECTROSCOPY
KW - MOSDEF SURVEY
KW - CHEMICAL-COMPOSITION
KW - COLLISION STRENGTHS
KW - NEBULAR EMISSION
KW - ATOMIC DATABASE
KW - LY-ALPHA
U2 - 10.3847/1538-4357/acba8a
DO - 10.3847/1538-4357/acba8a
M3 - Journal article
VL - 945
JO - Astrophysical Journal
JF - Astrophysical Journal
SN - 0067-0049
IS - 1
M1 - 35
ER -
ID: 344292260