JADES: Discovery of extremely high equivalent width Lyman-α emission from a faint galaxy within an ionized bubble at z = 7.3
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Published:2023-10
Issue:
Volume:678
Page:A68
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ISSN:0004-6361
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Container-title:Astronomy & Astrophysics
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language:
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Short-container-title:A&A
Author:
Saxena AayushORCID, Robertson Brant E., Bunker Andrew J., Endsley Ryan, Cameron Alex J.ORCID, Charlot StephaneORCID, Simmonds CharlotteORCID, Tacchella SandroORCID, Witstok JorisORCID, Willott Chris, Carniani StefanoORCID, Curtis-Lake Emma, Ferruit PierreORCID, Jakobsen PeterORCID, Arribas SantiagoORCID, Chevallard JacopoORCID, Curti MirkoORCID, D’Eugenio FrancescoORCID, De Graaff AnnaORCID, Jones Gareth C.ORCID, Looser Tobias J., Maseda Michael V.ORCID, Rawle TimORCID, Rix Hans-WalterORCID, Del Pino Bruno RodríguezORCID, Smit Renske, Übler HannahORCID, Eisenstein Daniel J.ORCID, Hainline Kevin, Hausen RyanORCID, Johnson Benjamin D.ORCID, Rieke MarciaORCID, Williams Christina C.ORCID, Willmer Christopher N. A.ORCID, Baker William M.ORCID, Bhatawdekar Rachana, Bowler RebeccaORCID, Boyett KristanORCID, Chen Zuyi, Egami Eiichi, Ji Zhiyuan, Kumari Nimisha, Nelson Erica, Perna MicheleORCID, Sandles LesterORCID, Scholtz Jan, Shivaei Irene
Abstract
We report the discovery of a remarkable Lyα emitting galaxy at z = 7.2782, JADES-GS+53.16746−27.7720 (shortened to JADES-GS-z7-LA), with rest-frame equivalent width, EW0(Lyα) = 388.0 ± 88.8 Å and UV magnitude −17.0. The spectroscopic redshift is confirmed via rest-frame optical lines [O II], Hβ and [O III] in its JWST/NIRSpec Micro-Shutter Assembly (MSA) spectrum. The Lyα line is detected in both lower resolution (R ∼ 100) PRISM as well as medium resolution (R ∼ 1000) G140M grating spectra. The line spread function-deconvolved Lyα full width at half maximum in the grating is 383.9 ± 56.2 km s−1 and the Lyα velocity offset compared to the systemic redshift is 113.3 ± 80.0 km s−1, indicative of very little neutral gas or dust within the galaxy. We estimate the Lyα escape fraction to be > 70%. JADES-GS-z7-LA has a [O III]/[O II] ratio (O32) of 11.1 ± 2.2 and a ([O III] + [O II])/Hβ ratio (R23) of 11.2 ± 2.6, consistent with low metallicity and high ionization parameters. Deep NIRCam imaging also revealed a close companion source (separated by 0.23″), which exhibits similar photometry to that of JADES-GS-z7-LA, with a photometric excess in the F410M NIRCam image consistent with [O III] + Hβ emission at the same redshift. The spectral energy distribution of JADES-GS-z7-LA indicates a “bursty” star formation history, with a low stellar mass of ≈107 M⊙. Assuming that the Lyα transmission through the intergalactic medium is the same as its measured escape fraction, an ionized region of size > 1.5 pMpc is needed to explain the high Lyα EW and low velocity offset compared to systemic seen in JADES-GS-z7-LA. Owing to its UV-faintness, we show that it is incapable of single-handedly ionizing a region large enough to explain its Lyα emission. Therefore, we suggest that JADES-GS-z7-LA (and possibly the companion source) may be a part of a larger overdensity, presenting direct evidence of overlapping ionized bubbles at z > 7.
Funder
European Research Council
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference124 articles.
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