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JADES NIRSpec Spectroscopy of GN-z11: Lyman- α emission and possible enhanced nitrogen abundance in a z = 10.60 luminous galaxy

Bunker, AJ, Saxena, A, Cameron, AJ, Willott, CJ, Curtis-Lake, E, Jakobsen, P, Carniani, S, Smit, R, Maiolino, R, Witstok, J, Curti, M, D'eugenio, F, Jones, GC, Ferruit, P, Arribas, S, Charlot, S, Chevallard, J, Giardino, G, De Graaff, A, Looser, TJ , Lützgendorf, N, Maseda, MV, Rawle, T, Rix, HW, Del Pino, BR, Alberts, S, Egami, E, Eisenstein, DJ, Endsley, R, Hainline, K, Hausen, R, Johnson, BD, Rieke, G, Rieke, M, Robertson, BE, Shivaei, I, Stark, DP, Sun, F, Tacchella, S, Tang, M, Williams, CC, Willmer, CNA, Baker, WM, Baum, S, Bhatawdekar, R, Bowler, R, Boyett, K, Chen, Z, Circosta, C, Helton, JM, Ji, Z, Kumari, N, Lyu, J, Nelson, E, Parlanti, E, Perna, M, Sandles, L, Scholtz, J, Suess, KA, Topping, MW, Übler, H, Wallace, IEB and Whitler, L (2023) JADES NIRSpec Spectroscopy of GN-z11: Lyman- α emission and possible enhanced nitrogen abundance in a z = 10.60 luminous galaxy. Astronomy and Astrophysics, 677. ISSN 0004-6361

JADES NIRSpec Spectroscopy of GN-z11 - Lyman-a emission and possible enhanced nitrogen abdundance in a z=10.60 luminous galaxy.pdf - Published Version
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We present JADES JWST/NIRSpec spectroscopy of GN-z11, the most luminous candidate z>10 Lyman break galaxy in the GOODS-North field with MUV =-21.5. We derive a redshift of z = 10.603 (lower than previous determinations) based on multiple emission lines in our low and medium resolution spectra over 0.7- 5.3 μm. We significantly detect the continuum and measure a blue rest-UV spectral slope of β =-2.4. Remarkably, we see spatially extended Lyman-α in emission (despite the highly neutral intergalactic medium expected at this early epoch), offset 555 km s-1 redwards of the systemic redshift. From our measurements of collisionally excited lines of both low and high ionisation (including [O II] λ3727, [Ne III] λ3869, and C III] λ1909), we infer a high ionisation parameter (log U ∼-2). We detect the rarely seen N IV] λ1486 and N III] λ1748 lines in both our low and medium resolution spectra, with other high ionisation lines seen in the low resolution spectrum, such as He II (blended with O III]) and C IV (with a possible P-Cygni profile). Based on the observed rest-UV line ratios, we cannot conclusively rule out photoionisation from an active galactic nucleus (AGN), although the high C III]/He II and N III]/He II ratios are compatible with a star formation explanation. If the observed emission lines are powered by star formation, then the strong N III] λ1748 observed may imply an unusually high N/O abundance. Balmer emission lines (Hγ, Hδ) are also detected, and if powered by star formation rather than an AGN, we infer a star formation rate of ∼20-30 M⊙ yr-1 (depending on the initial mass function) and low dust attenuation. Our NIRSpec spectroscopy confirms that GN-z11 is a remarkable galaxy with extreme properties seen 430 Myr after the Big Bang.

Item Type: Article
Uncontrolled Keywords: 0201 Astronomical and Space Sciences; Astronomy & Astrophysics
Subjects: Q Science > QB Astronomy
Divisions: Astrophysics Research Institute
Publisher: EDP Sciences
SWORD Depositor: A Symplectic
Date Deposited: 11 Dec 2023 17:07
Last Modified: 11 Dec 2023 17:15
DOI or ID number: 10.1051/0004-6361/202346159
URI: https://researchonline.ljmu.ac.uk/id/eprint/22083
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