The Astrophysical Journal (Jan 2024)

JWST and ALMA Multiple-line Study in and around a Galaxy at z = 8.496: Optical to Far-Infrared Line Ratios and the Onset of an Outflow Promoting Ionizing Photon Escape

  • Seiji Fujimoto,
  • Masami Ouchi,
  • Kimihiko Nakajima,
  • Yuichi Harikane,
  • Yuki Isobe,
  • Gabriel Brammer,
  • Masamune Oguri,
  • Clara Giménez-Arteaga,
  • Kasper E. Heintz,
  • Vasily Kokorev,
  • Franz E. Bauer,
  • Andrea Ferrara,
  • Takashi Kojima,
  • Claudia del P. Lagos,
  • Sommovigo Laura,
  • Daniel Schaerer,
  • Kazuhiro Shimasaku,
  • Bunyo Hatsukade,
  • Kotaro Kohno,
  • Fengwu Sun,
  • Francesco Valentino,
  • Darach Watson,
  • Yoshinobu Fudamoto,
  • Akio K. Inoue,
  • Jorge González-López,
  • Anton M. Koekemoer,
  • Kirsten Knudsen,
  • Minju M. Lee,
  • Georgios E. Magdis,
  • Johan Richard,
  • Victoria B. Strait,
  • Yuma Sugahara,
  • Yoichi Tamura,
  • Sune Toft,
  • Hideki Umehata,
  • Gregory Walth

DOI
https://doi.org/10.3847/1538-4357/ad235c
Journal volume & issue
Vol. 964, no. 2
p. 146

Abstract

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We present Atacama Large Millimeter/submillimeter Array (ALMA) deep spectroscopy for a lensed galaxy at z _spec = 8.496 with $\mathrm{log}({M}_{\mathrm{star}}/{M}_{\odot })\sim 7.8$ whose optical nebular lines and stellar continuum are detected by JWST/NIRSpec and NIRCam Early Release Observations in the field of SMACS J0723.3–7327. Our ALMA spectrum shows [O iii ] 88 μ m and [C ii ] 158 μ m line detections at 4.0 σ and 4.5 σ , respectively. The redshift and position of the [O iii ] line coincide with those of the JWST source, while the [C ii ] line is blueshifted by 90 km s ^−1 with a spatial offset of 0.″5 (≈0.5 kpc in the source plane) from the centroid of the JWST source. The NIRCam F444W image, including [O iii ] λ 5007 and H β line emission, spatially extends beyond the stellar components by a factor of >8. This indicates that the z = 8.5 galaxy has already experienced strong outflows as traced by extended [O iii ] λ 5007 and offset [C ii ] emission, which would promote ionizing photon escape and facilitate reionization. With careful slit-loss corrections and the removal of emission spatially outside the galaxy, we evaluate the [O iii ] 88 μ m/ λ 5007 line ratio, and derive the electron density n _e by photoionization modeling to be ${220}_{-130}^{+230}$ cm ^−3 , which is comparable with those of z ∼ 2–3 galaxies. We estimate an [O iii ] 88 μ m/[C ii ] 158 μ m line ratio in the galaxy of >4, as high as those of known z ∼ 6–9 galaxies. This high [O iii ] 88 μ m/[C ii ] 158 μ m line ratio is generally explained by the high n _e as well as the low metallicity ( ${Z}_{\mathrm{gas}}/{Z}_{\odot }={0.04}_{-0.02}^{+0.02}$ ), high ionization parameter ( $\mathrm{log}U\gt -2.27$ ), and low carbon-to-oxygen abundance ratio (log(C/O) = [−0.52: −0.24]) obtained from the JWST/NIRSpec data; further [C ii ] follow-up observations will constrain the covering fraction of photodissociation regions.

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