TY - JOUR

T1 - Deep ALMA redshift search of a z ∼12 GLASS-JWST galaxy candidate

AU - Bakx, Tom J.L.C.

AU - Zavala, Jorge A.

AU - Mitsuhashi, Ikki

AU - Treu, Tommaso

AU - Fontana, Adriano

AU - Tadaki, Ken Ichi

AU - Casey, Caitlin M.

AU - Castellano, Marco

AU - Glazebrook, Karl

AU - Hagimoto, Masato

AU - Ikeda, Ryota

AU - Jones, Tucker

AU - Leethochawalit, Nicha

AU - Mason, Charlotte

AU - Morishita, Takahiro

AU - Nanayakkara, Themiya

AU - Pentericci, Laura

AU - Roberts-Borsani, Guido

AU - Santini, Paola

AU - Serjeant, Stephen

AU - Tamura, Yoichi

AU - Trenti, Michele

AU - Vanzella, Eros

N1 - Publisher Copyright: © 2022 The Author(s).

PY - 2023/3/4

Y1 - 2023/3/4

N2 - The JWST has discovered a surprising abundance of bright galaxy candidates in the very early universe (≤500 Myr after the Big Bang), calling into question current galaxy formation models. Spectroscopy is needed to confirm the primeval nature of these candidates, as well as to understand how the first galaxies form stars and grow. Here we present deep spectroscopic and continuum ALMA observations towards GHZ2/GLASS-z12, one of the brightest and most robust candidates at z > 10, identified in the GLASS-JWST Early Release Science Program. We detect a 5.8σ line, offset 0″.5 from the JWST position of GHZ2/GLASS-z12, that associating it with the [O iii] 88 μm transition, implies a spectroscopic redshift of z = 12.117 ± 0.001. We verify the detection using extensive statistical tests. The oxygen line luminosity places GHZ2/GLASS-z12 above the [O iii]-SFR relation for metal-poor galaxies, implying an enhancement of [O iii] emission in this system while the JWST-observed emission is likely a lower-metallicity region. The lack of dust emission seen by these observations is consistent with the blue UV slope observed by JWST, which suggest little dust attenuation in galaxies at this early epoch. Further observations will unambiguously confirm the redshift and shed light on the origins of the wide and offset line and physical properties of this early galaxy. This work illustrates the synergy between JWST and ALMA, and paves the way for future spectroscopic surveys of z > 10 galaxy candidates.

AB - The JWST has discovered a surprising abundance of bright galaxy candidates in the very early universe (≤500 Myr after the Big Bang), calling into question current galaxy formation models. Spectroscopy is needed to confirm the primeval nature of these candidates, as well as to understand how the first galaxies form stars and grow. Here we present deep spectroscopic and continuum ALMA observations towards GHZ2/GLASS-z12, one of the brightest and most robust candidates at z > 10, identified in the GLASS-JWST Early Release Science Program. We detect a 5.8σ line, offset 0″.5 from the JWST position of GHZ2/GLASS-z12, that associating it with the [O iii] 88 μm transition, implies a spectroscopic redshift of z = 12.117 ± 0.001. We verify the detection using extensive statistical tests. The oxygen line luminosity places GHZ2/GLASS-z12 above the [O iii]-SFR relation for metal-poor galaxies, implying an enhancement of [O iii] emission in this system while the JWST-observed emission is likely a lower-metallicity region. The lack of dust emission seen by these observations is consistent with the blue UV slope observed by JWST, which suggest little dust attenuation in galaxies at this early epoch. Further observations will unambiguously confirm the redshift and shed light on the origins of the wide and offset line and physical properties of this early galaxy. This work illustrates the synergy between JWST and ALMA, and paves the way for future spectroscopic surveys of z > 10 galaxy candidates.

KW - dust, extinction

KW - galaxies: distances and redshifts

KW - galaxies: evolution

KW - galaxies: formation

KW - galaxies: high-redshift

KW - techniques: spectroscopic

U2 - 10.1093/mnras/stac3723

DO - 10.1093/mnras/stac3723

M3 - Journal article

AN - SCOPUS:85148422982

VL - 519

SP - 5076

EP - 5085

JO - Royal Astronomical Society. Monthly Notices

JF - Royal Astronomical Society. Monthly Notices

SN - 0035-8711

IS - 4

ER -