Detection of [OIII]88$μ$m in JADES-GS-z14-0 at z=14.1793
Sander Schouws, Rychard J. Bouwens, Katherine Ormerod, Renske Smit, Hiddo Algera, Laura Sommovigo, Jacqueline Hodge, Andrea Ferrara, Pascal A. Oesch, Lucie E. R… 展开作者
Sander Schouws, Rychard J. Bouwens, Katherine Ormerod, Renske Smit, Hiddo Algera, Laura Sommovigo, Jacqueline Hodge, Andrea Ferrara, Pascal A. Oesch, Lucie E. Rowland, Ivana van Leeuwen, Mauro Stefanon, Thomas Herard-Demanche, Yoshinobu Fudamoto, Huub Röttgering, Paul van der Werf
We report the first successful ALMA follow-up observations of a secure $z > 10$ JWST-selected galaxy, by robustly detecting ($6.6σ$) the [OIII]$_{88μm}\,$ line in JADES-GS-z14-0 (hereafter GS-z14). The ALMA detection yields a spectroscopic redshift of $z=14.1793\pm0.0007$, and increases the precision on the prior redshift measurement of $z=14.32_{-0.20}^{+0.08}$ from NIRSpec by $\gtrsim$180$\times$. Moreover, the redshift is consistent with that previously determined from a tentative detection ($3.6σ$) of CIII]$_{1907,1909}$ ($z=14.178\pm0.013$), solidifying the redshift determination via multiple line detections. We measure a line luminosity of $L_\mathrm{[OIII]88} = (2.1 \pm 0.5)\times10^8\,L_\odot$, placing GS-z14 at the lower end, but within the scatter of, the local $L_\mathrm{[OIII]88}$-star formation rate relation. No dust continuum from GS-z14 is detected, suggesting an upper limit on the dust-to-stellar mass ratio of $< 2 \times 10^{-3}$, consistent with dust production from supernovae with a yield $y_d < 0.3\,M_\odot$. Combining a previous JWST/MIRI photometric measurement of the [OIII]$λλ$4959,5007$\mathrm{\mathring{A}}$ and H$β$ lines with Cloudy models, we find GS-z14 to be surprisingly metal-enriched ($Z\sim0.05 - 0.2\,Z_\odot$) a mere $300\,\mathrm{Myr}$ after the Big Bang. The detection of a bright oxygen line in GS-z14 thus reinforces the notion that galaxies in the early Universe undergo rapid evolution.
JADES: Detecting [OIII]$λ4363$ Emitters and Testing Strong Line Calibrations in the High-$z$ Universe with Ultra-deep JWST/NIRSpec Spectroscopy up to $z \sim 9.5$
JADES reveals a large population of low mass black holes at high redshift
University of Cambridge（剑桥大学）；University College London（伦敦大学学院）；Waseda University（早稻田大学）；University of Groningen（格罗宁根大学）；Università degli Studi dell’Insubria（因苏布利亚大学）；INAF/Osservatorio Astronomico di Roma（意大利国家天体物理研究所罗马天文台）；INFN, Sezione Roma I（意大利国家核物理研究所罗马一分部）；Centro de Astrobiología (CAB), CSIC–INTA（西班牙国家航空航天技术研究所/西班牙国家科学研究委员会天体生物学中心）；European Space Agency (ESA)（欧洲空间局）；University of Oxford（牛津大学）；Scuola Normale Superiore（比萨高等师范学院）；Sorbonne Université（索邦大学）；University of Hertfordshire（赫特福德大学）；Center for Astrophysics | Harvard & Smithsonian（哈佛-史密森尼天体物理中心）；Max-Planck-Institut für extraterrestrische Physik (MPE)（马克斯·普朗克地外物理学研究所）；Steward Observatory, University of Arizona（亚利桑那大学斯蒂沃德天文台）；University of California, Santa Cruz（加州大学圣克鲁兹分校）；NSF National Optical-Infrared Astronomy Research Laboratory（美国国家光学-红外天文研究实验室）；Cosmic Dawn Center (DAWN)（宇宙黎明中心）；Niels Bohr Institute, University of Copenhagen（哥本哈根大学尼尔斯·玻尔研究所）；Canadian Institute for Theoretical Astrophysics（加拿大理论天体物理研究所）
JADES: the mass-metallicity relation at $z=1-10$. New calibrations, extremely metal-poor galaxies, and chemical diversity
University of Cambridge（剑桥大学）；Waseda University（早稻田大学）；INAF, Osservatorio di Astrofisica e Scienza dello Spazio（意大利国家天体物理研究所空间科学观测站）；University College London（伦敦大学学院）
JWST & ALMA Joint Analysis with [OII]$λλ$3726,3729, [OIII]$λ$4363, [OIII]88$μ$m, and [OIII]52$μ$m: Multi-Zone Evolution of Electron Densities at $\mathbf{z\sim0-14}$ and Its Impact on Metallicity Measurements
Institute for Cosmic Ray Research, The University of Tokyo（东京大学宇宙射线研究所）；University of Kentucky（肯塔基大学）；University College London（伦敦大学学院）；University of California, Davis（加州大学戴维斯分校）；National Astronomical Observatory of Japan（日本国立天文台）；SOKENDAI (The Graduate University for Advanced Studies)（综合研究大学院大学）；Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo（东京大学宇宙物理数学 Kavli 研究所（WPI））；University of Chicago（芝加哥大学）；Kanazawa University（金泽大学）
Tentative rotation in a galaxy at z$\sim$14 with ALMA
University of Cambridge（剑桥大学）；Cavendish Laboratory, University of Cambridge（剑桥大学卡文迪许实验室）；Scuola Normale Superiore（意大利高等师范学院）；Max-Planck-Institut für extraterrestrische Physik (MPE)（马克斯·普朗克地外物理学研究所）；Center for Astrophysics | Harvard & Smithsonian（哈佛与史密森尼天体物理中心）；Department of Physics and Astronomy, University College London（伦敦大学学院物理与天文系）；Centro de Astrobiología (CAB), CSIC–INTA（西班牙国家航空航天技术研究所/西班牙国家科学研究委员会天体生物学中心）；European Space Agency (ESA), European Space Astronomy Centre (ESAC)（欧洲空间局欧洲航天飞行控制中心）；University of Oxford（牛津大学）；Sorbonne Université, CNRS, UMR 7095, Institut d’Astrophysique de Paris（巴黎天体物理研究所（索邦大学/CNRS））；Steward Observatory, University of Arizona（亚利桑那大学斯蒂沃德天文台）；Department of Astronomy and Astrophysics University of California, Santa Cruz（加州大学圣克鲁斯分校天文学与天体物理学系）；Dipartimento di Fisica “Enrico Fermi”, Universitá di Pisa（比萨大学物理系）
Intense and extended CIII] emission suggests a strong outflow in JADES-GS-z14-0
Scuola Normale Superiore（高等师范学院）；Cosmic Dawn Center (DAWN)（宇宙黎明中心）；Niels Bohr Institute, University of Copenhagen（哥本哈根大学尼尔斯玻尔研究所）；Kavli Institute for Cosmology, University of Cambridge（剑桥大学卡弗里宇宙学研究所）；Cavendish Laboratory, University of Cambridge（剑桥大学卡文迪许实验室）；Steward Observatory, University of Arizona（亚利桑那大学斯图尔德天文台）；Centro de Astrobiología (CAB), CSIC-INTA（西班牙国家航空航天技术研究所/西班牙国家研究委员会天体生物学中心）；Department of Physics, University of Oxford（牛津大学物理系）；Sorbonne Université, CNRS（索邦大学法国国家科学研究中心）
Detection of new galaxy candidates at z > 11 in the JADES field using JWST NIRCam
Department of Physics, University of Arkansas（阿肯色大学物理系）；Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology（麻省理工学院卡弗里天体物理与空间研究研究所）；Stony Brook University（石溪大学）
Ionizing Photon Production Efficiencies and Chemical Abundances at Cosmic Dawn Revealed by Ultra-Deep Rest-Frame Optical Spectroscopy of JADES-GS-z14-0
The Pennsylvania State University（宾夕法尼亚州立大学）；University of Arizona（亚利桑那大学）；University of Cambridge（剑桥大学）
DREAMS. JWST Spectroscopy of a $z=8.3$ Galaxy with an ALMA Dust Continuum Detection: Early Dust, Very High $T_{\rm dust}$, and a Multi-wavelength [OIII] Ratio Discrepancy
Institute for Cosmic Ray Research, The University of Tokyo（宇宙射线研究所，东京大学）；Department of Physics, Graduate School of Science, The University of Tokyo（理学研究科物理学系，东京大学）；National Astronomical Observatory of Japan（日本国立天文台）；Astronomical Science Program, Graduate Institute for Advanced Studies, SOKENDAI（综合研究大学院大学天文学研究科，SOKENDAI）；Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU, WPI), The University of Tokyo（宇宙线起源研究宇宙前沿中心（Kavli IPMU），东京大学）；Institute of Liberal Arts and Science, Kanazawa University（金泽大学教养部）
Highly-ionized gas in lensed z = 6.027 Little Red Dot seen through [OIII] 88$μ$m with ALMA
Chalmers University of Technology（查尔姆斯理工大学）；Durham University（杜伦大学）；University of KwaZulu-Natal（夸祖鲁-纳塔尔大学）；Universidade Federal do Rio de Janeiro（里约热内卢联邦大学）；University of Arizona（亚利桑那大学）；Columbia University（哥伦比亚大学）；Flatiron Institute（平顿研究所）
Abundant Population of Broad H$α$ Emitters in the GOODS-N Field Revealed by CONGRESS, FRESCO, and JADES
Steward Observatory, University of Arizona（亚利桑那大学斯图尔德天文台）；Department of Astronomy, Tsinghua University（清华大学天文系）；Space Telescope Science Institute（太空望远镜科学研究所）；Department of Physics, University of Oxford（牛津大学物理系）；European Space Agency (ESA), European Space Astronomy Centre (ESAC)（欧洲空间局（ESA）欧洲空间天文中心（ESAC））；Department of Astronomy & Astrophysics, The Pennsylvania State University（宾夕法尼亚州立大学天文与天体物理系）；Kavli Institute for Cosmology, University of Cambridge（剑桥大学卡弗里宇宙学研究所）
