First Sample of H$α$+[O III] $λ$5007 Line Emitters at $z > 6$ Through JWST/NIRCam Slitless Spectroscopy: Physical Properties and Line Luminosity Functions
Fengwu Sun, Eiichi Egami, Nor Pirzkal, Marcia Rieke, Stefi Baum, Martha Boyer, Kristan Boyett, Andrew J. Bunker, Alex J. Cameron, Mirko Curti, Daniel J. Eisenst… 展开作者
Fengwu Sun, Eiichi Egami, Nor Pirzkal, Marcia Rieke, Stefi Baum, Martha Boyer, Kristan Boyett, Andrew J. Bunker, Alex J. Cameron, Mirko Curti, Daniel J. Eisenstein, Mario Gennaro, Thomas P. Greene, Daniel Jaffe, Doug Kelly, Anton M. Koekemoer, Nimisha Kumari, Roberto Maiolino, Michael Maseda, Michele Perna, Armin Rest, Brant E. Robertson, Everett Schlawin, Renske Smit, John Stansberry, Ben Sunnquist, Sandro Tacchella, Christina C. Williams, Christopher N. A. Willmer
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26 pages, 11 figures, accepted for publication in ApJ on May 11, 2023
We present a sample of four emission-line galaxies at $z=6.11-6.35$ that were serendipitously discovered using the commissioning data for the JWST/NIRCam wide-field slitless spectroscopy (WFSS) mode. One of them (at $z=6.11$) has been reported previously while the others are new discoveries. These sources are selected by the secure detections of both [O III] $λ$5007 and H$α$ lines with other fainter lines tentatively detected in some cases (e.g., [O II] $λ$3727, [O III] $λ$4959). In the [O III]/H$β$ - [N II]/H$α$ Baldwin-Phillips-Terlevich diagram, these galaxies occupy the same parameter space as that of $z\sim2$ star-forming galaxies, indicating that they have been enriched rapidly to sub-solar metallicities ($\sim$0.4 $Z_{\odot}$), similar to galaxies with comparable stellar masses at much lower redshifts. The detection of strong H$α$ lines suggests a higher ionizing photon production efficiency within galaxies in the early Universe. We find brightening of the [O III] $λ$5007 line luminosity function (LF) from $z=3$ to 6, and weak or no redshift evolution of the H$α$ line LF from $z=2$ to 6. Both LFs are under-predicted at $z\sim6$ by a factor of $\sim$10 in certain cosmological simulations. This further indicates a global Ly$α$ photon escape fraction of 7-10% at $z\sim6$, slightly lower than previous estimates through the comparison of the UV-derived star-formation rate density and Ly$α$ luminosity density. Our sample recovers $66^{+128}_{-44}$% of $z=6.0-6.6$ galaxies in the survey volume with stellar masses greater than $5\times10^8$ $M_{\odot}$, suggesting the ubiquity of strong H$α$ and [O III] line emitters in the Epoch of Reionization, which will be further uncovered in the era of JWST.
Slitless Areal Pure-Parallel HIgh-Redshift Emission Survey (SAPPHIRES): Early Data Release of Deep JWST/NIRCam Images and Spectra in MACS J0416 Parallel Field
MOCSS: Multi-Object Coronagraphy for JWST/NIRSpec Slitless Spectroscopy
University of Minnesota（明尼苏达大学）；Stockholm University（斯德哥尔摩大学）；Space Telescope Science Institute（太空望远镜科学研究所）；University of Texas at Austin（德克萨斯大学奥斯汀分校）；University of Modena & Reggio Emilia（摩德纳与雷焦艾米利亚大学）；University College London（伦敦大学学院）；Williams College（威廉姆斯学院）
Faint galaxies in the Zone of Avoidance revealed by JWST/NIRCam
Universidad de La Serena（拉塞雷纳大学）；Instituto de Astronomía Teórica y Experimental, (IATE-CONICET)（理论与实验天文研究所）；Observatorio Astronómico de Córdoba, Universidad Nacional de Córdoba（科尔多瓦天文台，科尔多瓦国立大学）；Steward Observatory, University of Arizona（斯图尔德天文台，亚利桑那大学）；Instituto de Investigación en Astronomía y Ciencias Planetarias, Universidad de Atacama（天文学与行星科学研究所，阿塔卡马大学）；Instituto de Astrofísica, Facultad de Ciencias Exactas, Universidad Andrés Bello（天体物理研究所，精确科学学院，安德烈斯·贝略大学）；Vatican Observatory（梵蒂冈天文台）
A Single Line-Emitter Identified in an Unbiased Search with JWST/NIRSpec: Multi-Object Coronagraphy for Slitless Spectroscopy
University of Minnesota（明尼苏达大学）；Stockholm University（斯德哥尔摩大学）；Space Telescope Science Institute（太空望远镜科学研究所）；University of Texas at Austin（德克萨斯大学奥斯汀分校）；University of Modena & Reggio Emilia（摩德纳与雷焦艾米利亚大学）；University College London（伦敦大学学院）；Williams College（威廉姆斯学院）
JWST Advanced Deep Extragalactic Survey (JADES) Data Release 5: NIRCam Imaging in GOODS-S and GOODS-N
Department of Astronomy and Astrophysics, University of California, Santa Cruz（加州大学圣克鲁兹分校天文与天体物理系）；Kavli Institute for Cosmology, University of Cambridge（剑桥大学卡弗里宇宙学研究所）；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）
NGDEEP Epoch 1: Spatially Resolved H$α$ Observations of Disk and Bulge Growth in Star-Forming Galaxies at $z \sim$ 0.6-2.2 from JWST NIRISS Slitless Spectroscopy
Disk-like galaxies at 4 < z < 7.7 : JWST/NIRCam morphologies revealed by denoising VAE-GCNN classification
Center for Cosmology and Astrophysics, Alikhanyan National Laboratory（阿利哈尼扬国家实验室宇宙学与天体物理中心）；Yerevan State University（埃里温国立大学）；SIA, Sapienza University of Rome（罗马智慧大学天体物理研究所）
研究利用去噪VAE-GCNN分类方法分析JWST/NIRCam多滤光片切片，确定红移4 < z < 7.7范围内盘状星系占比为0.34，揭示高红移星系中盘状结构的重要性。
JWST Advanced Deep Extragalactic Survey (JADES) Data Release 5: Catalogs of inferred morphological properties of galaxies from JWST/NIRCam imaging in GOODS-N and GOODS-S
University of California, Santa Cruz（加州大学圣克鲁兹分校）；University of Cambridge（剑桥大学）；University of Arizona（亚利桑那大学）；The University of Texas at Austin（德克萨斯大学奥斯汀分校）；Niels Bohr Institute, University of Copenhagen（哥本哈根大学尼尔斯·玻尔研究所）；Cosmic Dawn Center (DAWN)（宇宙黎明中心）；University of Hertfordshire（赫特福德大学）；The Johns Hopkins University（约翰斯·霍普金斯大学）；University College London（伦敦大学学院）；Space Telescope Science Institute（太空望远镜科学研究所）；NSF National Optical-Infrared Astronomy Research Laboratory（美国国家光学-红外天文研究实验室）
A first look at a complete view of spatially resolved star formation at 1<z<1.8 with JWST NGDEEP+FRESCO slitless spectroscopy
Cosmic Dawn Center（宇宙黎明中心）；Max-Planck-Institut für Astronomie（马克斯·普朗克天文学研究所）；Department of Physics and Astronomy, Texas A&M University（德克萨斯农工大学物理与天文系）；George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, Texas A&M University（德克萨斯农工大学乔治·P和辛西娅·伍兹基础物理与天文研究所）；Centro de Astrobiología (CAB), CSIC-INTA（西班牙国家航空航天技术研究所/西班牙高等科学研究理事会天体生物学中心）；Department of Astronomy, University of Geneva（日内瓦大学天文系）
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）
Assessing the Impact of Source Confusion for GREX-PLUS based on Deep JWST NIRCam Imaging
Institute for Cosmic Ray Research, The University of Tokyo（东京大学宇宙线研究所）；Waseda Research Institute for Science and Engineering, Faculty of Science and Engineering, Waseda University（早稻田大学理工学府理工学研究科理工学研究院）；Department of Pure and Applied Physics, School of Advanced Science and Engineering, Faculty of Science and Engineering, Waseda University（早稻田大学理工学府理工学研究科理工学部应用物理学科）；Department of Astronomy, Kyoto University（京都大学天文学系）；Photocross., Co. Ltd.（Photocross有限公司）
Searching for Extremely Blue UV Continuum Slopes at $z=7-11$ in JWST/NIRCam Imaging: Implications for Stellar Metallicity and Ionizing Photon Escape in Early Galaxies
AGNBoost: A Machine Learning Approach to AGN Identification with JWST/NIRCam+MIRI Colors and Photometry
University of Kansas（堪萨斯大学）；Rochester Institute of Technology（罗切斯特理工学院）；Colby College（科尔比学院）；Space Telescope Science Institute（太空望远镜科学研究所）；NASA-Goddard Space Flight Center（美国宇航局戈达德太空飞行中心）；Texas A&M University（得克萨斯农工大学）
