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Beyond the stars: Linking H α sizes, kinematics, and star formation in galaxies at z ≈ 4−6 with JWST grism surveys and geko

Year: 2025
Type: article
Abstract: Acknowledgements: We thank the referee for the helpful comments that greatly improved the paper. We thank Hannah Übler for the insightful discussions, Pierluigi Rinaldi and William Baker for the helpful comments, and Christopher Lovell, William Roper, and Xuejian (Jacob) Shen for facilitating access to flares and thesan data. ALD thanks the University of Cambridge Harding Distinguished Postgraduate Scholars Programme and Technology Facilities Council (STFC) Center for Doctoral Training (CDT) in Data intensive science at the University of Cambridge (STFC grant number2742605) for a PhD studentship. ALD and ST acknowledge support by the Royal Society Research Grant G125142. WM thanks the Science and Technology Facilities Council (STFC) Center for Doctoral Training (CDT) in Data Intensive Science at the University of Cambridge (STFC grant number 2742968) for a PhD studentship. BER acknowledges support from the NIRCam Science Team contract to the University of Arizona, NAS5-02105, and JWST Program 3215. S.C acknowledges support by European Union’s HE ERC Starting Grant No. 101040227–WINGS. CC acknowledges support from the JWST/NIRCam Science Team contract to the University of Arizona, NAS5-02105, and JWST Program 3215. EE, ZJ, BDJ, MR, CNAW, and YZ acknowledge support from the JWST/NIRCam contract to the University of Arizona NAS5-02105. AJB acknowledge funding from the ’FirstGalaxies’ Advanced Grant from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (Grant agreement no. 789056). ECL acknowledges support of an STFC Webb Fellowship (ST/W001438/1). DJE is supported as a Simons Investigator and by JWST/NIRCam contract to the University of Arizona, NAS5-02105. Support for programme #3215 was provided by NASA through a grant from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5–03127. NCV acknowledges support from the Charles and Julia Henry Fund through the Henry Fellowship. This work is based on observations made with the NASA/ESA Hubble Space Telescope and NASA/ESA/CSA JWST. The data were obtained from the Mikulski Archive for Space Telescopes at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5–03127 for JWST. These observations are associated with programme #1180, 1181, 1210 (JADES), #1895 (FRESCO), # 1963 (JEMS), and #3577 (CONGRESS). Support for programme #3577 was provided by NASA through a grant from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5–03127. The authors acknowledge the FRESCO team for developing their observing programme with a zero-exclusive-access period. The authors acknowledge use of the lux supercomputer at UC Santa Cruz, funded by NSF MRI grant AST 1828315.
Authors: Danhaive, A Lola, Tacchella, Sandro, McClymont, William, Robertson, Brant, Carniani, Stefano, Carreira, Courtney, Egami, Eiichi, Bunker, Andrew J, Curtis-Lake, Emma, Eisenstein, Daniel J, Ji, Zhiyuan, Johnson, Benjamin D, Rieke, Marcia, Villanueva, Natalia C, Willmer, Christopher NA, Willot, Chris, Wu, Zihao, Zhu, Yongda
Institutions: University of Cambridge, University of California, Santa Cruz, Scuola Normale Superiore, University of Oxford, University of Hertfordshire, Center for Astrophysics Harvard & Smithsonian, University of Arizona, Herzberg Institute of Astrophysics
Language: English
Open Access status: green
Funders: National Science Foundation, National Aeronautics and Space Administration, University of California, Santa Cruz, University of Arizona, Space Telescope Science Institute, Science and Technology Facilities Council, H2020 European Research Council
Awards: G1338664626, G1824424381, Star formation in galaxies from the Epoch of Reionisation to the present day with JWST, Finding the most distant galaxies with NIRSpec guaranteed time on the James Webb Space Telescope, G3575130984, Investigating galaxy evolution with radiative transfer simulations and observations, G5568641063, G6464745819, Probing the Cosmic Dawn: a spectroscopic view of the first galaxies, MRI: Acquisition of a High Performance Computer for Computational Science at UC Santa Cruz
OpenAlex ID: W7141782982
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