The Large-scale Environments of Low-luminosity AGNs at 3.9 &lt; <i>z</i> &lt; 6 and Implications for Their Host Dark Matter Halos from a Complete NIRCam Grism Redshift Survey

Acknowledgements: We thank the anonymous referee for providing constructive comments. We thank Nickolas Kokron, Michael Strauss, and Yin Li for very helpful discussions on the clustering analysis. X.L. and X.F. acknowledge support from the NSF award AST-2308258. F.W. acknowledges support from NSF award AST-2513040. X.L. and Z.C. acknowledge support from the National Key R&D Program of China (grant No. 2023YFA1605600) and Tsinghua University Initiative Scientific Research Program (No. 20223080023). A.J.B. acknowledges funding from the “FirstGalaxies” Advanced Grant from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation program (grant agreement No. 789056). B.E.R. acknowledges support from the NIRCam Science Team contract to the University of Arizona, NAS5-02015, and JWST Program 3215. S.T. acknowledges support by the Royal Society Research grant G125142. C.N.A.W. acknowledges JWST/NIRCam contract to the University of Arizona NAS5-02015. R.M. acknowledges support by the Science and Technology Facilities Council (STFC), by the ERC through Advanced grant 695671 “QUENCH,” and by the UKRI Frontier Research grant RISE and FALL. R.M. also acknowledges funding from a research professorship from the Royal Society. This work is based on observations made with the NASA/ESA Hubble Space Telescope and NASA/ESA/CSA James Webb Space Telescope. 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 program Nos. 1181 (JADES), 1895 (FRESCO), and 3577 (CONGRESS). Support for program No. 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 program with a zero-exclusive-access period.