The ALPINE-CRISTAL-JWST Survey: Gas-phase abundance gradients of main sequence star-forming galaxies and their kinematics at $4 < z < 6$ Lilian L. Lee, Natascha M. F"orster Schreiber, Seiji Fujimoto, Andreas L. Faisst, Rodrigo Herrera-Camus, Reinhard Genzel, Linda J. Tacconi, Dieter Lutz, Alvio Renzini, Ryan Sanders, Emily Wisnioski, Stijn Wuyts, Eleonora Parlanti, Gareth Jones, Hannah "Ubler, Daizhong Liu, Jianhang Chen, Ric I. Davies, Giulia Tozzi, Andreas Burkert, Sedona H. Price, Manuel Aravena, M'ed'eric Boquien, Matthieu B'ethermin, Elisabete da Cunha, Rebecca L. Davies, Ilse De Looze, Miroslava Dessauges-Zavadsky, Andrea Ferrara, Deanne B. Fisher, Steven Gillman, Michele Ginolfi, Edo Ibar, Anton M. Koekemoer, Juan Molina, Thorsten Naab, M'onica Rela~no, Dominik A. Riechers, David B. Sanders, Justin S. Spilker, Livia Vallini, Giovanni Zamorani, Ambra Nanni, Poulomi Dam, Tanio Diaz-Santos, Diego G'omez-Espinoza, Ali Hadi, Ryota Ikeda, Ana Posses, Michael Romano, Amiel Sternberg, Vicente Villanueva, Wuji Wang arXiv:2603.13493v2 Announce Type: replace Abstract: We present gas-phase radial metallicity profiles for 20 main-sequence galaxies at $40.05{rm dexkpc^{-1}}$ at $1sigma$, and none have a significant negative gradient. We investigated the correlation between the metallicity gradients and the intrinsic gas velocity dispersion $sigma_0$ as well as the $V_{rm rot}/sigma_0$ ratio of the disks. Combining our sample with mass-matched literature samples at $3arXiv:2603.13493v2 Announce Type: replace
Abstract: We present gas-phase radial metallicity profiles for 20 main-sequence galaxies at $40.05{rm dexkpc^{-1}}$ at $1sigma$, and none have a significant negative gradient. We investigated the correlation between the metallicity gradients and the intrinsic gas velocity dispersion $sigma_0$ as well as the $V_{rm rot}/sigma_0$ ratio of the disks. Combining our sample with mass-matched literature samples at $3