The ALPINE-CRISTAL-JWST Survey: JWST/IFU Optical Observations for 18 Main-sequence Galaxies at  z  = 4–6

Faisst, A. L.; Fujimoto, S.; Tsujita, A.; Wang, W.; Nezhad, N.; Loiacono, F.; Übler, Hannah; Béthermin, M.; Cassata, P.; Dessauges‐Zavadsky, M.; Herrera-Camus, Rodrigo; Schaerer, D.; Silverman, J. D.; Yan, L.; Aravena, M.; Looze, Ilse De; Schreiber, N. M. Förster; González-López, J.; Spilker, Justin; Tadaki, Ken-ichi; Casey, C. M.; Franco, M.; Harish, S.; McCracken, H. J.; Kartaltepe, J. S.; Koekemoer, A. M.; Khostovan, A. A.; Liu, D.; Rhodes, J.; Robertson, B. E.; Amorin, R.; Assef, R. J.; Battisti, A. J.; Birkin, J. E.; Boquien, M.; Cunha, E. Da; Dam, P.; Davies, R. L.; Gómez-Espinoza, D. A.; Ferrara, A.; Fudamoto, Yoshinobu; Gillman, S.; Ginolfi, M.; Gozaliasl, G.; Gruppioni, C.; Hadi, A.; Hathi, Nimish P.; Ibar, E.; Ikeda, R.; Inami, H.; Jones, G. C.; Kohandel, M.; Li, Y.; Lin, Y.-H.; Liu, Z.; Liu, L-J.; Long, A. S.; Magdis, G.; Maraston, Claudia; Martin, C. L.; Mitsuhashi, Ikki; Mobasher, B.; Molina, J.; Nanni, A.; Palla, M.; Pallottini, A.; Pozzi, F.; Relaño, M.; Ren, W.; Riechers, D. A.; Romano, M.; Sanders, D. B.; Sawant, P.; Shuntov, Marko; Smit, R.; Sommovigo, Laura; Talia, M.; Vallini, L.; Veraldi, E.; Vergani, D.; Vijayan, A. P.; Villanueva, V.; Zamorani, G.

doi:10.3847/1538-4365/ae0928

articleThe Astrophysical Journal Supplement SeriesJan 1, 2026GOLD OA

The ALPINE-CRISTAL-JWST Survey: JWST/IFU Optical Observations for 18 Main-sequence Galaxies at z = 4–6

ALA. L. Faisst SFS. Fujimoto ATA. Tsujita WWW. Wang NNN. Nezhad

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Abstract

Abstract To fully characterize the formation and evolution of galaxies, we need to observe their stars, gas, and dust on resolved spatial scales. We present the ALPINE-CRISTAL-JWST survey, which combines kiloparsec-resolved imaging and spectroscopy from the Hubble Space Telescope, JWST, and Atacama Large Millimeter/submillimeter Array for 18 representative main-sequence galaxies at z = 4–6 and log ( M * / M ⊙ ) > 9.5 to study their star formation, chemical properties, and extended gas reservoirs. The cospatial measurements resolving the ionized gas, molecular gas, stars, and dust on 1–2 kpc scales make this a unique benchmark sample for the study of galaxy formation and evolution at z ∼ 5, connecting…

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Keywords

Galaxy
Reionization
Star formation
Galaxy formation and evolution
Active galactic nucleus
COSMIC cancer database
Galaxy merger
Spectroscopy

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