[FBF2023] CEERS2 1298 , the SIMBAD biblio

[FBF2023] CEERS2 1298 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST19:32:49

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
2023ApJ...946L..13F 195       D     X         5 38 132 CEERS Key Paper. I. An Early Look into the First 500 Myr of Galaxy Formation with JWST. FINKELSTEIN S.L., BAGLEY M.B., FERGUSON H.C., et al.
2023Natur.616..266L 24       D               1 18 142 A population of red candidate massive galaxies ∼600 Myr after the Big Bang. LABBE I., VAN DOKKUM P., NELSON E., et al.
2023ApJ...955L..12B 61       D     X         2 13 ~ Sizes and Mass Profiles of Candidate Massive Galaxies Discovered by JWST at 7 < z < 9: Evidence for Very Early Formation of the Central ∼100 pc of Present-day Ellipticals. BAGGEN J.F.W., VAN DOKKUM P., LABBE I., et al.
2024MNRAS.527.1381T 18       D               1 9 ~ Excess of high-z galaxies as a test for bumpy power spectrum of density perturbations. TKACHEV M.V., PILIPENKO S.V., MIKHEEVA E.V., et al.
2024MNRAS.530.2935D 18       D               1 36 ~ ΛCDM not dead yet: massive high-z Balmer break galaxies are less common than previously reported. DESPREZ G., MARTIS N.S., ASADA Y., et al.
2024PASJ...76..219O viz 18       D               1 173 ~ Census for the rest-frame optical and UV morphologies of galaxies at z = 4-10: First phase of inside-out galaxy formation. ONO Y., HARIKANE Y., OUCHI M., et al.
2024ApJ...969L...2F 18       D               1 95 ~ The Complete CEERS Early Universe Galaxy Sample: A Surprisingly Slow Evolution of the Space Density of Bright Galaxies at z ∼ 8.5-14.5. FINKELSTEIN S.L., LEUNG G.C.K., BAGLEY M.B., et al.
2024ApJ...970...63L 18       D               3 13 ~ Age of Massive Galaxies at Redshift 8. LOPEZ-CORREDOIRA M., MELIA F., WEI J.-J., et al.
2025ApJ...978...89H 93           X         2 18 ~ EPOCHS. IV. SED Modeling Assumptions and Their Impact on the Stellar Mass Function at 6.5 ≤ z ≤ 13.5 Using PEARLS and Public JWST Observations. HARVEY T., CONSELICE C.J., ADAMS N.J., et al.

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