NAME MOM-z14 , the SIMBAD biblio

NAME MOM-z14 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST16:52:28


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Title First 3 Authors
2025ApJ...991...24B 47           X         1 27 ~ Discovery of SiC and Iron Dust around AGB Stars in the Very Metal-poor Sextans a Dwarf Galaxy with JWST: Implications for Dust Production at High Redshift. BOYER M.L., SLOAN G.C., NANNI A., et al.
2025ApJ...991..179P 93           X         2 5 ~ The Rise of the Galactic Empire: Ultraviolet Luminosity Functions at z ∼ 17 and z ∼ 25 Estimated with the MIDIS+NGDEEP Ultra-deep JWST/NIRCam Data Set. PEREZ-GONZALEZ P.G., OSTLIN G., COSTANTIN L., et al.
2025ApJ...992..212W 140           X         3 11 ~ JADES-GS-z14-1: A Compact, Faint Galaxy at z ≈ 14 with Weak Metal Lines from Extremely Deep JWST MIRI, NIRCam, and NIRSpec Observations. WU Z., EISENSTEIN D.J., JOHNSON B.D., et al.
2025MNRAS.541.3606T 19       D               1 16 ~ Bridging theory and observations: insights into star formation efficiency and dust attenuation in z > 5 Galaxies. TOYOUCHI D., YAJIMA H., FERRARA A., et al.
2025ApJS..281...50E 47           X         1 5 ~ The JADES Origins Field: A New JWST Deep Field in the JADES Second NIRCam Data Release. EISENSTEIN D.J., JOHNSON B.D., ROBERTSON B., et al.
2025ApJ...995...21T 47           X         1 10 ~ Discovery of a Little Red Dot Candidate at z ≳ 10 in COSMOS-web Based on MIRI-NIRCam Selection. TANAKA T.S., AKINS H.B., HARIKANE Y., et al.
2026ApJ...996..115A 50           X         1 15 ~ Earliest Galaxy Evolution in the CANUCS+Technicolor Fields: Galaxy Properties at z ∼ 10-16 Seen with the Full NIRCam Medium- and Broadband Filters. ASADA Y., WILLOTT C.J., MUZZIN A., et al.
2026A&A...705A.171V 50           X         1 2 ~ The z = 9.625 Cosmic Gems galaxy was a compact “blue monster” propelled by massive star clusters. VANZELLA E., MESSA M., ADAMO A., et al.
2026A&A...707A..71V 50           X         1 4 ~ Efficient black hole seed formation in low-metallicity and dense stellar clusters with implications for JWST sources. VERGARA M.C., ASKAR A., FLAMMINI DOTTI F., et al.

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