ZFOURGE COSMOS 20133 , the SIMBAD biblio

ZFOURGE COSMOS 20133 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST21:01:56


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Title First 3 Authors
2014ApJS..214...24S viz 15       D               1 97940 733 3D-HST WFC3-selected photometric catalogs in the five CANDELS/3D-HST fields: photometry, photometric redshifts, and stellar masses. SKELTON R.E., WHITAKER K.E., MOMCHEVA I.G., et al.
2016ApJ...830...51S viz 16       D               1 67525 168 The FourStar galaxy evolution survey (ZFOURGE): ultraviolet to far-infrared catalogs, medium-bandwidth photometric redshifts with improved accuracy, stellar masses, and confirmation of quiescent galaxies to z ∼ 3.5. STRAATMAN C.M.S., SPITLER L.R., QUADRI R.F., et al.
2017ApJS..228....7N viz 16       D               1 37352 95 CANDELS multi-wavelength catalogs: source identification and photometry in the CANDELS COSMOS Survey Field. NAYYERI H., HEMMATI S., MOBASHER B., et al.
2018A&A...618A..85S viz 21       D               2 24 140 Near infrared spectroscopy and star-formation histories of 3 ≤ z ≤ 4 quiescent galaxies. SCHREIBER C., GLAZEBROOK K., NANAYAKKARA T., et al.
2020ApJ...893...23G 82               F     1 11 ~ MOSEL survey: tracking the growth of massive galaxies at 2 < z < 4 using kinematics and the IllustrisTNG simulation. GUPTA A., TRAN K.-V., COHN J., et al.
2023MNRAS.519..980G 87               F     1 20 2 MOSEL survey: extremely weak outflows in EoR analogues at z = 3-4. GUPTA A., TRAN K.-V., MENDEL T., et al.
2024MNRAS.531.3187M 242       D     X   F     5 30 ~ The origin of large emission line widths in massive galaxies at redshifts z ∼ 3-4. MARTINEZ-MARIN M., GLAZEBROOK K., NANAYAKKARA T., et al.
2025ApJ...981...78N 299       D     X         7 22 ~ The Formation Histories of Massive and Quiescent Galaxies in the 3 < z < 4.5 Universe. NANAYAKKARA T., GLAZEBROOK K., SCHREIBER C., et al.
2026ApJ...997...29K 820       D     X C       16 24 ~ Connecting Environment, Star Formation History, and Morphology of Massive Quiescent Galaxies at 3 < z < 4 with JWST. KAWINWANICHAKIJ L., GLAZEBROOK K., NANAYAKKARA T., et al.
2026ApJ..1000...59M 200           X         4 10 ~ Counting Little Red Dots at z < 4 with Ground-based Surveys and Spectroscopic Follow-up. MA Y., GREENE J.E., SETTON D.J., et al.

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