COSMOS2015 547226 , the SIMBAD biblio

COSMOS2015 547226 , the SIMBAD biblio (31 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST18:29:28

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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
2013A&A...556A..55I viz 15       D               1 259207 819 Mass assembly in quiescent and star-forming galaxies since z ≃ 4 from UltraVISTA. ILBERT O., McCRACKEN H.J., LE FEVRE O., et al.
2015Natur.522..455C 12 15 368 Galaxies at redshifts 5 to 6 with systematically low dust content and high [C II] emission. CAPAK P.L., CARILLI C., JONES G., et al.
2017ApJ...845...41B 17       D               1 13 26 Dust properties of C II detected z ∼ 5.5 galaxies: new HST/WFC3 near-IR observations. BARISIC I., FAISST A.L., CAPAK P.L., et al.
2017ApJ...846..105O viz 17       D               2 36 76 SIGAME simulations of the [C II], [O I] and [O III] line emission from star-forming galaxies at z ~= 6. OLSEN K., GREVE T.R., NARAYANAN D., et al.
2017ApJ...847...21F 175       D     X         5 47 93 Are high-redshift galaxies hot? Temperature of z > 5 galaxies and implications for their dust properties. FAISST A.L., CAPAK P.L., YAN L., et al.
2018A&A...609A.130L viz 2 50 132 The [CII] 158 µm line emission in high-redshift galaxies. LAGACHE G., COUSIN M. and CHATZIKOS M.
2018ApJ...858...77H viz 16       D               1 7945 125 The DEIMOS 10k spectroscopic survey catalog of the COSMOS field. HASINGER G., CAPAK P., SALVATO M., et al.
2018ApJ...859...84H 17       D               1 87 105 SILVERRUSH. V. Census of Lyα, [O III] λ5007, Hα, and [C II] 158 µm line emission with ∼1000 LAEs at z = 4.9-7.0 revealed with Subaru/HSC. HARIKANE Y., OUCHI M., SHIBUYA T., et al.
2018MNRAS.473.1909G 123           X   F     2 17 56 Alma suggests outflows in z∼ 5.5 galaxies. GALLERANI S., PALLOTTINI A., FERUGLIO C., et al.
2018MNRAS.478.1170C 18       D               3 41 108 Kiloparsec-scale gaseous clumps and star formation at z = 5-7. CARNIANI S., MAIOLINO R., AMORIN R., et al.
2018A&A...617A.131S 241           X         6 16 2 "Zombie" or active? An alternative explanation to the properties of star-forming galaxies at high redshift. SATURNI F.G., MANCINI M., PEZZULLI E., et al.
2019MNRAS.487.3007K 18       D               2 26 66 Kinematics of z >= 6 galaxies from [C II] line emission. KOHANDEL M., PALLOTTINI A., FERRARA A., et al.
2019ApJ...886...29S 19       D               1 10 34 Fast outflows identified in early star-forming galaxies at z = 5-6. SUGAHARA Y., OUCHI M., HARIKANE Y., et al.
2019ApJ...887..107F 20       D               1 20 93 First identification of 10 kpc [C II] 158 µm halos around star-forming galaxies at z = 5-7. FUJIMOTO S., OUCHI M., FERRARA A., et al.
2020MNRAS.494.1071G 100       D         F     2 54 62 The assembly of dusty galaxies at z >= 4: statistical properties. GRAZIANI L., SCHNEIDER R., GINOLFI M., et al.
2020A&A...637A..32B 16       D               3 50 30 Observational and theoretical constraints on the formation and early evolution of the first dust grains in galaxies at 5 < z < 10. BURGARELLA D., NANNI A., HIRASHITA H., et al.
2020ApJ...896...93H 18       D               1 50 106 Large population of ALMA galaxies at z > 6 with very high [O III] 88 µm to [C II] 158 µm flux ratios: evidence of extremely high ionization parameter or PDR deficit? HARIKANE Y., OUCHI M., INOUE A.K., et al.
2021MNRAS.502.3210L 17       D               1 23 16 The IRX-β relation of high-redshift galaxies. LIANG L., FELDMANN R., HAYWARD C.C., et al.
2022ApJS..259...20H viz 17       D               1 1042 83 GOLDRUSH. IV. Luminosity Functions and Clustering Revealed with ∼4,000,000 Galaxies at z ∼ 2-7: Galaxy-AGN Transition, Star Formation Efficiency, and Implication for Evolution at z > 10. HARIKANE Y., ONO Y., OUCHI M., et al.
2023MNRAS.518.3183L 1594     A     X C       36 4 6 An extended [C II] halo around a massive star-forming galaxy at z = 5.3. LAMBERT T.S., POSSES A., ARAVENA M., et al.
2023A&A...673A.153P 192       D       C F     4 13 1 ALMA hints at the presence of turbulent disk galaxies at z > 5. PARLANTI E., CARNIANI S., PALLOTTINI A., et al.
2024MNRAS.528..499L 18       D               1 192 ~ [C II] 158 μm emission as an indicator of galaxy star formation rate. LIANG L., FELDMANN R., MURRAY N., et al.
2024A&A...684A..23T 358           X C       7 4 ~ Fitting pseudo-Sérsic (Spergel) light profiles to galaxies in interferometric data: The excellence of the uυ-plane. TAN Q.-H., DADDI E., DE SOUZA MAGALHAES V., et al.
2024A&A...690A.197M 63       D     X         2 26 ~ The ALMA-CRISTAL survey Widespread dust-obscured star formation in typical star-forming galaxies at z = 4-6. MITSUHASHI I., TADAKI K.-I., IKEDA R., et al.
2024MNRAS.535.2068R 90           X         2 12 ~ REBELS-25: discovery of a dynamically cold disc galaxy at z = 7.31. ROWLAND L.E., HODGE J., BOUWENS R., et al.
2024A&A...691A.133V 45           X         1 11 ~ The ALMA-CRISTAL survey: Dust temperature and physical conditions of the interstellar medium in a typical galaxy at z = 5.66. VILLANUEVA V., HERRERA-CAMUS R., GONZALEZ-LOPEZ J., et al.
2024ApJ...976...70L 421       D     X   F     9 18 ~ The ALMA-CRISTAL Survey: Spatially Resolved Star Formation Activity and Dust Content in 4 < z < 6 Star-forming Galaxies. LI J., DA CUNHA E., GONZALEZ-LOPEZ J., et al.
2025A&A...693A.237I 205       D     X         5 33 ~ The ALMA-CRISTAL Survey Spatial extent of [C II] line emission in star-forming galaxies at z = 4-6. IKEDA R., TADAKI K.-I., MITSUHASHI I., et al.
2025ApJ...985..243B 47           X         1 24 ~ The ALMA-CRISTAL Survey: Weak Evidence for Star-formation-driven Outflows in z ∼ 5 Main-sequence Galaxies. BIRKIN J.E., SPILKER J.S., HERRERA-CAMUS R., et al.
2025A&A...699A.256P 47           X         1 5 ~ The ALMA-CRISTAL survey: Extended [CII] emission in an interacting galaxy system at z ∼ 5.5. POSSES A., ARAVENA M., GONZALEZ-LOPEZ J., et al.
2025A&A...701A.260L 19       D               2 39 ~ The ALMA-CRISTAL survey: Resolved kinematic studies of main sequence star-forming galaxies at 4 < z < 6. LEE L.L., FORSTER SCHREIBER N.M., HERRERA-CAMUS R., et al.

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