COSMOS2015 494763 , the SIMBAD biblio

COSMOS2015 494763 , the SIMBAD biblio (19 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST20:58:33


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Title First 3 Authors
2012ApJ...760..128M viz 15       D               1 235 51 Lyα emission from high-redshift sources in COSMOS. MALLERY R.P., MOBASHER B., CAPAK P., et al.
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.
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.
2018PASJ...70S..10O viz 16       D               1 365 182 Great Optically Luminous Dropout Research Using Subaru HSC (GOLDRUSH). I. UV luminosity functions at z ∼ 4-7 derived with the half-million dropouts on the 100 deg2 sky. ONO Y., OUCHI M., HARIKANE Y., et al.
2020ApJ...900....1F 18       D               1 46 94 The ALPINE-ALMA [C II] Survey: size of individual star-forming galaxies at z = 4-6 and their extended halo structure. FUJIMOTO S., SILVERMAN J.D., BETHERMIN M., et al.
2020A&A...643A...1L 17       D               1 77 137 The ALPINE-ALMA [CII] survey. Survey strategy, observations, and sample properties of 118 star-forming galaxies at 4 < z < 6. LE FEVRE O., BETHERMIN M., FAISST A., et al.
2020A&A...643A...2B viz 17       D               1 124 139 The ALPINE-ALMA [CII] survey: Data processing, catalogs, and statistical source properties. BETHERMIN M., FUDAMOTO Y., GINOLFI M., et al.
2020A&A...643A...4F viz 16       D               1 117 75 The ALPINE-ALMA [CII] survey. Dust attenuation properties and obscured star formation at z ∼ 4.4-5.8. FUDAMOTO Y., OESCH P.A., FAISST A., et al.
2020A&A...643A...6C viz 16       D               1 55 34 The ALPINE-ALMA [CII] survey. Small Lyα-[CII] velocity offsets in main-sequence galaxies at 4.4 < z < 6. CASSATA P., MORSELLI L., FAISST A., et al.
2022A&A...664A..73B viz 17       D               1 113 8 The ALMA-ALPINE [CII] survey. The star formation history and the dust emission of star-forming galaxies at 4.5 < z < 6.2. BURGARELLA D., BOGDANOSKA J., NANNI A., et al.
2024A&A...690A.197M 18       D               1 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.
2024ApJ...976...70L 108       D         F     8 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..34V 19       D               1 47 ~ The ALPINE-ALMA [CII] Survey: Modelling ALMA and JWST lines to constrain the interstellar medium of z∼ 5 galaxies Connecting UV, optical, and far-infrared line emission. VERALDI E., VALLINI L., POZZI F., et al.
2025A&A...693A.237I 19       D               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 19       D               2 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...701A.260L 392       D     X C       8 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.
2025A&A...702A.206A 19       D               2 13 ~ The ALPINE-CRISTAL-JWST survey: Spatially resolved star formation relations at z ∼ 5. ACCARD C., BETHERMIN M., BOQUIEN M., et al.
2026ApJS..282...19F 320       D     X         7 20 ~ 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., et al.
2026ApJ...997..319T 20       D               1 21 ~ The ALPINE-CRISTAL-JWST Survey: Stellar and Nebular Dust Attenuation of Main-sequence Galaxies at z ∼ 4-6. TSUJITA A., FUJIMOTO S., FAISST A., et al.

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