COSMOS2015 848185 , the SIMBAD biblio

COSMOS2015 848185 , the SIMBAD biblio (68 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST20:04:15


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Title First 3 Authors
2011Natur.470..233C 7 15 235 A massive protocluster of galaxies at a redshift of z ∼ 5.3. CAPAK P.L., RIECHERS D., SCOVILLE N.Z., et al.
2013ApJS..206....8M viz 15       D               1 208367 332 A public Ks-selected catalog in the COSMOS/ULTRAVISTA field: photometry, photometric redshifts, and stellar population parameters. MUZZIN A., MARCHESINI D., STEFANON M., et al.
2014ApJ...796...84R 41           X         1 30 164 ALMA imaging of gas and dust in a galaxy protocluster at redshift 5.3: [C II] emission in "typical" galaxies and dusty starbursts ~1 billion years after the Big Bang. RIECHERS D.A., CARILLI C.L., CAPAK P.L., 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.
2016ApJ...832..151P 1985       D S   X C       49 12 67 ALMA reveals weak [N II] emission in "typical" galaxies and intense starbursts at z = 5-6. PAVESI R., RIECHERS D.A., CAPAK P.L., et al.
2017ApJ...834L..16U 40           X         1 11 11 ALMA reveals strong [C II] emission in a galaxy embedded in a giant Lyα blob at z = 3.1. UMEHATA H., MATSUDA Y., TAMURA Y., et al.
2017ApJ...845...41B 255       D     X C       6 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 572       D     X         15 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.
2017ApJ...850..180J 80           X         2 19 47 Dynamical characterization of galaxies at z ∼ 4-6 via tilted ring fitting to ALMA [C II] observations. JONES G.C., CARILLI C.L., SHAO Y., et al.
2017MNRAS.471.5018F 81           X         2 5 23 The infrared-dark dust content of high redshift galaxies. FERRARA A., HIRASHITA H., OUCHI M., 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.477..552B 53           X         1 7 92 Dusty galaxies in the Epoch of Reionization: simulations. BEHRENS C., PALLOTTINI A., FERRARA A., et al.
2018MNRAS.473.1909G 324           X C F     6 17 56 Alma suggests outflows in z∼ 5.5 galaxies. GALLERANI S., PALLOTTINI A., FERUGLIO C., et al.
2018MNRAS.478.1170C 219       D     X         6 41 108 Kiloparsec-scale gaseous clumps and star formation at z = 5-7. CARNIANI S., MAIOLINO R., AMORIN R., et al.
2018ApJ...861...95H 42           X         1 32 76 SHINING, a survey of far-infrared lines in nearby galaxies. II. Line-deficit models, AGN impact, [C II]-SFR scaling relations, and mass-metallicity relation in (U)LIRGs. HERRERA-CAMUS R., STURM E., GRACIA-CARPIO J., et al.
2018A&A...617A.131S 321           X         8 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.487.1689P 86               F     1 15 87 Deep into the structure of the first galaxies: SERRA views. PALLOTTINI A., FERRARA A., DECATALDO D., 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...882..168P 3103       D     X C       76 20 7 Low star formation efficiency in typical galaxies at z = 5-6. PAVESI R., RIECHERS D.A., FAISST A.L., 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 183       D     X C       4 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.
2020ApJS..247...61F 130           X         3 13 91 The ALPINE-ALMA [C II] Survey: multiwavelength ancillary data and basic physical measurements. FAISST A.L., SCHAERER D., LEMAUX B.C., 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.
2020MNRAS.494.4090C 82             C       1 41 16 The [C II]/[N II] ratio in 3 < z < 6 sub-millimetre galaxies from the South Pole Telescope survey. CUNNINGHAM D.J.M., CHAPMAN S.C., ARAVENA 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.
2020MNRAS.495L..22V 82           X         2 5 ~ Star formation law in the epoch of reionization from [C II] and C III] lines. VALLINI L., FERRARA A., PALLOTTINI A., 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.
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.
2020MNRAS.498.4192F 1300       D     X C       31 7 58 ALMA characterizes the dust temperature of z ∼ 5.5 star-forming galaxies. FAISST A.L., FUDAMOTO Y., OESCH P.A., 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...3S 49           X         1 10 89 The ALPINE-ALMA [C II] survey. Little to no evolution in the [C II]-SFR relation over the last 13 Gyr. SCHAERER D., GINOLFI M., BETHERMIN 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.
2020A&A...643A...7G 45           X         1 6 27 The ALPINE-ALMA [CII] survey. Circumgalactic medium pollution and gas mixing by tidal stripping in a merging system at z ∼ 4.57. GINOLFI M., JONES G.C., BETHERMIN M., et al.
2021A&A...646A..76L 270       D     X C       6 18 44 The ALPINE-ALMA [C II] survey. Luminosity function of serendipitous [C II] line emitters at z ∼ 5. LOIACONO F., DECARLI R., GRUPPIONI C., et al.
2021MNRAS.502.2757O 84           X         2 5 ~ Massive black holes in high-redshift Lyman Break Galaxies. OROFINO M.C., FERRARA A. and GALLERANI S.
2021MNRAS.502.3210L 100       D     X         3 23 16 The IRX-β relation of high-redshift galaxies. LIANG L., FELDMANN R., HAYWARD C.C., et al.
2021A&A...653A..84P 17       D               1 26 15 The ALPINE-ALMA [CII] survey. Dust mass budget in the early Universe. POZZI F., CALURA F., FUDAMOTO Y., et al.
2021MNRAS.507.3540J 226       D     X   F     5 37 27 The ALPINE-ALMA [C II] Survey: kinematic diversity and rotation in massive star-forming galaxies at z ∼ 4.4-5.9. JONES G.C., VERGANI D., ROMANO M., et al.
2022ApJ...925...34C viz 17       D               1 208670 12 Diagnosing DASH: A Catalog of Structural Properties for the COSMOS-DASH Survey. CUTLER S.E., WHITAKER K.E., MOWLA L.A., et al.
2022A&A...660A.137G viz 3193     A D S   X C       74 21 3 Tomography of the environment of the COSMOS/AzTEC-3 submillimeter galaxy at z ∼ 5.3 revealed by Lyα and MUSE observations. GUAITA L., ARAVENA M., GURUNG-LOPEZ S., et al.
2022MNRAS.513.3122S 18       D               1 30 49 The ALMA REBELS Survey: cosmic dust temperature evolution out to z ∼ 7. SOMMOVIGO L., FERRARA A., PALLOTTINI A., et al.
2022A&A...663A..50B 17       D               1 27 6 The ALPINE-ALMA [C II] survey. Dust attenuation curves at z = 4.4-5.5. BOQUIEN M., BUAT V., BURGARELLA D., et al.
2022A&A...664A..73B viz 17       D               4 113 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.
2022MNRAS.516.1612H 17       D               1 10 6 Analytic models of dust temperature in high-redshift galaxies. HIRASHITA H. and CHIANG I.-D.
2022MNRAS.517.5930S 358       D     X C F     7 27 10 A new look at the infrared properties of z ∼ 5 galaxies. SOMMOVIGO L., FERRARA A., CARNIANI S., et al.
2022ApJ...941...74O 639           X C       14 11 ~ ALMA Observations of CO Emission from Luminous Lyman-break Galaxies at z = 6.0293-6.2037. ONO Y., FUJIMOTO S., HARIKANE Y., et al.
2023MNRAS.521.2962F 409       D     X   F     9 9 7 Estimating dust temperature and Far-IR luminosity of high-redshift galaxies using ALMA single-band continuum observations. FUDAMOTO Y., INOUE A.K. and SUGAHARA Y.
2024MNRAS.527.5808B 45           X         1 63 ~ The ALMA REBELS survey: obscured star formation in massive Lyman-break galaxies at z= 4-8 revealed by the IRX-β and M⋆ relations. BOWLER R.A.A., INAMI H., SOMMOVIGO L., et al.
2024MNRAS.527.6867A 18       D               1 21 ~ Cold dust and low [O III]/[C II] ratios: an evolved star-forming population at redshift 7. ALGERA H.S.B., INAMI H., SOMMOVIGO L., et al.
2024A&A...686A.187P 18       D               1 14 ~ The ALPINE-ALMA [CII] survey: Dust emission effective radius up to 3 kpc in the early Universe. POZZI F., CALURA F., D'AMATO Q., et al.
2024ApJ...971..161M 18       D               2 39 ~ SERENADE. II. An ALMA Multiband Dust Continuum Analysis of 28 Galaxies at 5 < z < 8 and the Physical Origin of the Dust Temperature Evolution. MITSUHASHI I., HARIKANE Y., BAUER F.E., et al.
2024MNRAS.534.2062V 45           X         1 72 ~ Characterising the contribution of dust-obscured star formation at ≳ 5 using 18 serendipitously identified [C II] emitters. VAN LEEUWEN I.F., BOUWENS R.J., VAN DER WERF P.P., 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     10 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 345       D     X         8 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 513     A D     X C       11 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.336B 93             C       1 10 ~ CEERS: Possibly forging the first dust grains in the universe A population of galaxies with spectroscopically derived extremely low dust attenuation (GELDA) at 4.0 < z ≲ 11.4. BURGARELLA D., BUAT V., THEULE P., 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.
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.
2025MNRAS.544..211R 905       D     X C F     18 10 ~ The ALPINE-CRISTAL-JWST survey: revealing less massive black holes in high-redshift galaxies. REN W., SILVERMAN J.D., FAISST A.L., et al.
2026ApJS..282...19F 570       D     X         12 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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