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| COSMOS2015 711112 , the SIMBAD biblio (35 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST11:09:48 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 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 | 136 | D | X C | 3 | 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 |
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 | 492 | D | X | 13 | 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 | 914 | A | D | S X | 23 | 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. |
|
2018A&A...609A.130L |
2 | 50 | 132 | The [CII] 158 µm line emission in high-redshift galaxies. | LAGACHE G., COUSIN M. and CHATZIKOS M. | ||||
|
2018ApJ...858...77H |
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 | 164 | X F | 3 | 17 | 56 | Alma suggests outflows in z∼ 5.5 galaxies. | GALLERANI S., PALLOTTINI A., FERUGLIO C., et al. | ||
| 2018MNRAS.478.1170C | 179 | D | X | 5 | 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 | 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.487.1689P | 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 | 1681 | D | X C | 41 | 20 | 7 | Low star formation efficiency in typical galaxies at z = 5-6. | PAVESI R., RIECHERS D.A., FAISST A.L., et al. | |
|
2019ApJS..244...40L |
16 | D | 1 | 660 | 51 | Automated mining of the ALMA archive in the COSMOS field (A3COSMOS). I. Robust ALMA continuum photometry catalogs and stellar mass and star formation properties for ∼700 galaxies at z = 0.5-6. | LIU D., LANG P., MAGNELLI B., et al. | ||
| 2019ApJ...886...29S | 44 | X | 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 | 61 | D | X | 2 | 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 | 4 | 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. | ||
| 2020MNRAS.498.4192F | 436 | D | X | 11 | 7 | 58 | ALMA characterizes the dust temperature of z ∼ 5.5 star-forming galaxies. | FAISST A.L., FUDAMOTO Y., OESCH P.A., et al. | |
| 2021MNRAS.502.3210L | 59 | D | X | 2 | 23 | 16 | The IRX-β relation of high-redshift galaxies. | LIANG L., FELDMANN R., HAYWARD C.C., et al. | |
| 2021MNRAS.507.3540J | 351 | D | X F | 8 | 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. | |
| 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...664A..73B |
230 | D | X C | 5 | 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. | ||
| 2023MNRAS.521.2962F | 366 | D | X F | 8 | 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. | |
| 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.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. | ||
| 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. | ||
| 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.535.2068R | 45 | X | 1 | 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 | 90 | C | 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. |