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| [DWV2017b] CFHQ J2100-1715 companion , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST08:20:24 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2017Natur.545..457D | 9 | 8 | 146 | Rapidly star-forming galaxies adjacent to quasars at redshifts exceeding 6. | DECARLI R., WALTER F., VENEMANS B.P., 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. | ||
| 2018ApJ...869L..22W | 809 | X C | 19 | 3 | 18 | No evidence for enhanced [O III] 88 µm emission in a z ∼ 6 quasar compared to its companion starbursting galaxy. | WALTER F., RIECHERS D., NOVAK M., et al. | ||
| 2019ApJ...881..163M | 544 | D | X C | 13 | 21 | ~ | Spectral energy distributions of companion galaxies to z ∼ 6 quasars. | MAZZUCCHELLI C., DECARLI R., FARINA E.P., et al. | |
| 2019ApJ...882...10N | 182 | D | X | 5 | 16 | 51 | Resolved [C II] emission from z > 6 quasar host-companion galaxy pairs. | NEELEMAN M., BANADOS E., WALTER F., et al. | |
|
2019A&A...631A.167D |
125 | X C | 2 | 10 | 32 | A dense, solar metallicity ISM in the z = 4.2 dusty star-forming galaxy SPT 0418-47. | DE BREUCK C., WEISS A., BETHERMIN M., et al. | ||
| 2020ApJ...904..130V | 17 | D | 1 | 54 | 75 | Kiloparsec-scale ALMA imaging of [C II] and dust continuum emission of 27 quasar host galaxies at z ∼ 6. | VENEMANS B.P., WALTER F., NEELEMAN M., et al. | ||
|
2023A&A...679A.131R |
44 | O X | 1 | 138 | ~ | Diagnosing the interstellar medium of galaxies with far-infrared emission lines II. [C II], [O I], [O III], [N II], and [N III] up to z = 6. | RAMOS PADILLA A.F., WANG L., VAN DER TAK F.F.S., et al. | ||
| 2024MNRAS.534.2062V | 18 | D | 2 | 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. |