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| [CDC2018] C-J0305 , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST11:09:23 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2018ApJ...867..153C | 16 | D | 1 | 54 | 13 | No evidence for millimeter continuum source overdensities in the environments of z >= 6 quasars. | CHAMPAGNE J.B., DECARLI R., CASEY C.M., et al. | ||
| 2019ApJ...874L..30V | 186 | D | X C | 4 | 7 | 49 | 400 pc imaging of a massive quasar host galaxy at a redshift of 6.6. | VENEMANS B.P., NEELEMAN M., WALTER F., 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. | ||
| 2022ApJ...930...27L | 1251 | D | X C | 29 | 9 | 7 | Spatially Resolved Molecular Interstellar Medium in a z = 6.6 Quasar Host Galaxy. | LI J., VENEMANS B.P., WALTER F., et al. | |
| 2023ApJ...951L...4W | 261 | X C | 5 | 8 | 4 | A SPectroscopic Survey of Biased Halos in the Reionization Era (ASPIRE): JWST Reveals a Filamentary Structure around a z = 6.61 Quasar. | WANG F., YANG J., HENNAWI J.F., 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. | ||
| 2025ApJ...980...20M | 159 | D | X F | 3 | 12 | ~ | Pushing the Atacama Large Millimeter/submillimeter Array to the Limit: 140 pc Resolution Observations of a z = 6.6 Quasar-Galaxy Merger Resolve Strikingly Different Morphologies of Dust Continuum and [C II] 158 μm Emission. | MEYER R.A., VENEMANS B., NEELEMAN M., et al. | |
| 2025ApJ...982...72S | 47 | X | 1 | 12 | ~ | Direct Evidence for Active Galactic Nuclei Feedback from Fast Molecular Outflows in Reionization-era Quasars. | SPILKER J.S., CHAMPAGNE J.B., FAN X., et al. |