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| QSO J2201+0302 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST09:49:40 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2016ApJ...819...24W |
16 | D | 1 | 796 | 79 | A survey of luminous high-redshift quasars with SDSS and WISE. I. Target selection and optical spectroscopy. | WANG F., WU X.-B., FAN X., et al. | ||
|
2016ApJ...829...33Y |
16 | D | 1 | 100 | 57 | A survey of luminous high-redshift quasars with SDSS and WISE. II. The bright end of the quasar luminosity function at z ~= 5. | YANG J., WANG F., WU X.-B., et al. | ||
|
2019ApJ...883..163B |
16 | D | 1 | 199 | 41 | The evolution of O I over 3.2 < z < 6.5: reionization of the circumgalactic medium. | BECKER G.D., PETTINI M., RAFELSKI M., et al. | ||
|
2019MNRAS.490.2542P |
16 | D | 1 | 2245 | ~ | Unveiling the weak radio quasar population at z≥4. | PERGER K., FREY S., GABANYI K.E., et al. | ||
|
2020MNRAS.494..789R |
16 | D | 1 | 489 | 25 | The near and mid-infrared photometric properties of known redshift z >= 5 quasars. | ROSS N.P. and CROSS N.J.G. | ||
| 2020ApJ...904..111K | 58 | D | X | 2 | 45 | 26 | The Infrared Medium-deep Survey. VIII. Quasar luminosity function at z ∼ 5. | KIM Y., IM M., JEON Y., et al. | |
|
2021A&A...656A.137G |
17 | D | 1 | 493 | 12 | Low frequency radio properties of the z > 5 quasar population. | GLOUDEMANS A.J., DUNCAN K.J., ROTTGERING H.J.A., et al. | ||
| 2024MNRAS.527.3912L | 18 | D | 1 | 85 | ~ | XQz5: a new ultraluminous z ∼ 5 quasar legacy sample. | LAI S., ONKEN C.A., WOLF C., et al. | ||
| 2025ApJ...983...10O | 19 | D | 2 | 63 | ~ | The Qz5 Survey. I. How the H I Mass Density of the Universe Evolves with Cosmic Time. | OYARZUN G.A., RAFELSKI M., CHRISTENSEN L., et al. | ||
|
2025A&A...698A.145B |
19 | D | 3 | 40 | ~ | Multi-phase investigation of outflows in the circumgalactic and interstellar media of luminous quasars at z ∼ 5. | BRAZZINI M., D'ODORICO V., BISCHETTI M., et al. |