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| HSCS J221027+030428 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST09:11:14 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2018ApJS..237....5M | 16 | D | 1 | 93 | 82 | Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). IV. Discovery of 41 quasars and luminous galaxies at 5.7 <= z <= 6.9. | MATSUOKA Y., IWASAWA K., ONOUE 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. | ||
|
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. | ||
|
2022ApJS..259...20H |
17 | D | 1 | 1042 | 83 | GOLDRUSH. IV. Luminosity Functions and Clustering Revealed with ∼4,000,000 Galaxies at z ∼ 2-7: Galaxy-AGN Transition, Star Formation Efficiency, and Implication for Evolution at z > 10. | HARIKANE Y., ONO Y., OUCHI M., et al. | ||
| 2022MNRAS.517.1264L | 145 | D | X F | 3 | 94 | 3 | Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) - XV. Constraining the cosmic reionization at 5.5 < z < 7. | LU T.-Y., GOTO T., HASHIMOTO T., et al. | |
| 2023ApJ...949L..42M | 17 | D | 1 | 35 | 5 | Quasar Luminosity Function at z = 7. | MATSUOKA Y., ONOUE M., IWASAWA K., et al. | ||
| 2025ApJ...979..183I | 19 | D | 1 | 73 | ~ | Subaru High-z Exploration of Low-luminosity Quasars (SHELLQs). XXI. Candidate Red Quasars at z ≥ 6 from Near-infrared Photometry. | IWAMOTO R., MATSUOKA Y., IMANISHI M., et al. | ||
| 2025MNRAS.540.1308O | 19 | D | 1 | 72 | ~ | Optical and near-infrared spectroscopy of quasars at z > 6.5: public data release and composite spectrum. | ONORATO S., HENNAWI J.F., SCHINDLER J.-T., et al. |