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| HSCS J120754-000553 , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST08:30:03 |
Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
More on score
| 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...828...26M | 19 | D | 4 | 25 | 167 | Subaru high-z exploration of low-luminosity quasars (SHELLQs). I. Discovery of 15 quasars and bright galaxies at 5.7 < z < 6.9. | MATSUOKA Y., ONOUE M., KASHIKAWA N., et al. | ||
2016ApJS..227...11B 
|
16 | D | 1 | 173 | 283 | The Pan-STARRS1 distant z > 5.6 quasar survey: more than 100 quasars within the first Gyr of the Universe. | BANADOS E., VENEMANS B.P., DECARLI R., et al. | ||
|
2018PASJ...70S..10O
|
16 | D | 1 | 365 | 182 | Great Optically Luminous Dropout Research Using Subaru HSC (GOLDRUSH). I. UV luminosity functions at z ∼ 4-7 derived with the half-million dropouts on the 100 deg2 sky. | ONO Y., OUCHI M., HARIKANE Y., 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 | 102 | D | F | 2 | 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. |
