[MOK2016b] HSC J114658.89-000537.7 , the SIMBAD biblio

[MOK2016b] HSC J114658.89-000537.7 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST10:27:27


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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 viz 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 viz 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.
2021ApJ...919...61O 44           X         1 6 13 Subaru high-z exploration of low-luminosity quasars (SHELLQs). XIV. A candidate Type II quasar at z = 6.1292. ONOUE M., MATSUOKA Y., KASHIKAWA N., et al.
2021A&A...656A.137G viz 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.
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.
2025ApJ...988...57M 1232       D     X C       26 14 ~ SHELLQs. Bridging the Gap: JWST Unveils Obscured Quasars in the Most Luminous Galaxies at z > 6. MATSUOKA Y., ONOUE M., IWASAWA K., et al.
2025ApJ...993...91D 532       D     X C       11 13 ~ SHELLQs-JWST Unveils the Host Galaxies of 12 Quasars at z > 6. DING X., ONOUE M., SILVERMAN J.D., et al.
2025ApJ...995L..67S 47           X         1 6 ~ SHELLQs-JWST Perspective on the Intrinsic Mass Relation between Supermassive Black Holes and Their Host Galaxies at z > 6. SILVERMAN J.D., LI J., DING X., et al.
2026A&A...706A.305I 50           X         1 5 ~ Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) XXII. Chandra observations of narrow-line quasar candidates at z ≥ 6. IWASAWA K., GILLI R., VITO F., et al.

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