[MOK2016b] HSC J120103.02+013356.4 , the SIMBAD biblio

[MOK2016b] HSC J120103.02+013356.4 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST23:26:18


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Title First 3 Authors
2018ApJ...869..150M 17       D               1 111 151 Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). V. Quasar luminosity function and contribution to cosmic reionization at z = 6. MATSUOKA Y., STRAUSS M.A., KASHIKAWA N., et al.
2018PASJ...70S..35M 17       D               1 66 104 Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). II. Discovery of 32 quasars and luminous galaxies at 5.7 < z ≤ 6.8. MATSUOKA Y., ONOUE M., KASHIKAWA N., 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...908..124L 17       D               1 38 28 Constraining the quasar radio-loud fraction at z ∼ 6 with deep radio observations. LIU Y., WANG R., MOMJIAN E., 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.
2024ApJ...960..112T 134           X   F     2 13 ~ Subaru High-z Exploration of Low-luminosity Quasars (SHELLQs). XVII. Black Hole Mass Distribution at z ∼ 6 Estimated via Spectral Comparison with Low-z Quasars. TAKAHASHI A., MATSUOKA Y., ONOUE M., et al.
2025MNRAS.539.2039H 112       D         F     3 26 ~ Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) - XXIII. The powering mechanisms of the Lyα haloes around high-z quasars probed by slit spectroscopy. HOSHI H., ISHIMOTO R., KASHIKAWA N., et al.

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