HSCS J100401+023930 , the SIMBAD biblio

HSCS J100401+023930 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST10:40:39


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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.
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.
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.
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.
2022ApJS..259...20H viz 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.
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.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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