HSCS J021624-045516 , the SIMBAD biblio

HSCS J021624-045516 , the SIMBAD biblio (8 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST12:57:41


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Title First 3 Authors
2017ApJ...846..134J 16       D               1 40 8 A Magellan M2FS spectroscopic survey of galaxies at 5.5 < z < 6.8: program overview and a sample of the brightest Lyα emitters. JIANG L., SHEN Y., BIAN F., et al.
2018ApJ...859...84H 17       D               1 87 105 SILVERRUSH. V. Census of Lyα, [O III] λ5007, Hα, and [C II] 158 µm line emission with ∼1000 LAEs at z = 4.9-7.0 revealed with Subaru/HSC. HARIKANE Y., OUCHI M., SHIBUYA T., et al.
2018PASJ...70S..10O viz 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.
2018PASJ...70S..15S 17       D               1 104 117 SILVERRUSH. III. Deep optical and near-infrared spectroscopy for Lyα and UV-nebular lines of bright Lyα emitters at z = 6-7. SHIBUYA T., OUCHI M., HARIKANE Y., et al.
2020ApJ...903....4N viz 16       D               1 265 ~ The Magellan M2FS spectroscopic survey of high-redshift galaxies: a sample of 260 Lyα emitters at redshift z ≃ 5.7. NING Y., JIANG L., ZHENG Z.-Y., et al.
2021ApJ...911...78O viz 17       D               1 181 17 SILVERRUSH X: machine learning-aided selection of 9318 LAEs at z = 2.2, 3.3, 4.9, 5.7, 6.6, and 7.0 from the HSC SSP and CHORUS survey data. ONO Y., ITOH R., SHIBUYA T., 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.
2023ApJS..268...24K viz 17       D               1 289 ~ SILVERRUSH. XIII. A Catalog of 20,567 Lyα Emitters at z = 2-7 Identified in the Full-depth Data of the Subaru/HSC-SSP and CHORUS Surveys. KIKUTA S., OUCHI M., SHIBUYA T., et al.

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