HSCS J021827-043507 , the SIMBAD biblio

HSCS J021827-043507 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST20:07:59


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Title First 3 Authors
2010ApJ...723..869O 30       D               1 18 563 Statistics of 207 Lyα emitters at a redshift near 7: constraints on reionization and galaxy formation models. OUCHI M., SHIMASAKU K., FURUSAWA H., et al.
2014ApJ...795....5O 54       D     X         2 36 59 Faint submillimeter galaxies revealed by multifield deep ALMA observations: number counts, spatial clustering, and a dark submillimeter line emitter. ONO Y., OUCHI M., KURONO Y., et al.
2016ApJS..222....1F viz 80           X         2 40 108 ALMA census of faint 1.2 mm sources down to ∼ 0.02 mJy: extragalactic background light and dust-poor, high-z galaxies. FUJIMOTO S., OUCHI M., ONO Y., et al.
2017MNRAS.469.2646C 159           X C       3 10 5 Gran Telescopio Canarias observations of an overdense region of Lyman α emitters at z = 6.5. CHANCHAIWORAWIT K., GUZMAN R., RODRIGUEZ ESPINOSA J.M., 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.
2019MNRAS.489.3294C 504       D     X C       12 19 ~ MOS spectroscopy of protocluster candidate galaxies at z = 6.5. CALVI R., RODRIGUEZ ESPINOSA J.M., MAS-HESSE J.M., et al.
2020MNRAS.495L..17R 263       D     X C       6 12 ~ An ionized superbubble powered by a protocluster at z = 6.5. RODRIGUEZ ESPINOSA J.M., MAS-HESSE J.M., SALVADOR-SOLE E., 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.
2022ApJ...926..230N 17       D               1 42 8 The Magellan M2FS Spectroscopic Survey of High-z Galaxies: Lyα Emitters at z ≃ 6.6 and the Evolution of Lyα Luminosity Function over z ≃ 5.7-6.6. NING Y., JIANG L., ZHENG Z.-Y., et al.

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