HSCS J100153+020459 , the SIMBAD biblio

HSCS J100153+020459 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST06:50:00


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Title First 3 Authors
2014MNRAS.440.2810B viz 17       D               1 40 174 The bright end of the galaxy luminosity function at z ≃ 7: before the onset of mass quenching ? BOWLER R.A.A., DUNLOP J.S., McLURE R.J., et al.
2017ApJ...842L..22Z 4 12 114 First results from the Lyman Alpha Galaxies in the epoch of reionization (LAGER) survey: cosmological reionization at z ∼ 7. ZHENG Z.-Y., WANG J., RHOADS J., et al.
2017ApJ...845L..16H 414       D     X C       10 8 21 First spectroscopic confirmations of z ∼ 7.0 Lyα emitting galaxies in the LAGER survey. HU W., WANG J., ZHENG Z.-Y., et al.
2018ApJ...867...46I 177       D     X C       4 37 14 CHORUS. II. Subaru/HSC determination of the Lyα luminosity function at z = 7.0: constraints on Cosmic reionization model parameter. ITOH R., OUCHI M., ZHANG H., et al.
2019ApJ...886...90H 47           X         1 7 43 The Lyα luminosity function and cosmic Reionization at z ∼ 7.0: a tale of two LAGER fields. HU W., WANG J., ZHENG Z.-Y., et al.
2021MNRAS.500.5229E 18       D               1 103 111 The [O III]+H β equivalent width distribution at z ≃ 7: implications for the contribution of galaxies to reionization. ENDSLEY R., STARK D.P., CHEVALLARD J., 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.
2023MNRAS.519.5859W 105       D         F     3 36 43 Star formation histories of UV-luminous galaxies at z ≃ 6.8: implications for stellar mass assembly at early cosmic times. WHITLER L., STARK D.P., ENDSLEY R., et al.

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