COSMOS2015 604211 , the SIMBAD biblio

COSMOS2015 604211 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST11:10:16


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Title First 3 Authors
2009ApJ...696..546S viz 15       D               1 86 28 Photometric properties of Lyα emitters at z∼4.86 in the COSMOS 2 square degree field. SHIOYA Y., TANIGUCHI Y., SASAKI S.S., et al.
2012ApJ...760..128M viz 15       D               1 235 51 Lyα emission from high-redshift sources in COSMOS. MALLERY R.P., MOBASHER B., CAPAK P., et al.
2015ApJ...815...57U viz 16       D               1 306 7 A correlation between Lyα spectral line profile and rest-frame UV morphology. U V., HEMMATI S., DARVISH B., et al.
2016ApJ...819...25K 94       D         F     2 63 9 Morphological properties of Lyα emitters at redshift 4.86 in the cosmos field: clumpy star formation or merger? KOBAYASHI M.A.R., MURATA K.L., KOEKEMOER A.M., et al.
2018ApJ...858...77H viz 16       D               1 7945 125 The DEIMOS 10k spectroscopic survey catalog of the COSMOS field. HASINGER G., CAPAK P., SALVATO M., 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.
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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