COSMOS2015 809358 , the SIMBAD biblio

COSMOS2015 809358 , the SIMBAD biblio (19 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST11:32:45

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
2015ApJ...808..139S 1509     A D S   X C       37 5 275 Evidence for PopIII-like stellar populations in the most luminous lyman-α emitters at the epoch of reionization: spectroscopic confirmation. SOBRAL D., MATTHEE J., DARVISH B., et al.
2015MNRAS.451..400M 285           X C       6 6 153 Identification of the brightest Lyα emitters at z = 6.6: implications for the evolution of the luminosity function in the reionization era. MATTHEE J., SOBRAL D., SANTOS S., et al.
2016ApJ...825L...7H 198           X         5 10 24 An ultraluminous Lyα emitter with a blue wing at z = 6.6. HU E.M., COWIE L.L., SONGAILA A., et al.
2017MNRAS.467..768R 40           X         1 7 4 A multiply imaged z ∼ 6.3 Lyman α emitter candidate behind Abell 2261. RYDBERG C.-E., ZITRIN A., ZACKRISSON E., et al.
2017ApJ...846..134J 95       D     X         3 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.
2017MNRAS.472..772M viz 135       D     X C       3 48 66 Spectroscopic properties of luminous Ly α emitters at z ~= 6-7 and comparison to the Lyman-break population. MATTHEE J., SOBRAL D., DARVISH B., et al.
2018ApJ...859...91S 136       D     X         4 12 5 Complex Lyα profiles in redshift 6.6 ultraluminous Lyα emitters. SONGAILA A., HU E.M., BARGER A.J., et al.
2018MNRAS.477.2817S viz 41           X         1 42 71 The nature of luminous Ly α emitters at z ∼ 2-3: maximal dust-poor starbursts and highly ionizing AGN. SOBRAL D., MATTHEE J., DARVISH B., et al.
2018A&A...619A.136M viz 89             C       1 7 63 Confirmation of double peaked Lyα emission at z=6.593. Witnessing a galaxy directly contributing to the reionisation of the Universe. MATTHEE J., SOBRAL D., GRONKE 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.
2019ApJ...881..124M 4103     A D S   X C       100 37 73 Resolved UV and [C II] structures of luminous galaxies within the epoch of reionization. MATTHEE J., SOBRAL D., BOOGAARD L.A., et al.
2020ApJ...896...93H 18       D               1 50 106 Large population of ALMA galaxies at z > 6 with very high [O III] 88 µm to [C II] 158 µm flux ratios: evidence of extremely high ionization parameter or PDR deficit? HARIKANE Y., OUCHI M., INOUE A.K., et al.
2021MNRAS.502.3210L 17       D               1 23 16 The IRX-β relation of high-redshift galaxies. LIANG L., FELDMANN R., HAYWARD C.C., 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.
2022ApJ...935...52S 60       D     X         2 19 2 The Evolution of Lyα Emitter Line Widths from z = 5.7 to z = 6.6. SONGAILA A., BARGER A.J., COWIE L.L., 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.
2024MNRAS.528..499L 18       D               1 192 ~ [C II] 158 μm emission as an indicator of galaxy star formation rate. LIANG L., FELDMANN R., MURRAY N., et al.
2024MNRAS.534.2062V 18       D               1 72 ~ Characterising the contribution of dust-obscured star formation at ≳ 5 using 18 serendipitously identified [C II] emitters. VAN LEEUWEN I.F., BOUWENS R.J., VAN DER WERF P.P., et al.

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