COSMOS2015 472215 , the SIMBAD biblio

COSMOS2015 472215 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.20CEST06:09:47


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Title First 3 Authors
2007ApJS..172..523M viz 15       D               121 97 Lyα emitters at redshift 5.7 in the COSMOS field. MURAYAMA T., TANIGUCHI Y., SCOVILLE N.Z., et al.
2009ApJ...701..915T 15       D               2 127 18 Hubble space Telescope/Advanced camera for surveys morphology of Lyα emitters at redshift 5.7 in the COSMOS field. TANIGUCHI Y., MURAYAMA T., SCOVILLE N.Z., 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.
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.
2020ApJ...903....4N viz 17       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.
2020A&A...643A...2B viz 18       D               1 124 139 The ALPINE-ALMA [CII] survey: Data processing, catalogs, and statistical source properties. BETHERMIN M., FUDAMOTO Y., GINOLFI M., et al.
2020A&A...643A...4F viz 17       D               1 117 75 The ALPINE-ALMA [CII] survey. Dust attenuation properties and obscured star formation at z ∼ 4.4-5.8. FUDAMOTO Y., OESCH P.A., FAISST A., 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.
2022A&A...660A..14R 31 7 The ALPINE-ALMA [CII] survey: The population of [CII]-undetected galaxies and their role in the L[CII]-SFR relation. ROMANO M., MORSELLI L., CASSATA P., et al.

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