Dictionary of Nomenclature of Celestial Objects
(Last update: 19-Apr-2024)

Result of query: info cati HOO2019b] z66LAE-NN$



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Details on Acronym:   [HOO2019b]
   [HOO2019b] (Harikane+Ouchi+Ono+, 2019) Write:<<[HOO2019b] z57LAE-NN>>
<<[HOO2019b] z66LAE-NN>> N: 44+12 Object:LAE  (SIMBAD class: EmissionG = Emission-line galaxy) Stat:is completely incorporated in Simbad Note:Gemini GMOS and Keck II DEIMOS observations of N=44+12 Lyman Alpha Emitters (LAEs) in two overdensities at z=5.692 (z57OD, [HOO2019] HSC-z6PCC1) and z=6.585 (z66OD, [HOO2019] HSC-z7PCC24) respectively. in source:[HOO2019] HSC-z6PCC1 in source:[HOO2019] HSC-z7PCC24 Ref:=2019ApJ...883..142H byHARIKANE Y. , OUCHI M., ONO Y., FUJIMOTO S., DONEVSKI D., SHIBUYA T., FAISST A.L., GOTO T., HATSUKADE B., KASHIKAWA N., KOHNO K., HASHIMOTO T., HIGUCHI R., INOUE A.K., LIN Y.-T., MARTIN C.L., OVERZIER R., SMAIL I., TOSHIKAWA J., UMEHATA H., AO Y., CHAPMAN S., CLEMENTS D.L., IM M., JING Y., KAWAGUCHI T., LEE C.-H., LEE M.M., LIN L., MATSUOKA Y., MARINELLO M., NAGAO T., ONODERA M., TOFT S., WANG W.-H. Astrophys. J., 883, 142-142 (2019) SILVERRUSH. VIII. Spectroscopic identifications of early large-scale structures with protoclusters over 200 Mpc at z ~ 6-7: strong associations of dusty star-forming galaxies. oTable 1: <[HOO2019b] z57LAE-NN> (Nos 1-44). Table 2: <[HOO2019b] z66LAE-NN> (Nos 1-12). oTable 3: Not all protoclusters are in SIMBAD. Originof the Acronym: S = Created by Simbad, the CDS Database