Dictionary of Nomenclature of Celestial Objects
(Last update: 26-Sep-2023)

Result of query: info cati HOO2019b]$

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