Details on Acronym: [SON2014] | |
[SON2014] | (Shibuya+Ouchi+Nakajima+, 2014) |
Write: | <<[SON2014] COSMOS NNNNN>> <<[SON2014] HDFN1 20042>> <<[SON2014] HDFN2 NNNNN>> <<[SON2014] COSMOS3B NNNNN>> <<[SON2014] HUDF maB NNNNN>> <<[SON2014] SXDS495B NNNNN>> |
N: | 7+1+3+7+2+4 |
Object: | LAE (SIMBAD class: EmissionG = Emission-line galaxy) |
Note: | Keck I LRIS and Subaru FMOS observations of N=7+1+3+7+2+4 Lyα emitters. |
in source: | NAME COSMOS Field |
in source: | NAME HDFN |
in source: | NAME HUDF |
in source: | NAME SXDF |
Ref: | =2014ApJ...788...74S |
by | SHIBUYA T. , OUCHI M., NAKAJIMA K., HASHIMOTO T., ONO Y., RAUCH M., GAUTHIER J.-R., SHIMASAKU K., GOTO R., MORI M., UMEMURA M. |
Astrophys. J., 788, 74 (2014) | |
What is the physical origin of strong Lyα emission? II. Gas kinematics and distribution of Lyα emitters. | |
o | Table 2: <[SON2014] COSMOS NNNNN> N=7, <[SON2014] HDFN1 20042> N=1, <[SON2014] HDFN2 NNNNN> N=3, <[SON2014] COSMOS3B NNNNN> N=7, <[SON2014] HUDF maB NNNNN> N=2, <[SON2014] SXDS495B NNNNN> N=4. |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |