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Query : 2014ApJ...785...64S |
2014ApJ...785...64S - Astrophys. J., 785, 64 (2014/April-2)
What is the physical origin of strong Lyα emission? I. Demographics of Lyα emitter structures.
SHIBUYA T., OUCHI M., NAKAJIMA K., YUMA S., HASHIMOTO T., SHIMASAKU K., MORI M. and UMEMURA M.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): cosmology: observations - early universe - galaxies: formation - galaxies: high-redshift
Simbad objects: 5
Number of rows : 5 |
N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2024 |
#notes |
---|---|---|---|---|---|---|---|---|---|---|---|---|
1 | NAME Himiko | EmG | 02 17 57.6122 | -05 08 44.898 | ~ | 102 | 0 | |||||
2 | NAME Chandra Deep Field-South | reg | 03 32 28.0 | -27 48 30 | ~ | 2088 | 1 | |||||
3 | NAME COSMOS Field | reg | 10 00 28.60 | +02 12 21.0 | ~ | 2975 | 0 | |||||
4 | NAME Hubble Deep Field | reg | 12 36 49.5 | +62 12 58 | ~ | 1922 | 1 | |||||
5 | SSA 22 | reg | 22 17 34.7 | +00 15 07 | ~ | 326 | 0 |
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