lbg s at z~5 k. ohta (kyoto univ.) with i. iwata (naoj, okayama) m. ando (kyoto univ.) m. akiyama...
Post on 19-Dec-2015
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LBG s at z~5
K. Ohta (Kyoto Univ.)
with
I. Iwata (NAOJ, Okayama)
M. Ando (Kyoto Univ.)
M. Akiyama (NAOJ, Subaru)
N. Tamura (Durham, UK)
K. Aoki (NAOJ, Subaru)
•LBG search at GOODS-N and J0053+1234
fields
•V, I_c, z’ ; z~5 with S-Cam/Subaru
•Highest redshift achieved with two-color
diagram using standard filter system
•Age of 1Gyr and 1Gyr earlier from z~3
•Number density of luminous LBGs does not change so much from z=5 to 3
•Fainter LBGs increase at the later epoch
•Luminosity-dependent evolution?
However….
•Disagreement among UVLFs at z~4, 5
in a luminous part
Downsizing of LBGs?•Number density of luminous LBGs does not
change so much from z=5 to 3
•Fainter LBGs at z~3 are late comers?
•Luminous z~5 LBGs in dusty environment?
chemically evolved to some degree?
=> lack of blue luminous ones?
•Luminous z~5 LBGs show larger clustering amp.
luminous LBGs reside in massive DHs?
=> SF started eariler?