activity
20062008
most citedDifferential Evolution of the UV Luminosity Function of Lyman Break Galaxies from z~5 to 3

79 citations · 158 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph2008

Evolution of Star-forming Galaxies seen from Lyman Break Galaxies at

K. Ohta, K. Yabe, I. Iwata +4

Properties of Lyman Break Galaxies at are presented and are compared with those at LBGs to see evolution of LBGs from to . The LBGs at $z\s…

astro-ph2008

The Stellar Populations of Lyman Break Galaxies at

Kiyoto Yabe, Kouji Ohta, Ikuru Iwata +4

We present the results of Spectral Energy Distribution (SED) fitting analysis for Lyman Break Galaxies (LBGs) at in the GOODS-N and its flanking fields. From the SED fitti…

astro-ph2008

Differential Evolution of Lyman Break Galaxies from =5 to 3

Ikuru Iwata, Kouji Ohta, Marcin Sawicki +3

We briefly summarize our findings from the unbiased surveys for 5 LBGs based on Subaru/Suprime-Cam and follow-up optical spectroscopy.

astro-ph200779 cited

Differential Evolution of the UV Luminosity Function of Lyman Break Galaxies from z~5 to 3

I. Iwata, K. Ohta, N. Tamura +5

(abridged) We report the UV luminosity function (LF) of Lyman break galaxies at z~5 derived from a deep and wide survey using the Subaru/Suprime-Cam. Target fields consist of two b…

astro-ph2006

Balmer Absorption Lines in FeLoBALs

K. Aoki, I. Iwata, K. Ohta +5

We discovered non-stellar Balmer absorption lines in two many-narrow-trough FeLoBALs (mntBALs) by the near-infrared spectroscopy with Subaru/CISCO. Presence of the non-stellar Balm…

astro-ph2006

The Long Faint Tail of the High-Redshift Galaxy Population

Marcin Sawicki, Ikuru Iwata, Kouji Ohta +6

We study the properties of very faint, sub-L* Lyman break galaxies at z~2-5 - thus far a largely neglected but numerically and energetically very important population. We find that…