Haruka Kusakabe

Bright and Faint Ends of Ly

We present the Lya luminosity functions (LFs) derived by our deep Subaru narrowband survey that identifies a total of 3,137 Lya emitters (LAEs) at

\alpha

z = 2.2

Luminosity Functions at

in five independent blank fields. The sample of these LAEs is the largest, to date, and covers a very wide Lya luminosity range of

\textit{z} = 2

\log L_{Ly\alpha} = 41.7-44.4

Determined by the Subaru Survey: Implications for AGN, Magnification Bias, and ISM HI Evolution

erg s

A Hard Ionizing Spectrum in z=3-4 Ly-alpha Emitters with Intense [OIII] Emission: Analogs of Galaxies in the Reionization Era?

^{-1}

SILVERRUSH. III. Deep optical and near-infrared spectroscopy for Ly alpha and UV-nebular lines of bright Ly alpha emitters at z=6-7

. We determine the Lya LF at

First Infrared-Based Implications for the Dust Attenuation and Star Formation of Typical Lyα Emitters

z = 2.2

SILVERRUSH. II. First catalogs and properties of ∼2000 Lyα emitters and blobs at z ∼ 6–7 identified over the 14–21 deg2 sky*

with unprecedented accuracies, and obtain the best-fit Schechter parameters of

SILVERRUSH. IV. Lyα luminosity functions at z = 5.7 and 6.6 studied with ∼1300 Lyα emitters on the 14–21 deg2 sky

L^{*}_{Ly\alpha} = 5.29^{+1.67}_{-1.13} \times 10^{42}