34 papers found
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CHORUS. III. Photometric and Spectroscopic Properties of Lyα Blobs at z = 4.9–7.0
The Lyman Continuum Escape Survey. II. Ionizing Radiation as a Function of the [O iii]/[O ii] Line Ratio
The Lyman Continuum Escape Survey: Ionizing Radiation from [O iii]-strong Sources at a Redshift of 3.1
The dominant origin of diffuse Lyα halos around Lyα emitters explored by spectral energy distribution fitting and clustering analysis
Morphologies of ∼190,000 Galaxies at z = 0–10 Revealed with HST Legacy Data. III. Continuum Profile and Size Evolution of Lyα Emitters
The mean ultraviolet spectrum of a representative sample of faint z ∼ 3 Lyman alpha emitters
The dominant origin of diffuse Ly$α$ halos around LAEs explored by SED fitting and clustering analysis
The stellar mass, star formation rate and dark matter halo properties of LAEs at z ∼ 2
SILVERRUSH. IV. Lyα luminosity functions at z = 5.7 and 6.6 studied with ∼1300 Lyα emitters on the 14–21 deg2 sky
SILVERRUSH. II. First catalogs and properties of ∼2000 Lyα emitters and blobs at z ∼ 6–7 identified over the 14–21 deg2 sky*
A Spectroscopic Search for AGN Activity in the Reionization Era
SILVERRUSH. III. Deep optical and near-infrared spectroscopy for Lyα and UV-nebular lines of bright Lyα emitters at z = 6–7†‡
Great Optically Luminous Dropout Research Using Subaru HSC (GOLDRUSH). I. UV luminosity functions at z ∼ 4–7 derived with the half-million dropouts on the 100 deg2 sky†
Systematic Identification of LAEs for Visible Exploration and Reionization Research Using Subaru HSC (SILVERRUSH). I. Program strategy and clustering properties of ∼2000 Lyα emitters at z = 6–7 over the 0.3–0.5 Gpc2 survey area†
Evolution of N/O abundance ratios and ionization parameters from z ∼ 0 to 2 investigated by the direct temperature method*†
Lyα emitters with very large Lyα equivalent widths, EW0(Lyα) ≃ 200–400 Å, atz∼ 2
A HARD IONIZING SPECTRUM IN Z = 3–4 Ly α EMITTERS WITH INTENSE $[{\Rm{O}}\,{\rm{III}}]$ EMISSION: ANALOGS OF GALAXIES IN THE REIONIZATION ERA?
BRIGHT AND FAINT ENDS OF LyαLUMINOSITY FUNCTIONS ATz= 2 DETERMINED BY THE SUBARU SURVEY: IMPLICATIONS FOR AGNs, MAGNIFICATION BIAS, AND ISM H I EVOLUTION
Statistical properties of diffuse Lyα haloes around star-forming galaxies atz∼ 2
A CLOSE COMPARISON BETWEEN OBSERVED AND MODELED LyαLINES FORz∼ 2.2 LyαEMITTERS
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