All Stories

  1. Properties of LBGs with [OIII] detection at z ∼ 3.5
  2. Spatially resolved star formation and dust attenuation in Mrk 848: Comparison of the integral field spectra and the UV-to-IR SED
  3. Star formation history of the galaxy merger Mrk848 with SDSS-IV MaNGA
  4. The spectral energy distribution of galaxies atz> 2.5: Implications from theHerschel/SPIRE color–color diagram
  5. Herschel/SPIRE colors of galaxies at z>2.5