Studying the spectral properties of Active Galactic Nuclei in the JWST era

Studying the stochasticity in astrophysical signals

Studying the Warm-Hot Intergalactic Medium in Emission

Studying the WHIM Content of the Galaxy Large-Scale Structures along the Line of Sight to H 2356-309

Studying the WHIM with Gamma Ray Bursts

Studying X-ray reprocessing and continuum variability in quasars: PG 1211+143

Sub-arcsecond radio continuum mapping in and around the spiral galaxy NGC3351 using MERLIN

Sub-millimeter brightness of early star-forming galaxies

Sub-millimeter Detected z~2 Radio-quiet QSOs: Accurate Redshifts, Black Hole Masses, and Inflow/Outflow Velocities

Sub-millimeter to centimeter excess emission from the Magellanic Clouds. I. Global spectral energy distribution

Sub-millimetre galaxies reside in dark matter halos with masses greater than 3x10^11 solar masses

Sub-parsec supermassive Binary Quasars: expectations at z<1

Subaru and Gemini High Spatial Resolution Infrared 18 Micron Imaging Observations of Nearby Luminous Infrared Galaxies

Subaru FOCAS Spectroscopic Observations of High-Redshift Supernovae

Subaru FOCAS survey of z=7-7.1 Lyα emitters: a test for z >~ 7 Lyα photometric luminosity functions

Subaru Mid-infrared Imaging of the Quadruple Lenses. II. Unveiling Lens Structure of MG0414+0534 and Q2237+030

Subaru Spectroscopy of SDSS-II Supernovae

Subaru Studies of the Cosmic Dawn

Subaru Weak Lensing Measurements of Four Strong Lensing Clusters: Are Lensing Clusters Over-Concentrated?

Subaru weak-lensing study of A2163: bimodal mass structure