Environment is one of the primary drivers of galaxy evolution; via multiple mechanisms, it
can control the critical process of transforming galaxies from star forming to quiescent …

Context. Sources at the brightest end of the quasi-stellar object (QSO) luminosity function,
during the peak epoch in the history of star formation and black hole accretion (z∼ 2− 4 …

We report the identification of Lyman break galaxy (LBG) candidates around the most
luminous hot dust-Obscured galaxy (Hot DOG) known, WISE J224607. 56− 052634.9 …

Submillimetre galaxies represent a rapid growth phase of both star formation and massive
galaxies. Mapping SMGs in galaxy protoclusters provides key insights into where and how …

We have been undertaking a systematic survey at 850 μm based on a sample of four
prototypical z∼ 2− 3 enormous Lyα nebulae (ELANe) as well as their megaparsec-scale …

Hot, dust-obscured galaxies (Hot DOGs) are a population of hyper-luminous obscured
quasars identified by WISE. We present ALMA observations of the [C II] 158 μm fine …

We report the results of the deep and wide Atacama Large Millimeter/submillimeter Array
(ALMA) 1.2 mm mapping of the Spiderweb protocluster at z= 2.16. The observations were …

We study the environmental effect of galaxy evolution as a function of the underlying three-
dimensional dark matter density for the first time at–2.5, in which the underlying matter …

Abstract Wide-field Infrared Survey Explorer all-sky survey has discovered a new population
of hot dust-obscured galaxies (Hot DOGs), which have been confirmed to be dusty quasars …

We present a UV to millimeter spectral energy distribution (SED) analysis of 16
hyperluminous, dust-obscured quasars at z∼ 3, selected by the Wide-field Infrared Survey …