[HTML][HTML] From clusters to proto-clusters: the infrared perspective on environmental galaxy evolution
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 …
can control the critical process of transforming galaxies from star forming to quiescent …
An overdensity of Lyman break galaxies around the hot dust-obscured galaxy WISE J224607. 56− 052634.9
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 …
luminous hot dust-Obscured galaxy (Hot DOG) known, WISE J224607. 56− 052634.9 …
Kinematics and star formation of high-redshift hot dust-obscured quasars as seen by ALMA
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 …
quasars identified by WISE. We present ALMA observations of the [C II] 158 μm fine …
Radio Spectra of Luminous, Heavily Obscured WISE-NVSS Selected Quasars
We present radio spectra spanning 0.1–10 GHz for the sample of heavily obscured luminous
quasars with extremely red mid-infrared-optical colors and compact radio emission. The …
quasars with extremely red mid-infrared-optical colors and compact radio emission. The …
Physical Properties of Hyperluminous, Dust-obscured Quasars at z∼ 3: Multiwavelength Spectral Energy Distribution Analysis and Cold Gas Content Revealed by …
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 …
hyperluminous, dust-obscured quasars at z∼ 3, selected by the Wide-field Infrared Survey …
Cold molecular gas and free–free emission from hot, dust-obscured galaxies at z∼ 3
JI Penney, AW Blain, RJ Assef… - Monthly Notices of …, 2020 - academic.oup.com
We report on observations of redshifted CO (1–0) line emission and observed-frame GHz
radio continuum emission from five ultra-luminous, mid-IR selected hot, Dust-Obscured …
radio continuum emission from five ultra-luminous, mid-IR selected hot, Dust-Obscured …
Unveiling the weak radio quasar population at
K Perger, S Frey, KÉ Gabányi… - Monthly Notices of the …, 2019 - academic.oup.com
We applied image stacking on empty field Faint Images of the Radio Sky at Twenty-
Centimeters (FIRST) survey maps centred on optically identified high-redshift quasars at to …
Centimeters (FIRST) survey maps centred on optically identified high-redshift quasars at to …
A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). VI. Distant Filamentary Structures Pointed Out by High-z Radio Galaxies at z∼ 4
H Uchiyama, T Yamashita, J Toshikawa… - The Astrophysical …, 2022 - iopscience.iop.org
We present the environmental properties around high-z radio galaxies (HzRGs) at z∼ 4,
which have been poorly investigated because of their rarity. We use the largest samples of …
which have been poorly investigated because of their rarity. We use the largest samples of …
Connecting the growth of galaxies to the large-scale environment in a massive node of the Cosmic Web at z~ 3
M Galbiati, S Cantalupo, C Steidel… - arXiv preprint arXiv …, 2024 - arxiv.org
A direct link between large-scale environment and galaxy properties is very well established
in the local universe. However, very little is known about the role of the environment for …
in the local universe. However, very little is known about the role of the environment for …
Black Hole Mass and Eddington Ratio Distribution of Hot Dust-Obscured Galaxies
Hot Dust-Obscured Galaxies (Hot DOGs) are a rare population of hyper-luminous infrared
galaxies discovered by the WISE mission. Despite the significant obscuration of the AGN by …
galaxies discovered by the WISE mission. Despite the significant obscuration of the AGN by …