[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 …
Growing supermassive black holes in the late stages of galaxy mergers are heavily obscured
Mergers of galaxies are thought to cause significant gas inflows to the inner parsecs, which
can activate rapid accretion on to supermassive black holes (SMBHs), giving rise to active …
can activate rapid accretion on to supermassive black holes (SMBHs), giving rise to active …
Galaxy and Mass Assembly (GAMA): exploring the WISE web in G12
TH Jarrett, ME Cluver, C Magoulas… - The Astrophysical …, 2017 - iopscience.iop.org
We present an analysis of the mid-infrared Wide-field Infrared Survey Explorer (WISE)
sources seen within the equatorial GAMA G12 field, located in the North Galactic Cap. Our …
sources seen within the equatorial GAMA G12 field, located in the North Galactic Cap. Our …
Polar dust, nuclear obscuration, and IR SED diversity in type-1 AGNs
Despite the hypothesized similar face-on viewing angles, the infrared emission of type-1
active galactic nuclei (AGNs) has diverse spectral energy distribution (SED) shapes that …
active galactic nuclei (AGNs) has diverse spectral energy distribution (SED) shapes that …
Extremely red quasars from SDSS, BOSS and WISE: classification of optical spectra
NP Ross, F Hamann, NL Zakamska… - Monthly Notices of …, 2015 - academic.oup.com
Quasars with extremely red infrared-to-optical colours are an interesting population that can
test ideas about quasar evolution as well as orientation, obscuration and geometric effects in …
test ideas about quasar evolution as well as orientation, obscuration and geometric effects in …
Radio and far-IR emission associated with a massive star-forming galaxy candidate at z ≃ 6.8: a radio-loud AGN in the reionization era?
R Endsley, DP Stark, X Fan, R Smit… - Monthly Notices of …, 2022 - academic.oup.com
We report the identification of radio (0.144–3 GHz) and mid-, far-infrared, and sub-mm (24–
850μm) emission at the position of one of 41 UV-bright () z≃ 6.6–6.9 Lyman-break galaxy …
850μm) emission at the position of one of 41 UV-bright () z≃ 6.6–6.9 Lyman-break galaxy …
The discovery of gas-rich, dusty starbursts in luminous reddened quasars at z ∼ 2.5 with ALMA
We present ALMA observations of cold dust and molecular gas in four high-luminosity,
heavily reddened (AV∼ 2.5–6 mag) type 1 quasars at z∼ 2.5 with virial M BH∼ 1010 M⊙ …
heavily reddened (AV∼ 2.5–6 mag) type 1 quasars at z∼ 2.5 with virial M BH∼ 1010 M⊙ …
NuSTAR observations of WISE J1036+ 0449, a galaxy at z∼ 1 obscured by hot dust
Hot dust-obscured galaxies (hot DOGs), selected from Wide-Field Infrared Survey Explorer's
all-sky infrared survey, host some of the most powerful active galactic nuclei known and may …
all-sky infrared survey, host some of the most powerful active galactic nuclei known and may …
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 …
Radio jet feedback and star formation in heavily obscured, hyperluminous quasars at redshifts∼ 0.5–3. I. ALMA observations
CJ Lonsdale, M Lacy, AE Kimball, A Blain… - The Astrophysical …, 2015 - iopscience.iop.org
ABSTRACT We present Atacama Large Millimeter/submillimeter Array (ALMA) 870 μm (345
GHz) data for 49 high-redshift (0.47< z< 2.85), luminous ($11.7\lt\mathrm {log}({L} _ {{\rm …
GHz) data for 49 high-redshift (0.47< z< 2.85), luminous ($11.7\lt\mathrm {log}({L} _ {{\rm …