Abstract We present Atacama Large Millimeter Array 1 mm observations of the rest-frame far-
infrared (FIR) dust continuum in 27 quasars at redshifts 6.0≲ z< 6.7. We detect FIR emission …

In this paper, we develop a new unsupervised machine learning technique comprised of a
feature extractor, a convolutional autoencoder, and a clustering algorithm consisting of a …

We resolve the host galaxies of seven gravitationally lensed quasars at redshift 1.5–2.8
using observations with the Atacama Large (sub) Millimetre Array. Using a visibility plane …

Recent studies have suggested that red quasars are a phase in quasar evolution when
feedback from black hole accretion evacuates obscuring gas from the nucleus of the host …

Dusty star-forming galaxies (DSFGs) at redshift z≥ 1 are among the most vigorously star-
forming galaxies in the Universe. However, their dense (≥ 10 5 cm− 3) gas phase–typically …

We investigate the merging rates of compact binaries in galaxies and the related detection
rate of gravitational wave (GW) events with AdvLIGO/Virgo and with the Einstein Telescope …

It is widely assumed that long-wavelength infrared (IR) emission from cold dust (T∼ 20–40
K) is a reliable tracer of star formation even in the presence of a bright active galactic …

A Survey of Atomic Carbon [C i] in High-redshift Main-sequence Galaxies - IOPscience This
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In this paper, we study the impact of different galaxy statistics and empirical metallicity
scaling relations on the merging rates and properties of compact object binaries. Firstly, we …

We present the discovery of a gravitationally lensed dust-reddened QSO at z= 2.517,
identified in a survey for QSOs by infrared selection. Hubble Space Telescope imaging …