Understanding the properties of dust attenuation curves in galaxies and the physical
mechanisms that shape them are among the fundamental questions of extragalactic …

The Atacama Large Millimetre/submillimetre Array (ALMA) is currently in the process of
transforming our view of star-forming galaxies in the distant (z≳ 1) universe. Before ALMA …

Over the past decades, rest-frame ultraviolet (UV) observations have provided large
samples of UV luminous galaxies at redshift (z) greater than 6 (refs.,–), during the so-called …

Combining the public JWST/NIRCam imaging programs CEERS, PRIMER, and JADES,
spanning a total area of, we obtain a sample of 30 000 galaxies at that allows us to perform …

For the past 50 years, superconducting detectors have offered exceptional sensitivity and
speed for detecting faint electromagnetic signals in a wide range of applications. These …

Over the last few years, both Atacama Large Millimeter/submillimeter Array (ALMA) and
Spitzer observations have revealed a population of likely massive galaxies at z> 3 that was …

We measure host galaxy stellar masses for a sample of five luminous quasars at z∼ 5–7.
Using JWST/NIRCam medium-band images of nearby point-spread function reference stars …

Understanding how super-massive black holes form and grow in the early Universe has
become a major challenge, since it was discovered that luminous quasars existed only 700 …

Aims. We present the detailed characterisation of a sample of 56 sources serendipitously
detected in ALMA band 7 as part of the ALMA Large Program to INvestigate CII at Early …

We analyse the physical properties of a large, homogeneously selected sample of ALMA-
located sub-millimetre galaxies (SMGs). This survey, AS2UDS, identified 707 SMGs across …