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 …

We present the results of a systematic search for candidate quiescent galaxies in the distant
universe in 11 JWST fields with publicly available observations collected during the first 3 …

We present the first results from the Mapping Obscuration to Reionization with ALMA
(MORA) survey, the largest Atacama Large Millimeter/submillimeter Array (ALMA) blank-field …

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 present the results of the first, deep Atacama Large Millimeter Array (ALMA) imaging
covering the full≃ 4.5 arcmin2 of the Hubble Ultra Deep Field (HUDF) imaged with Wide …

Aims. We present a 69 arcmin 2 ALMA survey at 1.1 mm, GOODS-ALMA, matching the
deepest HST-WFC3 H-band part of the GOODS-South field. Methods. We tapered the 0 ″24 …

We present a set of multiwavelength mosaics and photometric catalogs in the Atacama
Large Millimeter/submillimeter Array (ALMA) lensing cluster survey fields. The catalogs were …

Abstract We present Atacama Large Millimeter/submillimeter Array [C ii] 158 μm line and
underlying far-infrared (FIR) continuum emission observations (0 farcs 70× 0 farcs 56 …

Submillimeter/millimeter observations of dusty star-forming galaxies with the Atacama Large
Millimeter/submillimeter Array (ALMA) have shown that dust continuum emission generally …

Dust temperature is an important property of the interstellar medium (ISM) of galaxies. It is
required when converting (sub) millimetre broad-band flux to total infrared luminosity (L IR) …