Over the past decade, increasingly robust estimates of the dense molecular gas content in
galaxy populations between redshift z= 0 and the peak of cosmic galaxy/star formation (z∼ …

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 …

JWST has revolutionized the field of extragalactic astronomy with its sensitive and high-
resolution infrared view of the distant Universe. Adding to the new legacy of JWST …

We make use of sensitive (9.3 μJy beam− 1 rms) 1.2 mm continuum observations from the
Atacama Large Millimeter/submillimeter Array (ALMA) Spectroscopic Survey in the Hubble …

We present the MUSE Hubble Ultra Deep Survey, a mosaic of nine MUSE fields covering
90% of the entire HUDF region with a 10-h deep exposure time, plus a deeper 31-h …

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 a search for extremely red, dust-obscured, z> 7 galaxies with JWST/NIRCam+
MIRI imaging over the first 20 arcmin 2 of publicly available Cycle 1 data from the COSMOS …

We present ALMA Band 9 observations of the [C ii] 158 m emission for a sample of 10 main-
sequence galaxies at redshift∼ 2, with typical stellar masses (log M⋆/M⊙∼ 10.0–10.9) and …

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 …