We present the survey design, implementation, and outlook for COSMOS-Web, a 255 hr
treasury program conducted by the James Webb Space Telescope in its first cycle of …

We present a multiwavelength analysis using the Submillimeter Array (SMA), James Clerk
Maxwell Telescope, NOEMA, JWST, the Hubble Space Telescope (HST), and the Spitzer …

We present the characteristics of 2 mm selected sources from the largest Atacama Large
Millimeter/submillimeter Array (ALMA) blank-field contiguous survey conducted to date, the …

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

We present band 6 ALMA observations of a heavily obscured radio-loud (L 1.4 GHz= 1025.4
W Hz− 1) active galactic nucleus (AGN) candidate at z phot= 6.83±0.06 found in the 1.5 …

Abstract The 2 mm Mapping Obscuration to Reionization with ALMA (MORA) Survey was
designed to detect high-redshift (z≳ 4), massive, dusty star-forming galaxies (DSFGs). Here …

We report the serendipitous detection of two 3 mm continuum sources found in deep ALMA
Band 3 observations to study intermediate-redshift galaxies in the COSMOS field. One is …

Matching the number counts of high-z submillimetre-selected galaxies (SMGs) has been a
long-standing problem for galaxy formation models. In this paper, we use 3D dust radiative …

Some recent literature has claimed there to be an evolution in galaxies' dust temperatures
toward warmer (or colder) spectral energy distributions (SEDs) between low and high …

We present an ALMA-Herschel joint analysis of sources detected by the ALMA Lensing
Cluster Survey (ALCS) at 1.15 mm. Herschel/PACS and SPIRE data at 100–500 μm are …