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 …

What are the faintest distant galaxies we can see with the Hubble Space Telescope (HST)
now, before the launch of the James Webb Space Telescope? This is the challenge taken …

We measure the stellar mass function (SMF) and stellar mass density of galaxies in the
COSMOS field up to z~ 6. We select them in the near-IR bands of the COSMOS2015 …

We present a robust measurement and analysis of the rest-frame ultraviolet (UV) luminosity
functions at z= 4–8. We use deep Hubble Space Telescope imaging over the Cosmic …

This paper describes the Hubble Space Telescope imaging data products and data
reduction procedures for the Cosmic Assembly Near-infrared Deep Extragalactic Legacy …

We present new measurements of the evolution of the X-ray luminosity functions (XLFs) of
unabsorbed and absorbed active galactic nuclei (AGNs) out to z∼ 5. We construct samples …

Using a compilation of 25 studies from the literature, we investigate the evolution of the star-
forming galaxy (SFG) main sequence (MS) in stellar mass and star formation rate (SFR) out …

We present results from the deepest Herschel-Photodetector Array Camera and
Spectrometer (PACS) far-infrared blank field extragalactic survey, obtained by combining …

We describe a new program for determining photometric redshifts, dubbed EAZY. The
program is optimized for cases where spectroscopic redshifts are not available, or are only …

We present X-ray source catalogs for the≈ 7 Ms exposure of the Chandra Deep Field-South
(CDF-S), which covers a total area of 484.2 arcmin 2. Utilizing wavdetect for initial source …