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 …

During the first 500 million years of cosmic history, the first stars and galaxies formed,
seeding the Universe with heavy elements and eventually reionizing the intergalactic …

We investigate the evolution of galaxy gas-phase metallicity (O/H) over the range z= 0–3.3
using samples of∼ 300 galaxies at z∼ 2.3 and∼ 150 galaxies at z∼ 3.3 from the MOSDEF …

We use deep imaging from the JWST Advanced Deep Extragalactic Survey (JADES) to
study the evolution of the ionizing photon production efficiency, ξion. We estimate ξion for a …

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 Keck–MOSFIRE H and K spectra for a sample of 24 candidate quiescent
galaxies at 3< z< 4, identified from their rest-frame UVJ colors and photometric redshifts in …

Using cosmological simulations, we address the properties of high-redshift star-forming
galaxies (SFGs) across their main sequence (MS) in the plane of star formation rate (SFR) …

The VLA-COSMOS 3 GHz Large Project: Evolution of Specific Star Formation Rates out to z ∼
5 - IOPscience This site uses cookies. By continuing to use this site you agree to our use of …

We explore the connection between the UV luminosity functions (LFs) of high-z galaxies and
the distribution of stellar masses and star formation histories (SFHs) in their host dark matter …

We present a new, publicly available library of dust spectral energy distributions (SEDs).
These SEDs are characterized by only three parameters: the dust mass (M dust), the dust …