We present the mid-infrared (MIR) morphologies for 64 star-forming galaxies (SFGs) at 0.2<
z< 2.5 with stellar mass M*> 10 9 M⊙ using James Webb Space Telescope (JWST) Mid …

We present results on the environmental dependence of the star-forming galaxy main
sequence in 11 galaxy cluster fields at 1.0< z< 1.5 from the Gemini Observations of Galaxies …

Using spatially resolved Hα emission line maps of star-forming galaxies, we study the spatial
distribution of star formation over a wide range in redshift (0.5≲ z≲ 1.7). Our z∼ 0.5 …

The MAMMOTH–Grism slitless spectroscopic survey is a Hubble Space Telescope (HST)
cycle 28 medium program, which is obtaining 45 orbits of WFC3/IR grism spectroscopy in …

We present and publicly release (www. gclasshst. com) the first spatially resolved Hα maps
of star-forming cluster galaxies at z∼ 1, made possible with the Wide Field Camera 3 …

Reconstructing the Assembly of Massive Galaxies. II. Galaxies Develop Massive and Dense
Stellar Cores as They Evolve and Head toward Quiescence at Cosmic Noon - IOPscience This …

We present the first public data release of the GOGREEN (Gemini Observations of Galaxies
in Rich Early Environments) and GCLASS (Gemini CLuster Astrophysics Spectroscopic …

Galaxy Sizes Since z = 2 from the Perspective of Stellar Mass Distribution within Galaxies -
IOPscience This site uses cookies. By continuing to use this site you agree to our use of cookies …

We present the H 160 morphological catalogs for the COSMOS-DASH survey, the largest
area near-IR survey using HST-WFC3 to date. Utilizing the" Drift And SHift" observing …

Tracing the emergence of the massive quiescent galaxy (QG) population requires the build-
up of reliable quenched samples by distinguishing these systems from red, dusty star …