We present rest-frame optical data of the compact z= 5.55 galaxy GS_3073 obtained using
the integral field spectroscopy mode of the Near-InfraRed Spectrograph on board the James …

We combine results from deep ALMA observations of massive (M*> 10 10 M⊙) galaxies at
different redshifts to show that the column density of their interstellar medium (ISM) rapidly …

We introduce a suite of 30 cosmological magneto-hydrodynamical zoom simulations of the
formation of galaxies in isolated Milky Way mass dark haloes. These were carried out with …

We present reduced data and data products from the 3D-HST survey, a 248-orbit HST
Treasury program. The survey obtained WFC3 G141 grism spectroscopy in four of the five …

Spectroscopic+ photometric redshifts, stellar mass estimates, and rest-frame colors from the
3D-HST survey are combined with structural parameter measurements from CANDELS …

We present the results of a size and structural analysis of 1395 galaxies at 0.5≤ z≲ 8 with
stellar masses log (M*/M⊙)> 9.5 within the James Webb Space Telescope Public CEERS …

ABSTRACT The 3D-HST and CANDELS programs have provided WFC3 and ACS
spectroscopy and photometry over≈ 900 arcmin 2 in five fields: AEGIS, COSMOS, GOODS …

We present the KMOS 3D survey, a new integral field survey of over 600 galaxies at 0.7< z<
2.7 using KMOS at the Very Large Telescope. The KMOS 3D survey utilizes synergies with …

Galaxy sizes and their evolution over cosmic time have been studied for decades and serve
as key tests of galaxy formation models. However, at z≳ 1 these studies have been limited …

We present the redshift evolution of the galaxy effective radius re obtained from the Hubble
Space Telescope (HST) samples of∼ 190,000 galaxies at z= 0–10. Our HST samples …