1.9k citations · 2.6k across the 12 of their papers we have counts for
24 papers
A more probable explanation for a continuum flash in the direction of a redshift 11 galaxy
Charles L. Steinhardt, Michael I. Andersen, Gabriel B. Brammer +5
Recent work reported the discovery of a gamma-ray burst (GRB) associated with the galaxy GN-z11 at . The extreme improbability of the transient source being a GRB in the…
Spatially Resolved Star Formation and Inside-out Quenching in the TNG50 Simulation and 3D-HST Observations
Erica J. Nelson, Sandro Tacchella, Benedikt Diemer +21
We compare the star forming main sequence (SFMS) -- both integrated and resolved on 1kpc scales -- between the high-resolution TNG50 simulation of IllustrisTNG and observations fro…
A Comparison of Rest-frame Ultraviolet and Optical Emission-Line Diagnostics in the Lensed Galaxy SDSS J1723+3411 at Redshift z=1.3293
J. R. Rigby, Michael Florian, A. Acharyya +13
For the extremely bright lensed galaxy SDSS J1723+3411 at z=1.3293 , we analyze spatially integrated MMT, Keck, and Hubble Space Telescope spectra that fully cover the rest-frame w…
The kinematics of massive quiescent galaxies at : dark matter fractions, IMF variation, and the relation to local early-type galaxies
J. Trevor Mendel, Alessandra Beifiori, Roberto Saglia +10
We study the dynamical properties of massive quiescent galaxies at using deep Hubble Space Telescope WFC3/F160W imaging and a combination of literature stellar velo…
HST/WFC3 grism observations of clusters: evidence for evolution in the mass-size relation of quiescent galaxies from poststarburst galaxies
Jasleen Matharu, Adam Muzzin, Gabriel B. Brammer +10
Minor mergers have been proposed as the driving mechanism for the size growth of quiescent galaxies with decreasing redshift. The process whereby large star-forming galaxies quench…
The KMOS^3D Survey: data release and final survey paper
E. Wisnioski, N. M. Förster Schreiber, M. Fossati +28
We present the completed KMOS survey an integral field spectroscopic survey of 739, , galaxies at using the K-band Multi…