activity
19952021
most citedThe Fundamental Plane for cluster E and S0 galaxies

538 citations · 3.7k across the 47 of their papers we have counts for

collaborators

47 papers

astro-ph.GA2021★ 25 cited

Total mass density slopes of early-type galaxies using Jeans dynamical modelling at redshifts

Caro Derkenne, Richard M. McDermid, Adriano Poci +3

The change of the total mass density slope, , of early-type galaxies through cosmic time is a probe of evolutionary pathways. Hydrodynamical cosmological simulations show that a…

astro-ph.GA2020★ 7 cited

The Fundamental Plane of Massive Quiescent Galaxies at z~2

Mikkel Stockmann, Inger Jørgensen, Sune Toft +11

We examine the Fundamental Plane (FP) and mass-to-light ratio () scaling relations using the largest sample of massive quiescent galaxies at to date. The FP ($r_{e…

astro-ph.GA2019★ 44 cited

X-shooter Spectroscopy and HST Imaging of 15 Ultra Massive Quiescent Galaxies at

Mikkel Stockmann, Sune Toft, Anna Gallazzi +23

We present a detailed analysis of a large sample of spectroscopically confirmed ultra-massive quiescent galaxies () at . This sam…

astro-ph.IM2019★ 1 cited

Strategic Scientific Plan for Gemini Observatory

J. P. Blakeslee, A. Adamson, C. Davis +30

We present the Strategic Scientific Plan (SSP) for the direction and activities of the Gemini Observatory in the 2020s. The overarching goal is to ensure that Gemini best uses the…

astro-ph.IM2019

Entering into the Wide Field Adaptive Optics Era on Maunakea

Gaetano Sivo, John Blakeslee, Jennifer Lotz +32

As part of the National Science Foundation funded "Gemini in the Era of MultiMessenger Astronomy" (GEMMA) program, Gemini Observatory is developing GNAO, a widefield adaptive optic…

astro-ph.GA2019★ 3 cited

The Gemini/HST Galaxy Cluster Project: Environment Effects on the Stellar Populations in the Lynx Clusters at z=1.27

Inger Jorgensen, Laura C. Hunter, Conor R. O'Neill +4

Few detailed investigations of stellar populations in passive galaxies beyond z~1 are based on deep spectroscopic observations, due to the difficulty in obtaining such data. We pre…