57 citations · 189 across the 10 of their papers we have counts for
10 papers
High Redshift Massive Quiescent Galaxies are as Flat as Star Forming Galaxies: The Flattening of Galaxies and the Correlation with Structural Properties in CANDELS/3D-HST
Allison R. Hill, Arjen van der Wel, Marijn Franx +5
We investigate the median flattening of galaxies at in all five CANDELS/3D-HST fields via the apparent axis ratio . We separate the sample into bins of redshift, ste…
The Mass Growth and Stellar Ages of Galaxies: Observations versus Simulations
Allison R. Hill, Adam Muzzin, Marijn Franx +1
Using observed stellar mass functions out to , we measure the main progenitor stellar mass growth of descendant galaxies with masses of $\log{M_{*}/M_{\odot}}=11.5,11.0,10.5,1…
The average structural evolution of massive galaxies can be reliably estimated using cumulative galaxy number densities
Bart Clauwens, Allison Hill, Marijn Franx +1
Galaxy evolution can be studied observationally by linking progenitor and descendant galaxies through an evolving cumulative number density selection. This procedure can reproduce…
The mass, colour, and structural evolution of today's massive galaxies since z~5
Allison R. Hill, Adam Muzzin, Marijn Franx +12
In this paper, we use stacking analysis to trace the mass-growth, colour evolution, and structural evolution of present-day massive galaxies () out to $…
The evolution in the stellar mass of Brightest Cluster Galaxies over the past 10 billion years
Sabine Bellstedt, Chris Lidman, Adam Muzzin +14
Using a sample of 98 galaxy clusters recently imaged in the near infra-red with the ESO NTT, WIYN and WHT telescopes, supplemented with 33 clusters from the ESO archive, we measure…
Stellar Velocity Dispersion for a Strongly-Lensed, Intermediate-Mass Quiescent Galaxy at z=2.8
Allison R. Hill, Adam Muzzin, Marijn Franx +1
Measuring stellar velocity dispersions of quiescent galaxies beyond is observationally challenging. Such measurements require near-infrared spectra with a continuum detect…