activity
20072017
most citedThe relation between galaxy morphology and colour in the EAGLE simulation

99 citations · 313 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2017★ 90 cited

The three phases of galaxy formation

Bart Clauwens, Joop Schaye, Marijn Franx +1

We investigate the origin of the Hubble sequence by analysing the evolution of the kinematic morphologies of central galaxies in the EAGLE cosmological simulation. By separating ea…

astro-ph.GA2017★ 4 cited

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…

astro-ph.GA2017★ 99 cited

The relation between galaxy morphology and colour in the EAGLE simulation

Camila A. Correa, Joop Schaye, Bart Clauwens +5

We investigate the relation between kinematic morphology, intrinsic colour and stellar mass of galaxies in the EAGLE cosmological hydrodynamical simulation. We calculate the intrin…

astro-ph.GA2017★ 57 cited

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 $…

astro-ph.GA2016★ 19 cited

A large difference in the progenitor masses of active and passive galaxies in the EAGLE simulation

Bart Clauwens, Marijn Franx, Joop Schaye

Cumulative number density matching of galaxies is a method to observationally connect descendent galaxies to their typical main progenitors at higher redshifts and thereby to asses…

astro-ph.GA2016★ 26 cited

Implications of a variable IMF for the interpretation of observations of galaxy populations

Bart Clauwens, Joop Schaye, Marijn Franx

We investigate the effect of a metallicity-dependent stellar initial mass function (IMF), as deduced observationally by Martin-Navarro et al. (2015c), on the inferred stellar masse…

astro-ph.GA2014★ 11 cited

An assessment of the evidence from ATLAS3D for a variable initial mass function

Bart Clauwens, Joop Schaye, Marijn Franx

The ATLAS3D Survey has reported evidence for a non-universal stellar initial mass function (IMF) for early type galaxies (ETGs) (Cappellari et al. 2012, 2013b,a). The IMF was const…

hep-ph2007★ 7 cited

D-term inflation after spontaneous symmetry breaking

Bart Clauwens, Rachel Jeannerot

We show that 1-loop quantum corrections to the potential energy density in supersymmetric hybrid inflation, outside the inflationary valley, can not be neglected. A method is prese…