activity
20152026
most citedSlicing COSMOS with SC4K: the evolution of typical Lya emitters and the Lya escape fraction from z~2 to z~6

123 citations · 987 across the 26 of their papers we have counts for

collaborators
Showing 2018Show all

5 papers · 1 filter

astro-ph.GA2018★ 39 cited

The clustering of typical Ly emitters from : host halo masses depend on Ly and UV luminosities

Ali Ahmad Khostovan, David Sobral, Bahram Mobasher +7

We investigate the clustering and halo properties of Ly-selected emission line galaxies (LAEs) from the Slicing COSMOS 4K (SC4K) and from archival NB497 imaging of S…

astro-ph.GA2018★ 108 cited

The Large Early Galaxy Astrophysics Census (LEGA-C) Data Release II: dynamical and stellar population properties of z ~< 1 galaxies in the COSMOS field

Caroline M. S. Straatman, Arjen van der Wel, Rachel Bezanson +18

We present the second data release of the Large Early Galaxy Astrophysics Census (LEGA-C), an ESO 130-night public spectroscopic survey conducted with VIMOS on the Very Large Teles…

astro-ph.GA2018★ 55 cited

SFHs OF Galaxies in LEGA-C

Priscilla Chauke, Arjen van der Wel, Camilla Pacifici +17

Using high resolution spectra from the VLT LEGA-C program, we reconstruct the star formation histories (SFHs) of 607 galaxies at redshifts and stellar masses $\gtrsim…

astro-ph.GA2018★ 84 cited

Spatially Resolved Stellar Kinematics from LEGA-C: Increased Rotational Support in z~0.8 Quiescent Galaxies

Rachel Bezanson, Arjen van der Wel, Camilla Pacifici +18

We present stellar rotation curves and velocity dispersion profiles for 104 quiescent galaxies at from the Large Early Galaxy Astrophysics Census (LEGA-C) spectroscopic s…

astro-ph.GA2018★ 62 cited

Stellar Populations of over one thousand Galaxies from LEGA-C: Ages and Star Formation Histories from D4000 and H

Po-Feng Wu, Arjen van der Wel, Anna Gallazzi +18

Drawing from the LEGA-C dataset, we present the spectroscopic view of the stellar population across a large volume- and mass-selected sample of galaxies at large lookback time. We…