R. Skelton

activity

20082026

most cited3D-HST+CANDELS: The Evolution of the Galaxy Size-Mass Distribution since

z = 3

1.4k citations · 11.5k across the 75 of their papers we have counts for

collaborators

Showing 2024Show all

3 papers · 1 filter

astro-ph.GA2024★ 2 cited

The $K_{s}$ -band luminosity function of the rich cluster VC04 in the Vela supercluster

N. Hatamkhani, R. C. Kraan-Korteweg, S. L. Blyth +1

To learn more about the properties of the Vela Supercluster (VSCL) located behind the Milky Way at $cz \sim 18000$ ~km~s $^{- 1}$ , we determined the $K_{s}$ -band Luminosity Function (LF)…

astro-ph.GA2024★ 1 cited

Bulge+disc decomposition of HFF and CANDELS galaxies: UVJ diagrams and stellar mass-size relations of galaxy components at $0.2 \leq z \leq 1.5$

Kalina V. Nedkova, Boris Häußler, Danilo Marchesini +13

Using deep imaging from the CANDELS and HFF surveys, we present bulge+disc decompositions with GalfitM for $\sim$ 17,000 galaxies over $0.2 \leq z \leq 1.5$ . We use various model par…

astro-ph.GA2024

The effect of cosmic web filaments on galaxy properties in the RESOLVE and ECO surveys

Munira Hoosain, Sarah-L. Blyth, Rosalind E. Skelton +6

Galaxy environment plays an important role in driving the transformation of galaxies from blue and star-forming to red and quenched. Recent works have focused on the role of cosmic…

The Ks​-band luminosity function of the rich cluster VC04 in the Vela supercluster

Bulge+disc decomposition of HFF and CANDELS galaxies: UVJ diagrams and stellar mass-size relations of galaxy components at 0.2≤z≤1.5

The effect of cosmic web filaments on galaxy properties in the RESOLVE and ECO surveys

The $K_{s}$ -band luminosity function of the rich cluster VC04 in the Vela supercluster

Bulge+disc decomposition of HFF and CANDELS galaxies: UVJ diagrams and stellar mass-size relations of galaxy components at $0.2 \leq z \leq 1.5$